text:
Cabinet Kohl III
This article covers the Federal Cabinet from 1987–1991. For the state cabinet of Rhineland-Palatinate from 1975–1976 see Cabinet Kohl III (Rhineland-Palatinate)
16. Cabinet of the Federal Republic of Germany
Helmut Kohl
Legislative period
Federal President Richard von Weizsäcker
3 years and 312 days
Cabinet Kohl II
Cabinet Kohl IV
Party (s)
CDU / CSU, FDP
German Bundestag
Opposition leader
Hans-Jochen Vogel ( SPD )
1 cabinet
Cabinet Kohl III - March 12, 1987 to December 20, 1990
( charged with running the business until January 18, 1991 )
Parliamentary State Secretary
or Minister of State
(1930-2017) CDU - -
Deputy Federal Chancellor
Hans-Dietrich Genscher
(1927-2016) FDP
Foreign Irmgard Adam-Schwaetzer
(* 1933) FDP
Friedrich Zimmermann
until April 21, 1989 CSU Horst Waffenschmidt
Carl-Dieter Spranger
(* 1939) CDU
Wolfgang Schäuble
from April 21, 1989 CDU
Hans A. Engelhard
(1934-2008) FDP Friedrich-Adolf Jahn
(1935-2016) CDU
Gerhard Stoltenberg
until April 21, 1989 CDU Hansjörg Häfele
until April 21, 1989
Manfred Carstens
Friedrich Voss
(1931–2012) CDU
Theodor Waigel
from April 21, 1989 CSU
Martin Bangemann
until December 9, 1988 FDP Ludolf-Georg von Wartenberg
until July 4, 1989
Klaus Beckmann
Erich Riedl
Helmut Haussmann
from December 9, 1988 FDP
Food, Agriculture and Forestry
Ignaz Kiechle
(1930-2003) CSU Georg Gallus
Wolfgang von Geldern
Relations within Germany
Dorothee Wilms
(* 1929) CDU Ottfried Hennig
Work and social order
Norbert Blüm
(1935-2020) CDU Wolfgang Vogt
Stefan Höpfinger
Horst Seehofer
Manfred Wörner
until May 18, 1988 CDU Peter Kurt Würzbach
until December 19, 1988
Agnes Hürland-Büning
Rupert Scholz
May 18, 1988 to April 21, 1989 CDU
Youth, family, women and health
Rita Süssmuth
until November 25, 1988 CDU Anton Pfeifer
Ursula Lehr
from December 9, 1988 CDU
Jürgen Warnke
until April 21, 1989 CSU Dieter Schulte
from April 21, 1989
Environment, nature conservation and reactor safety
Walter Wallmann
until April 22, 1987 CDU
Martin Grüner
Wolfgang Gröbl
from May 7, 1987 CDU
Post and telecommunications from July 1, 1989: Post and telecommunications
Christian Schwarz-Schilling
(* 1930) CDU Wilhelm Rawe
Spatial planning, construction and urban planning
Oscar Schneider
until April 21, 1989 CSU Jürgen Echternach
Gerda Hasselfeldt
Heinz Riesenhuber
(* 1935) CDU Albert Probst
(1931-2015) CSU
Jürgen W. Möllemann
(1945–2003) FDP Irmgard Karwatzki
Norbert Lammert
Hans Klein
until April 21, 1989 CSU Volkmar Köhler
Hans-Peter Repnik
Special tasks
head of the Federal Chancellery
until April 21, 1989 CDU Lutz Stavenhagen
Lieselotte Berger
Representative of
the Federal Government in Berlin
until September 26, 1989 (deceased)
Günter Straßmeir
October 26, 1989 to December 20, 1990 CDU
Rudolf Seiters
Special duties
Head of the Federal Government's Press and Information Office
April 21, 1989 to December 20, 1990 CSU - -
Sabine Bergmann-Pohl
from October 3, 1990 CDU - -
Günther Krause
Lothar de Maizière
October 3 to December 19, 1990 CDU - -
Rainer Ortleb
from October 3, 1990 FDP - -
Hansjoachim Walther
from October 3, 1990 DSU - -
After the state elections in Hesse and the subsequent formation of a coalition of CDU and FDP, Federal Environment Minister Walter Wallmann resigned from the federal government on April 22, 1987; on April 24, 1987 he was elected Prime Minister of Hesse . The previous Minister for Environment and Health of the State of Rhineland-Palatinate, Klaus Töpfer , was appointed as the new Environment Minister on May 7, 1987 .
Defense Minister Manfred Wörner resigned on May 18, 1988 in order to take up his new post as NATO Secretary General on July 1, 1988 . His successor was the Senator for Justice and Federal Affairs of the State of Berlin , Rupert Scholz .
Federal Minister of Economics Martin Bangemann resigned on December 9, 1988 in order to be able to switch to the European Commission as Commissioner for Internal Market and Industry at the beginning of 1989 . His office as Minister of Economics was taken over by the former FDP General Secretary Helmut Haussmann .
Since she had been elected President of the German Bundestag on November 25, 1988 , Rita Süssmuth resigned on December 9, 1988. The new Federal Minister for Youth, Family, Women and Health was the Heidelberg Professor of Gerontology, Ursula Lehr .
On December 19, 1988, Parliamentary State Secretary Peter Kurt Würzbach resigned after a dispute with Federal Defense Minister Scholz about the low-level flight ban imposed by Würzbach after the plane crash in Remscheid . On the same day, Willy Wimmer was appointed as his successor as Parliamentary State Secretary at the Federal Minister of Defense .
An extensive cabinet reshuffle was carried out on April 21, 1989, which only affected the Union-led ministries. Federal Building Minister Oscar Schneider and Defense Minister Rupert Scholz , during whose short term of office the Ramstein and Remscheid accidents had occurred, were dismissed as Federal Ministers. The previous Minister of the Interior, Friedrich Zimmermann , became the new Federal Minister of Transport, the previous Minister of Finance, Gerhard Stoltenberg, the new Federal Minister of Defense and Transport Minister Jürgen Warnke, Federal Minister for Economic Cooperation. His predecessor in office, Hans Klein, took over as Federal Minister for Special Tasks as head of the Federal Government's Press and Information Office and the previous head of the Federal Chancellery, Wolfgang Schäuble , was appointed as the new Federal Minister of the Interior. For the first time, the previous chairman of the CSU regional group Theo Waigel and Gerda Hasselfeldt were appointed as Federal Minister for Regional Planning, Building and Urban Development. The previous First Parliamentary Managing Director of the CDU / CSU Bundestag faction , Rudolf Seiters , who was appointed as Federal Minister for special tasks to head the Federal Chancellery , also joined the cabinet .
Also on April 21, 1989, Parliamentary State Secretaries Hansjörg Häfele (Finance), Stefan Höpfinger (Labor and Social Affairs), Irmgard Karwatzki (Education and Science) and Volkmar Köhler (Economic Cooperation) left office. The previous chairman of the budget working group of the CDU / CSU parliamentary group Manfred Carstens , the previous social policy spokesman for the CSU regional group Horst Seehofer as parliamentary state secretary to the federal minister for labor and social affairs, and Norbert Lammert as parliamentary state secretary , were newly appointed as Parliamentary State Secretary at the Federal Minister of Finance at the Federal Minister of Education and Science and the previous chairman of the Baden-Württemberg regional group of the CDU / CSU parliamentary group Hans-Peter Repnik as Parliamentary State Secretary at the Federal Minister for Economic Cooperation.
After the number of CSU-led federal ministries had risen to six with the cabinet reshuffle, the FDP demanded another Parliamentary State Secretary to compensate. On July 4, 1989 Ludolf von Wartenberg left office. His successor at the Federal Minister of Economics was the previous parliamentary manager of the FDP parliamentary group, Klaus Beckmann .
After the death of the Parliamentary State Secretary to the Federal Chancellor and Plenipotentiary of the Federal Government in Berlin Lieselotte Berger on September 26, 1989, Günter Straßmeir was appointed her successor on October 26, 1989 .
With German reunification on October 3, 1990, the previous People's Chamber President Sabine Bergmann-Pohl , the last Prime Minister of the GDR Lothar de Maizière , the Parliamentary State Secretary to the Prime Minister of the GDR Günther Krause , the previous Chairman of the FDP Volkskammer faction Rainer Ortleb and the previous chairman of the DSU Volkskammer faction, Hansjoachim Walther, appointed federal minister for special tasks.
Lothar de Maizière resigned as Federal Minister on December 19, 1990 because of renewed allegations that he was an unofficial employee (IM) of the Ministry for State Security .
↑ a b c d e f g h i j k l m n o Reshuffle of the Federal Cabinet - dismissals and appointments by the Federal President. In: Bulletin 36-89. Press and Information Office of the Federal Government, April 21, 1989, accessed on March 10, 2018 .
↑ a b c Appointment of Prof. Dr. Ursula Maria Lehr as Federal Minister for Youth, Family, Women and Health. In: Bulletin 173-88. Press and Information Office of the Federal Government, December 10, 1988, accessed on March 10, 2018 .
↑ a b Appointment of Professor Dr. Rupert Scholz as Federal Minister of Defense. In: Bulletin 66-88. Press and Information Office of the Federal Government, May 19, 1988, accessed on March 10, 2018 .
↑ Responsibility for democracy in the service of all citizens - election of the President of the German Bundestag. In: Bulletin 165-88. Press and Information Office of the Federal Government, November 29, 1988, accessed on March 10, 2018 .
↑ Oath of the Federal Minister for the Environment, Nature Conservation and Nuclear Safety. (PDF; 2.9 MB) In: Minutes of the plenary 11/10. German Bundestag, May 7, 1987, pp. 523-524 , accessed on March 10, 2018 .
↑ a b c d e Appointment and oath of federal ministers. In: Bulletin 118-90. Press and Information Office of the Federal Government, October 5, 1990, accessed on March 10, 2018 .
^ On the decision of Federal Minister de Maizière. In: Bulletin 147-90. Press and Information Office of the Federal Government, December 20, 1990, accessed on March 10, 2018 .
List of German Federal Governments - List of German Federal Ministers
Federal Governments of the Federal Republic of Germany
Adenauer I | Adenauer II | Adenauer III | Adenauer IV | Adenauer V | Erhard I | Erhard II | Kiesinger | Brandt I | Brandt II | Schmidt I | Schmidt II | Schmidt III | Cabbage I | Kohl II | Kohl III | Cabbage IV | Cabbage V | Schröder I | Schröder II | Merkel I | Merkel II | Merkel III | Merkel IV
Kohl III cabinet - March 12, 1987 to January 18, 1991
Helmut Kohl (CDU) | Hans-Dietrich Genscher (FDP) | Friedrich Zimmermann (CSU) | Wolfgang Schäuble (CDU) | Hans A. Engelhard (FDP) | Gerhard Stoltenberg (CDU) | Theo Waigel (CSU) | Martin Bangemann (FDP) | Helmut Haussmann (FDP) | Ignaz Kiechle (CSU) | Dorothee Wilms (CDU) | Norbert Blüm (CDU) | Manfred Wörner (CDU) | Rupert Scholz (CDU) | Rita Süssmuth (CDU) | Ursula Lehr (CDU) | Jürgen Warnke (CSU) | Walter Wallmann (CDU) | Klaus Töpfer (CDU) | Christian Schwarz-Schilling (CDU) | Oscar Schneider (CSU) | Gerda Hasselfeldt (CSU) | Heinz Riesenhuber (CDU) | Jürgen Möllemann (FDP) | Hans Klein (CSU) | Rudolf Seiters (CDU) | Sabine Bergmann-Pohl (CDU) | Günther Krause (CDU) | Lothar de Maizière (CDU) | Rainer Ortleb (FDP) | Hansjoachim Walther (DSU)
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In preparing for food needs during the hard times, think of the first 10 days, the first 30 days, and the first year. Then imagine no truck deliveries of food in your regional area for a year. What are you going to do?
Most adults can survive without eating for two weeks, less so for children, and much less for infants. You should calculate 1500 calories per person per day in an emergency situation as a general rule of thumb. If you are travelling by foot to reach your destination, your safe place, remember somebody will have to carry this food as well as your water needs of 1 gallon per person per day.
You will want to use calorie dense foods as your main source of sustenance during the first ten (10) days of your journey. See our Noah Bucket, for a good example. There are a number of high calorie bars available that use fat and sugar. Your family should try them out for palatability. Don't worry about your protein needs for your first ten (10) days. That will come later. Peanut butter is the cheapest, calorie dense, readily available product. Prepackaged, high calorie soups are the best way to break the monotony of bars and help meet the fluid needs of approximately on and one half quarts of water per person per day. Remember, they will require cooking so don't forget the lighter, fuel, and pan to cook in. Don't plan on convenience stores or fast food restaurants being available.
Some are not big fans of coffee but there are instant forms of the drink and flavored caffeine products in powder from that you can add to your drinking water to give you an added boost during stressful times. It will also help with physical exertion if you're out of shape. If you have special dietary needs such as gluten-free or nut allergies, now is the time to make these preparations.
It is important to remember that you could become a refugee in your own country amongst thousands of others should mass displacement occur. Imagine that your local emergency Red Cross, and FEMA are all overwhelmed with in the first 24-48 hours. What would you and your family do? Please plan for self-reliance now. At minimum, have an emergency kit, like this one, for each family member. This would help you whether you are sheltering in place, or traveling to safety.


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We believe that our eclectic experiences have provided CDF with a unique ability to evaluate potential projects from multiple perspectives and provide the best solution.
Copyright © 2019 CDF Engineering LLC All Rights Reserved.


text:
What is a Class Action
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Elizabeth Fegan
Timothy Scott
Brooke Achua
Melissa Ryan Clark
Lynn Ellenberger
Jonathan Lindenfeld
Jessica Meeder
Ravi Sakthivel
Sexual Abuse and Assault Victims
Discrimination Victims
Antitrust Victims
Personal Injury Victims
Healthcare Payers
< Current Cases
Case Statistics
Defendant Name: First Love International Ministries, Loving InDeed Inc.
Case Number: 1:21-cv-00185
Court: United States District Court for the Northern District of Illinois
Practice Area: Consumer Fraud
Date Filed: 01/12/2021
FeganScott filed a class action lawsuit against Illinois-based non-profit, First Love International Ministries, and its partner, Loving InDeed, under the Racketeer Influenced and Corrupt Organizations (RICO) Act, claiming the organization stripped Kenyan children from their homes to create "profit orphanages," designed to attract donations from well-meaning contributors and voluntourists.
The complaint alleges that First Love built a rich but deceptive tapestry of children in need, claiming Kenyan children are in hopeless situations and have been "orphaned through AIDS, disease, violence, or simply been abandoned by their parents." However, according to the complaint, First Love utilizes a practice condemned as orphanage trafficking, where recruiters target poor Kenyan families, offering to educate their children at a boarding school with the promise of a better life.
First Love and its network of similar corporations, such as Loving InDeed and other children's homes, keep the children at their homes for years without promoting or ensuring family reunification. They then use the children's likenesses and presence to increase donations from churches and donors.
According to the complaint, filed in the United States District Court for the Northern District of Illinois, once the children reach 18 years of age, they are expelled from the orphanage, often without any attempt to reunite them with their families and without the skills necessary to integrate back into society.
In the United States and across international borders, the institutionalization of children has almost completely stopped. In fact, it is universally recognized that the placement of children in institutions should only occur as a last result, and then, only on a temporary, short-term basis.
Despite this international consensus, according to the complaint, First Love continued to traffic children, using various illicit methods to obfuscate the truth and otherwise demand the children perform for American voluntourists. In addition to these violations, the suit notes that First Love used financial and material poverty as justification for the removal of children from parental or family care, often exploiting them by forcing them to lie to voluntourists and exposing them to short, emotionally traumatic visits, which can further exacerbate the children's trauma.
Moreover, First Love allegedly utilized deceptive and misleading marketing to target donors, knowing that the monetary support was not helping the children as the donors would have expected.
The suit attempts to hold First Love for RICO Act violations including raising money to enrich themselves or their organization through activities that violate international norms and Kenyan standards, exploiting children, misleading voluntourists and donors, and harassing and threatening class members from reporting or disclosing allegations.
The suit seeks compensation and punitive damages on behalf of all persons who donated money or time to First Love or members of the First Love Solicitation Enterprise. It also seeks to expel and return the defendants' wrongful profits and revenue.
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Illinois-Based Charity Targeted in Lawsuit Alleging Orphanage Trafficking in Kenya
CHICAGO--(BUSINESS WIRE)--Today an Illinois-based charity was sued under the Racketeer Influenced and Corrupt Organizations (RICO) Act, claiming the non-profit, First Love International Ministries, and its partner, Loving InDeed, stripped Kenyan children from or failed to return them to their homes…
© 2021 FeganScott

redpajama_set_name: RedPajamaCommonCrawl


The multi-influence cylindrical bottom naval mine MINEA is the most advanced operational naval mine system in service. Cylindrical Bottom Live MINEA represent a real threat for warships and merchant ships ranging from 1.5m-15m draught. Also, conventional low-speed silent submarines operating in deep waters are threatened. The typical shock effect of 1.4 is achieved, ensuring immobilisation of the target. To find out more, please download this free white paper.


Thank you for your support of RYH and we hope to see you next time! If you have any questions, or to check on your registration status, please call our office at 770-460-1337 or email info@disciplebuilding.org.
This event is a time to hear testimony from around the world, honor those who have experienced Restoring Your Heart, and provide an opportunity to give generously so that others may experience this transformative ministry! Funds raised will help support WDA's ability to enhance curriculum, and increase the accessibility and reach of RYH. We invite you to partner with us to provide healing and freedom to people across the U.S. and the world!
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Romal uses purpose and passion to equip people to heal the wounds of their past. He bravely offers up his own journey as a case study of raw transparency and refreshing honesty. As a full-time speaker and author, Romal guides audiences through the process of identifying and embracing their unique destiny.
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text:
Q: C# FileSystemWatcher not firing off events - why not? here is my code... no FileSystemWatcher events are ever hit wen creating a new file into the Foo directory. What is wrong with my code?
I am testing this from an NUnit test by calling fileMonitorService.StartMonitoringForNewFiles(new RobotParameters()).
// attribute for autofac IoC
    [AutoRegister]
    public class FileMonitorService
    {
        private FileSystemWatcher _fileWatcher = new FileSystemWatcher();

        public void StartMonitoringForNewFiles(RobotParameters parameters)
        {

        _fileWatcher.Path = @"c:\testfiles\foo";
            _fileWatcher.NotifyFilter = NotifyFilters.Attributes |
                NotifyFilters.CreationTime |
                NotifyFilters.FileName |
                NotifyFilters.LastAccess |
                NotifyFilters.LastWrite |
                NotifyFilters.Size |
                NotifyFilters.Security;

            _fileWatcher.Filter = "*.xlsx";
            _fileWatcher.Created += new FileSystemEventHandler((sender, e)  => OnFileCreated(sender, e, parameters));
            _fileWatcher.Renamed += new RenamedEventHandler((sender, e) => OnFileRenamed(sender, e, parameters));
            _fileWatcher.Error += new ErrorEventHandler(OnError);
            _fileWatcher.EnableRaisingEvents = true;
            }

        public void StopMonitoringForFiles()
        {
_fileWatcher.EnableRaisingEvents = false;
        }

        private void OnFileRenamed(object sender, RenamedEventArgs e, RobotParameters parameters)
        {
            parameters.FileToProcess = e.FullPath;
            parameters.FileCreated = true;
        }

        private void OnFileCreated(object sender, FileSystemEventArgs e, RobotParameters parameters)
        {
            parameters.FileToProcess = e.FullPath;
            parameters.FileCreated = true;
        }

        private void OnError(object sender, ErrorEventArgs e)
        {
            var foo = e.GetException();
        }

    }

A: I never could get this to work and based on my google research, many others have had the same problem. I also tried using System.Timers.Timer and it's Elapsed event would not raise  either. Google research showed lots of others having this problem too. All my code was in a try/catch and no errors were ever raised by either. I unfortunately had to write my own file monitor code and while it is not pretty, it works. I'm posting it for any others who may have this problem and who may be looking for a custom solution.
public  class FileMonitorService
    {
        private bool stopProcessing = false;

        public  void StartMonitoringForNewFiles(RobotParameters parameters)
        {
            try
            {
                while (stopProcessing == false)
                {

                        stopProcessing = IsFileReady(parameters);
                    Thread.Sleep(5000);      // sleeps for 5 seconds

                    if (stopProcessing == true)
                    {
                        break;      // get out of loop since file is ready
                    }
                }
            }
            catch (Exception e)
            {
                throw;
            }
        }

        private bool IsFileReady(RobotParameters parameters)
        {
                try
                {
// code to try opening a file goes here
// or code to see if files exist goes here

// assuming file was opened with no errors and is ready for processing

                    return true;
                }
                catch (Exception e)
                {

// file is not ready for processing
// and could not be opened
                    return false;

                }
            }

            return false;

            }

    }

A: Never too late to get the answer. You only needed to make a small adjustment:
_fileWatcher.Created += new FileSystemEventHandler((sender, e) => OnFileCreated(sender, e, parameters));
_fileWatcher.Renamed += new RenamedEventHandler((sender, e) => OnFileRenamed(sender, e, parameters));

Just remove the new FileSystemEventHandler:
_fileWatcher.Created += (sender, e) => OnFileCreated(sender, e, parameters);
_fileWatcher.Renamed += (sender, e) => OnFileRenamed(sender, e, parameters);

This is what worked for me.

redpajama_set_name: RedPajamaStackExchange


text:
\section{Introduction}\label{sec:intro}
Cosmic ray (CR) spectra are now determined with  great accuracy revealing
noticeable disagreements with the theoretical predictions. Most of
these predictions rely on the diffusive shock acceleration theory
(DSA) -- a seemingly plausible long-standing solution for the production
of high-energy particles in a variety of shocks, primarily
supernova remnant (SNR) shocks (see, \emph{e.g.}, \citealp{Schure2012} and references therein).
The DSA theory, at least its basic version,
is remarkably insensitive to
most shock parameters and predicts
a power-law spectrum in momentum, $f\propto p^{-q},$ for the
accelerated particles. Its index, $q=3r/\left(r-1\right)$, depends
only on the shock compression, $r$. Therefore, the DSA theory can be
verified straightforwardly in strong
shocks with $r\approx4$. The agreement will then unlikely be coincidental,
but disagreement will raise doubts regarding the DSA as a viable explanation
for the observed spectrum. On the other hand, it would suggest to look
for missing elements in the ``standard'' DSA theory. These may still
reconcile the DSA even with high-precision observations.

Some difference between predicted and observed spectrum is expected
because of
factors not determined by the experiments, primarily
propagation losses. Their scaling with energy is not known precisely,
so the tight DSA index can be increased (steepened) in the range $0.3-0.6$.
However, there are two types of observations where corrections for
the losses are not required to test the DSA predictions. The first
type is pertinent to the spectrum of the \emph{ratio} of two different
elements attributable to the same or similar accelerators.
At least in one such case, the theory has already faced a serious
challenge when a $\Delta q\approx0.1$ difference between the proton
and helium rigidity spectra was firmly established \citep{ATIC06,Adriani11,Aguilar15}.
Explanations have been given (see \citealp{Serpico2015,Malkov2018}
for a review), but only a few of them address the proton
and helium spectra at the DSA level (see \citealp{Hanusch2019}
and the references therein). Even though they reproduce the data accurately, these
explanations do not vindicate the
DSA completely because they obtain particle spectra  integrated
over the entire history of an SNR evolution. Indeed,  the other type of observations
where the disagreements are present
provide the momentary particle spectra. They
are measured \emph{in situ}, using secondary emission from SNRs, produced
by accelerated CR.

At this point, it is worthwhile to separate the propagation effects
on the spectrum from the acceleration in the source. Only the latter
has a direct bearing on the DSA. At the same time, the CR propagation
models have long been used to offset for the DSA deviations from the
local spectra. A significant range in $\Delta q_{{\rm prop}}=0.3-0.6$,
depending on the particle scattering regime in the interstellar medium (ISM) (see, \emph{e.g.}, \citealp{Strong2007}), allowed one
to link the local spectrum measured on Earth, $E^{-2.7}-E^{-2.8}$ to that of the DSA-predicted,
$E^{-2}-E^{-2.2}$. Being marginal in the first place,
this link became more questionable after tighter constraints have
been imposed on both the $\Delta q_{{\rm prop}}$ (by independent
measurements of the secondary to primary CR ratios, \citealp{Aguilar2016}) and the SNR source
spectra ($\gamma$-emission generated
by accelerated CRs through the $\pi^{0}$ channel, \emph{e.g.}, \citealp{Aharonian2019}).

Even more persuasive indication of a steep source spectrum is the recent high-precision  spectral index measured to be in the range $q=2.87\pm0.06 $ below 500 GeV, by the CALET team \citep{CALET_2019PhRvL.}, fully confirming the previously published AMS-02 proton spectrum \citep{Aguilar15}. These findings
have added to the CR community concern about the DSA capacity to account for the CR production in SNRs (e.g.,  \citealp{Gabici2019}). The old paradigm  explaining  steep spectra by imposing an exponential cut-off on the DSA-produced power-law does not comply with the new data, even if one assumes that the steep part of the spectrum originates from a nearby source with a cut-off in the sub-TeV range.

To address the problem of spectrum steepening in the DSA
 several scenarios have been recently proposed. The authors of \citep{Bell2019} show that the steepened spectrum may be caused by the loss of CR energy due to turbulent magnetic field amplification during CR acceleration when the shock velocity is high.
Another particular scenario,
\citep{Malkov_Aharonian2019},
utilizes a well-known property of collisionless shocks to suppress
the proton injection when the magnetic field ahead of the shock makes
a large angle to its normal, typically $\theta_\mathrm{Bn} \gtrsim \pi/4$.
Two specific steepening mechanisms can be associated with
the variable field inclination.

The first mechanism is best represented in bilateral SNRs, where two
regions of active particle acceleration ($\theta_\mathrm{Bn} \lesssim \pi/4$,
polar caps) are separated by a region of oblique shock geometry (equatorial
$\pi/4 \lesssim \theta_\mathrm{Bn} < \pi/2$) where no significant injection/acceleration
is observed. A clear-cut example here is SN 1006. The steepening mechanism
derives from the growth of the active acceleration zone in time, as
the SNR expands. Compared to the case of a fixed acceleration area,
freshly injected particles with lower energies are added to the growing
acceleration zone at an area-integrated rate that increases with time.
This enhanced production of low-energy particles naturally results
in a steeper overall spectrum \citep{Malkov_Aharonian2019}.

The second steepening mechanism
is associated with particle diffusion from the active acceleration
zone into the neighboring oblique shock zone. As there is almost no
particle confining turbulence there, these particles have a good chance
to escape the accelerator. Since the diffusion coefficient typically
grows with energy, a steeper spectrum is expected. This mechanism
is much harder to quantify analytically since several competing factors
are at play. First, when a particle reaches the interface between
the active and inactive acceleration zones, the cross-field diffusion
decreases, whereas the parallel diffusion, on the contrary, increases.
This happens because the CR-driven turbulence level should decrease
at the interface, while the parallel and perpendicular particle diffusivities
are related as $\kappa_{\parallel}\kappa_{\perp}\simeq\kappa_{B}^{2}.$
Here $\kappa_{B}\propto r_{g}$ is the Bohm diffusion that linearly
growth with the particle gyro-radius $r_g.$  The turbulence decrease
will thus slow down the sideway losses but, at the same time, particles
reaching the interface are more likely to escape along the field.
If we add the wave self-generation by particles diffusing into the
``quiet'' zone of suppressed particle acceleration, the picture
becomes even more complicated for analytic treatment.

It may be noted from the preceding discussion that the second mechanism,
by contrast with the first one, does not require the growth of acceleration
area to produce steepening. Indeed, it results from particle losses
incurred at an energy-dependent rate. This suggests that the mechanism
can also work on a ``patchy'' shock where regions of active
and inactive acceleration are interspersed and coexist, not necessarily
growing or shrinking. Therefore, it should apply to planar shocks
and, to low-energy particles in spherical shocks where the shock curvature
is unimportant. This is the situation we study in this paper using
hybrid simulations with a magnetic field changing periodically along
the shock front.

It is important to note that the magnetic field ahead of the shock can vary
at sufficiently large scales due to the cyclotron instability of high
energy particles, escaping or diffusing further ahead of the shock.
In other words, the variable field component does not have to be preexisting
in the ISM. Under these circumstances, the shock geometry becomes
variable at scales significantly smaller than the shock radius but
still larger than the gyroradii of the low-energy accelerated particles.
The tilted magnetic field affects the injection of non-relativistic
particles. This makes hybrid simulations suitable for studying the
spectrum steepening mechanism outlined above, as no broad energy range
and, respectively, large simulation box is required.

In this paper, we study particle injection and acceleration in shocks
with magnetic field changing its direction along the shock face.
The simulation method is introduced in the next
section. Section~\ref{sec:Results} describes the principal results. We conclude with
a summary and brief discussion in Sec.~\ref{sec:Discussion}.

\section{Simulation setup}\label{sec:Set_up}
Hybrid simulations have been proven to be a valuable tool for investigating acceleration of ions at collisionless shocks in the solar system \citep{Lin2005,Burgess12,Giacalone2017} as well as CR injection and acceleration at SNR shocks \citep{Quest88, Caprioli2014}. In these simulations the electrons are considered as a massless, charge neutralizing fluid, while the ions are treated kinetically \citep[and references therein]{Lipatov2013}. In this paper we use a model, in which the electron pressure $p_{e}$ and the resistivity are both assumed to be isotropic, i.e. scalar quantities.
The pressure $p_{e}$ is modeled using an adiabatic equation of state with
the adiabatic index $\gamma_{e}=5/3.$ The fluid equations and the ion
equations of motion are non-relativistic, as $|\vec{v}| \ll c$ holds during the injection phase.  More details on our hybrid code are given in \citep{Hanusch2019}.

In the simulations times are given in units of the inverse proton cyclotron frequency, $\omega_c = e B_0 / m_pc$, where $e, m_p$ are the protons charge and mass,
respectively, $c$ denotes the velocity of light, and $B_0$ the amplitude of the background magnetic field. Distances are measured in terms of the proton skin depth
$c/\omega_p$, with $\omega_p = \sqrt{4\pi \, n_0 \, e^2/m_p}$ being the proton plasma frequency,
 where $n_0$ is the far upstream density.
The velocity is given in terms of the Alfv\'en velocity
$v_\mathrm{A} = B_0/\sqrt{4\pi \,n_0\,m_p}.$
Hence, the ratio of ion gyrofrequency to ion plasma frequency can be expressed as $\omega_c/\omega_p  =  v_\mathrm{A}/c$.
Spatially the motion of the ions is reduced to two dimensions, but all three components of the velocity and fields are included.

 Very recently the results of hydrodynamic modeling of the obliquity-dependent acceleration in a spherically expanding blast waves for different magnetic field
morphologies have been reported \citep{Pais2018}. Earlier hybrid and fully kinetic particle-in-cell simulations of shocks with variable obliquity
have been focused either on the interaction between the solar wind and a pla\-ne\-tary magnetic field \citep{Omidi2005,Blanco-Cano2009} or the simulations were initialized
with a radially expanding blast shell \citep{Dieckmann2018}. While the expanding blast shell setup resembles a spherically expanding SNR shock, it is computationally
not feasible to follow its evolution over long enough timescales and observe the acceleration of ions to high energies.
In our simulation we mimic the variation of $\theta_\mathrm{Bn}$ over the shock surface in a 2D model setup. As the shock is propagating in the $x$-direction,
we vary $\theta_\mathrm{Bn} = \theta_\mathrm{Bn}(y)$ as function of the transverse coordinate by properly choosing $B_x$ and $B_z$ as functions of $y$, ensuring $\nabla \vec B = 0$ and $|\vec B(y)| = B_0 = const$.

Two different setups of the initial magnetic field have been investigated. Both are depicted in Fig.~\ref{fig:setup}. While in the first setup the scale length of the magnetic field is twice the transverse size, in the second setup a full period is included in the simulation box. As both setups behave similarly we will focus on the first one when presenting the results.
Note, that the magnetic field inhomogeneity upstream may be at different scales, starting from the shock radius of an SNR, for example, down to the resonant wave lengths of suprathermal (shock-reflected, injected, etc.)  particles. Our choice of the scale  is suitable to capture the physics of transition between the active and suppressed injection regimes. A smoother or spatially more complicated  magnetic field geometry would be interesting to explore, but we are constrained by the box size here.
The initial configuration of the electric field is calculated using the same algorithm as at later time steps. In particular, the electric field is obtained from the equation of motion of the massless electron fluid. Since the ions are initially distributed homogeneously across the grid the density is constant and the electron pressure term is zero. This setup warrants that the Lorentz force $\vec{F}_{\mathrm{L}}=q_i(\vec{E}+\vec{v}\times\vec{B})$ acting on the ions far upstream is zero. It has been tested for stability using a simulation box with periodic boundary conditions in $x$- and $y$-direction with a size of $L_x \times L_y = 1000 \times 1000 \;(c/\omega_p)^2$. The simulation showed no sign of instability on a time of $200 \, \omega_c^{-1}$.

The simulation is initialized by sending a super-sonic and super-alfv\'enic hydrogen plasma  against a reflecting wall, placed  at $x=0.$ A shock forms upon the interaction of the
counter-propagating plasma streams and propagates in positive $x$-direction. Thus, the simulation frame is the downstream rest frame.

\begin{figure}
	\includegraphics[width=\linewidth]{setup3.pdf}
	\caption{ Background magnetic field $\vec B_0(y)$ distribution at $t=0$ for two different
			  setups with varying shock obliquity.
			  The right panel shows initial dependence of the components $B_x$ and $B_z$ on the
			  transverse coordinate, while in the left panel the angle between the shock and the
			  background magnetic field is depicted by the black arrows in addition to
			  $B_x(x,y)$.
			}
	\label{fig:setup}
\end{figure}

As the shock obliquity varies with the transverse coordinate, the transverse box size $L_y$ must be large enough, such that the results do not depend on $L_y.$ Our simulation box measures $L_x \times L_y = 8000 \times 1000 \; (c/\omega_p)^2,$ with the spatial resolution
$\Delta_x=\Delta_y=0.5\;c/\omega_{p}.$ We use 16 particles per cell and a time step of $\Delta t = 0.001 \, \omega_c^{-1}$ for an initial upstream flow velocity of $v_0 = 10 \, v_\mathrm{A}$. Ions and electrons are assumed to be in thermal equilibrium far upstream with $\beta_e = \beta_p = 1.$
The ion gyroradius $r_L = v_\perp/v_\mathrm{A} \;c/\omega_p$ ranges from 1 to 10 ion skin depths
depending on the magnetic field direction ($v_\perp = v_0$, where $\theta_\mathrm{Bn}=90^\circ$
and $v_\perp = v_\mathrm{th}$ for $\theta=0^\circ$.)
All numerical parameters have been checked for convergence.

\section{Simulation results}\label{sec:Results}
We start by presenting typical results from hybrid simulations of
a collisionless shock propagating into an environment where the
magnetic field inclination to the shock front varies. If not stated otherwise
the results correspond to an initial setup of the background magnetic field as
depicted in Fig.~\ref{fig:setup}a).
Figure~\ref{fig:fields} shows a snapshot of the ion density $n(x,y)$ and the
absolute value of the magnetic field $\vert \vec{B}(x,y)\vert$ in the simulation
domain at $t=300\,\omega_c^{-1}.$ The shock transition at
$x\sim 1200 \, c/\omega_p, $ the corresponding increase in density, and the
compression of the magnetic field are clearly visible.
The three regions, indicated by the red rectangles on Fig.~\ref{fig:fields}b)
correspond to the areas where the shock is parallel (1, $\theta_\mathrm{Bn} \approx 0^\circ$), quasi-parallel (2, $\theta_\mathrm{Bn} \approx 45^\circ$) or
perpendicular (3, $\theta_\mathrm{Bn} \approx 90^\circ$).
The components of the magnetic field in these regions
(averaged over $y$) are shown on Fig.~\ref{fig:fields}c)-e).
The proton injection is only efficient at quasi-parallel shocks. This follows from simple kinematic considerations \citep{Malkov95} and is supported by Monte-Carlo \citep{Ellison1995} and hybrid simulations \citep{Caprioli2014}.
The angle beyond which the proton injection drops fast is close to $\theta_{\mathrm{cr}}=\pi/4.$ In fact, only in regions
where the shock normal makes a reasonably sharp angle with the local magnetic field direction (quasi-parallel shock) particles can return upstream and
excite waves there (frames (c) and (d)). In the quasi-perpendicular shock geometry region (Fig.~\ref{fig:fields}e) no waves are present in the upstream.

The spatial distribution of protons with positive longitudinal
velocity $v_x>0$ is shown in Fig.~\ref{fig:positive_vx}. Due to the
turbulent fields in the downstream (note, that the simulation frame is
the downstream rest frame), many particles have there a positive $v_x.$ On the contrary, only a relatively low amount of particles have positive $v_x$ in the upstream. These particles are either directly reflected from the shock or have returned from the downstream plasma and are mainly present in regions of $\theta_\mathrm{Bn} \le 45^\circ$ (Fig.~\ref{fig:positive_vx}a). For comparison the density of particles with positive $v_x$ is also shown for a shock with constant obli\-qui\-ty $\theta_\mathrm{Bn} = 20^\circ$ in Fig.~\ref{fig:positive_vx}b). In this case the number of particles with $v_x>0$ upstream of the shock is almost independent of the transverse coordinate and variations are only present close to the shock transition.\\
\begin{figure}
	\includegraphics[width=1.02\linewidth]{fields_log.pdf}
	\caption{(a) -- Proton density $n(x,y)$  and (b) -- magnetic field amplitude $\vert \vec{B}\vert=
\sqrt{B_x^2+B_y^2+B_z^2}$ at $t=300\,\omega_c^{-1}$. The three panels (c)-(e) show the components of the magnetic field in regions of different shock obliquity, indicated by the red rectangles on frame (b).
			}
	\label{fig:fields}
\end{figure}
\begin{figure}
	\includegraphics[width=\linewidth]{positive_vx.pdf}
	\caption{Density of protons with $v_x>0$ for (a) -- the model setup with variable obliquity
			 and (b) -- a simulation of a quasi-parallel shock, both at $t=300\,\omega_c^{-1}$.
			 In the former case the presence of particles moving in $x$-direction in the upstream
			 is closely related to the condition for proton efficient injection
			 $\theta_\mathrm{Bn} \le 45^\circ$.
			}
	\label{fig:positive_vx}
\end{figure}
The proton distributions on the phase
plane $f(x,v_x)$ in the regions of different shock
obliquity (see Fig.~\ref{fig:fields}b) are shown in Fig.~\ref{fig:phase_space}.
They confirm the scenario above: shock
reflected and accelerated particles originate from regions where the shock
is quasi-parallel (Fig.~\ref{fig:phase_space}a,b). In the region where the
shock is perpendicular (Fig.~\ref{fig:phase_space}c) the shock transition
is very sharp and neither are reflected particles present in the upstream nor
accelerated ions in the downstream. Furthermore, a slight difference of the
shock positions for the parallel and perpendicular configuration becomes
apparent. This can also be observed in the plot of the ion density
(Fig.~\ref{fig:fields}a) in which the shape of the shock surface differs
significantly from a planar one.
However, we have not observed different shock velocities maintained over the whole time of the simulation for perpendicular and parallel regions.\\
\begin{figure}
	\includegraphics[width=\linewidth]{phase_space_xvx_t_300.pdf}
	\caption{ Proton distribution on phase plane $f(x,v_x)$ at $t = 300 \, \omega_c^{-1}$ in the regions indicated in Fig.~\ref{fig:fields}b) by the red rectangles. For the particles in frame (a) the shock is parallel, for (b) -- quasi parallel and for (c) -- perpendicular.
			}
	\label{fig:phase_space}
\end{figure}
In order to demonstrate the spectrum steepening effect, we have calculated proton energy
spectra in the whole downstream, as well as in different obliquity regions (Fig.~\ref{fig:fields}b) for our model setup and compared them to the spectra obtained in  a simulation of a quasi-parallel shock with $\theta_\mathrm{Bn} = 20^\circ$. Figure~\ref{fig:spectra} shows the energy spectra at two different times, $t = 200\,\omega_c^{-1}$ and at $t=400\,\omega_c^{-1}$. The energy is given in terms of $\displaystyle E_\mathrm{sh} = m_p\, v_0^2/2$. It is to be expected that the energy spectra have a spatial dependence. \citet{Guo2010} have observed spatially dependent momentum distribution functions in simulations of collisionless shocks containing large-scale magnetic-field variations.
At early times the spectrum in the region of
$\theta_\mathrm{Bn} \le 45^\circ$ of our model setup is similar to the spectrum, obtained in a simulation of a quasi-parallel shock. This is also not surprising
since the injection efficiency does not depend largely on the angle between the shock normal and the background magnetic field, as long as the shock is quasi-parallel \citep{Caprioli2014}. By the end of the simulation, however, a deviation is visible as ions can move in the turbulent downstream plasma into regions, where the shock was initially quasi-perpendicular and vice versa. The energy spectrum in the quasi-perpendicular region exhibits a behavior which has been observed in simulations of perpendicular shocks: ions are mildly energized by shock drift acceleration \citep{Park2012} and the formation of a power-law tail is suppressed. But in contrast to fully (quasi-)perpendicular shocks the spectrum shows the presence of accelerated ions, which have diffused from the quasi-parallel region into the quasi-perpendicular one.
\begin{figure}
	\includegraphics[width=\linewidth]{spectra_green_1.png}
	\caption{Downstream energy spectra: a simulation of a
quasi-parallel shock (blue) and our model with variable shock obliquity (red)
at two sequential time moments. Dotted (dashed) lines correspond to an
integration over regions where the shock is quasi-parallel
(quasi-perpendicular), (see Fig.~\ref{fig:setup}). The particles with $E > 20 E_\mathrm{sh}$
filling the green region at $t = 200\,\omega_c^{-1}$ are traced backwards in time in Fig.~\ref{fig:origin}.
			}
	\label{fig:spectra}
	\vspace{0.5cm}
\end{figure}
To confirm the origin of the accelerated particles we plot in Fig.~\ref{fig:origin} the positions of the particles ending up in the spectral tail $E > 20 E_\mathrm{sh}$ at $t = 200\,\omega_c^{-1}$ in the region $\theta_\mathrm{Bn} \ge 60^\circ$ (marked by the green region in the Fig.~\ref{fig:spectra})  at earlier times. The figure~\ref{fig:origin}  clearly shows, that the particles that contribute to the tail in the spectra in the quasi-perpendicular region ($\theta_\mathrm{Bn} > 60^\circ$) originate from the region where the shock normal is initially at an angle $\theta_\mathrm{Bn} < 60^\circ$ with respect to the background magnetic field (see panel $t = 100\,\omega_c^{-1}$ in Fig.~\ref{fig:origin}).\\
\begin{figure}
	\includegraphics[width=0.98\linewidth]{origin_B.pdf}
	\caption{Distributions of accelerated particles (red dots) ending up at $t=200\,\omega_c^{-1}$  in the spectral tail $E > 20 E_\mathrm{sh}$ (marked green in Fig.~\ref{fig:spectra}) at earlier times. The background shows the distribution of the magnetic field amplitude at the corresponding times.
			}
	\label{fig:origin}
\end{figure}
The energy spectra (Fig.~\ref{fig:spectra}) already indicate that the power-law exponent differs for the two simulation setups. To make it more evident, we have calculated the power-law index
\begin{equation}
	q = - \frac{\mathrm{d}\ln\left( f(E) \right)}{\mathrm{d}\ln E}
	\label{eq:power-law-index}
\end{equation}
from the computed spectra as function of energy and plot the result on
Fig.~\ref{fig:exponent} (dashed lines). From the downstream energy spectra we have first
calculated $\tilde q = \ln f(E) / \ln E$, indicated by the '+' markers and computed a spline (dotted line). This is then used to obtain $q$ according to Eq.~(\ref{eq:power-law-index}).
In the figure the blue lines corresponds to a setup with $\theta_\mathrm{Bn} = 20^\circ = const$, while the orange and green lines
correspond to simulations with variable obliquity.
Common to all spectra is the beginning of the power-law around $E = 10\, E_\mathrm{sh}$ (see also Fig.~\ref{fig:spectra}) which has been reported as a result from earlier hybrid simulations. At high energies the spectra exhibit an exponential cut-off due to the limited simulation time and box size.
In the region $10\, E_\mathrm{sh} < E < 50\, E_\mathrm{sh}$ $\ln f(E) / \ln E$ is almost constant and it is clearly visible, that the power-law exponent is larger for the simulation setups with variable shock obliquity. The difference of the spectral indices obtained from the simulations is $\Delta q = q_\mathrm{var} - q_\mathrm{const} \approx 0.1-0.15$.\\
\begin{figure}[!h]
	\includegraphics[width=\linewidth]{exponent_spline.pdf}
	\caption{Power-law spectral index $q$
            calculated from the downstream energy spectra at $t = 400\,\omega_c^{-1}$:
            blue line --  $\theta_\mathrm{Bn} = 20^\circ = const.,$ \
            orange line -- variable obliquity $ \vec{B}_0= B_0\left(\sin\frac{\pi y}{L_y}, 0, \left\vert\cos\frac{\pi y}{L_y}\right\vert\right), $
            green line -- variable obliquity $ \vec{B}_0= B_0\left(\cos\frac{2\pi y}{L_y}, 0,
\sin\frac{2\pi y}{L_y}\right).$ The discrepancy to the correct asymptotic index $q=1.5$ for $\theta_\mathrm{Bn} = 20^\circ$ is due to the limited run-time of the simulation and the limited box size. In the region closer to the shock particles are still accelerated to higher energies and a population of suprathermal particles exist in the transition region between the Maxwellian and the powerlaw. Our interest here is in the effect of shock obliquity which becomes evident already at $t = 400\,\omega_c^{-1}.$
	}
	\label{fig:exponent}
\end{figure}

\section{Summary}\label{sec:Discussion}
We have investigated the influence of a variable orientation
of the upstream magnetic field on ion acceleration at collisionless shocks
using hybrid simulations.
However limited in resources, our simulations have captured a new
physical phenomenon in the DSA -- the spectrum steepening associated
with the variation of shock obliquity along its face. The principal
results of this paper are as follows.\\
(i) For regions of parallel and perpendicular shock propagation coexisting
in one simulation box the DSA process, as expected, starts and proceeds
at high efficiency in the quasi-parallel region.\\[1mm]
(ii)
However, while the particle energy increases, some of them diffuse
to the quasi-perpendicular shock domain.\\[1mm]
(iii) The resulting shock-generated downstream spectrum is noticeably steeper
than canonical DSA result obtained for a quasi-parallel shock.\\[1mm]
(iv) No strong shock deceleration in the quasi-perpendicular field direction
compared to the quasi-parallel one is observed.

While the spectrum steepening observed in our simulations may be regarded
as relatively small, $\Delta q=0.1-0.15$,  it is significant for a
number of reasons. First, it is likely to be scalable to larger boxes
and longer simulation time, so that somewhat larger $\Delta q$ values
can be expected for realistic SNR conditions. Second, the mechanism
operates at relatively low energies while at higher energies a different
but closely related mechanism, described in the Introduction, should
take over. Again, a steeper overall spectrum in the SNRs will then
result, as suggested by observations. Finally, the highly determined
DSA predictions combined with extremely accurate CR data have proved
even small variations of the spectral index to be meaningful and even
testable. The $\Delta q\approx0.1$ difference between the helium
and proton local spectra is a good example.

\begin{acknowledgments}
The research was supported by the DFG within the Research grant 278305671 and in part by
NASA ATP-program within grant 80NSSC17K0255 and by the National Science Foundation under Grant No. NSF PHY-1748958. TVL acknowledges support of the Russian Science Foundation through the grant 19-71-20026 in the part related to the development of the analytic model and analysis of numerical results. Simulations were performed using the computing resources granted by the North-German Supercomputing Alliance (HLRN) under the project mvp00015.
\end{acknowledgments}

redpajama_set_name: RedPajamaArXiv


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text:
Wyatt, Atzmon, Stephen – For The Ghosts Within
(Domino) UK release date: 11 October 2010
by Daniel Paton
Robert Wyatt may be the most pertinent example in support of the argument that technique is not everything in music. His voice – vulnerable, sometimes hesitant, often straying from the true pitch – is far from any textbook case of 'proper' singing. He has little interest in conventional projection or false emoting. Instead, his is one of the most nuanced, compassionate and convincingly human voices in contemporary music. Like Billie Holiday or Bob Dylan, his phrasing is inventive and magical. Whilst there will always be blurring of boundaries with Wyatt, there is never any doubt as to the clarity of feeling or as to the texts he is interpreting. He is never anything other than a joy to hear, even when at his most poignant or melancholy.
For The Ghosts Within is rather different from much of his recent work. It is a collaborative project – with saxophonist Gilad Atzmon and violinist Ros Stephens offering contributions of equal magnitude and contrasting character. There were singular tracks on Cuckooland and Comicopera that, with hindsight, offered some hint of the territory explored here – notably the interpretation of Raining In My Heart and the touching duet with Karen Mantler on Just As You Are. The selection on For The Ghosts Within delves deeper into tradition – with several tracks drawn from the standard repertoire of jazz. Wyatt's take on the likes of Thelonious Monk's Round Midnight, Billy Strayhorn's Lush Life or Duke Ellington's In A Sentimental Mood may be less demonstrative than many of the classic recordings – but they are rich in subtlety, restraint and, crucially, warmth and humour.
A more obvious source of comparison lies outside Wyatt's own work though. Atzmon and Stephen have worked together before, on Atzmon's own standards album In Loving Memory Of America. Like much of Atzmon's work, that album also provided an opportunity to make a passionate and controversial political statement – although its impact was somewhat muted by the saccharine quality of some of the arrangements. It's arguable that For The Ghosts Within, and Stephen's contribution in particular, are more successful – lush, touching, tender – occasionally whimsical, but never sentimental.
Atzmon's articulate, full bodied playing – rich in both technique and musical language – both supports Wyatt's conversational approach and contrasts with it. Whilst Wyatt's tone is mostly reflective or meditative, Atzmon strikes a note of righteousness, purpose and conviction. His refracting of some of these familiar tunes through his Middle Eastern heritage and influences makes for something surprisingly unusual and distinctive – particularly on In A Sentimental Mood.
There are also unpredictable and disarming moments of weirdness, particularly amongst the originals. The title track begins with a contemporary-sounding introduction that is at once menacing and mysterious. It then burgeons into an ornate vocal chorus via some delightfully light and evocative cymbal work from Wyatt and an intoned melody that sounds not unlike a jazzed-up Yo La Tengo. It's an idiosyncratic, powerful and urgent plea for peace. Less immediately likeable, but somehow no less engaging, is the deeply peculiar Where Are They Now? This begins sounding like one of the Moondog-sampling escapades of Mr Scruff before the intervention of Palestinian rap group Ramallah Underground tips it well outside the realms of the sensible. It's more than a little jarring in this context – but perhaps that was the intention.
It would be easy to see this as an amiable diversion for Wyatt – but time may reveal this to be as vital a piece in the puzzle of his later work as Cuckooland. This music is at the core of what he does and has informed his musical language throughout his career. The fact that he manages to breathe new life into melodies as overplayed and hoary as What A Wonderful World or as complex and beautiful as Lush Life is triumph enough in itself.
Robert Wyatt MP3s or CDs
Robert Wyatt on Spotify
More on Robert Wyatt
Robert Wyatt – Different Every Time
Robert Wyatt – His Greatest Misses
Robert Wyatt – Comicopera
Interview: Robert Wyatt


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GRABE THIS RED CARPET!
The second annual ABS-CBN Ball took place last night, September 14, 2019, at the Shangri-La at the Fort Hotel! The entertainment industry's biggest love teams and real-life couples definitely looked like ~royalty~ as they walked the red
WATCH: Sarah Geronimo Embarks On A Journey With Her Dog In The Teaser Trailer For 'Unforgettable'
Sarah's upcoming movie has a star-studded cast!
ICYDK, Sarah Geronimo is starring in an upcoming movie called Unforgettable which will be directed by Jun Lana.In December 2018, Jun teased a video post on Instagram as Sarah was doing a look test with a golden retriever.On August 31,
WATCH: Toni Gonzaga Sang A Duet With Her Idol Regine Velasquez
Toni got to realize her childhood dream of singing a duet with Regine!
In Toni Gonzaga's latest YouTube vlog published on July 31, the host and actress shared that she has realized a childhood dream by singing a duet with her idol Regine Velasquez in the Sunday ABS-CBN noontime show, ASAP.Toni said
'Idol Philippines' Judges Pushed For A Trans Woman To Be Grouped With Female Contestants
21-year-old contestant Jeremiah Torayno identifies as a woman.
On the latest episode of singing competition Idol Philippines, the judges had an important and relevant exchange about one particular contestant, Jeremiah Torayno. While discussing the next stage of the competition, Vice Ganda wanted to group Jeremiah, a transgender woman, with the
Lovi Poe Talks About Her Workout, Favorite Songs, Her Tattoos, And More
Lovi took some time off to answer fan questions!
ICYDK, actress Lovi Poe has been in California for some time now.On May 26, Lovi threw a quick Instagram Stories Q&A session for her 3.4 million Instagram followers. Lovi got asked about her workout routine, favorite Regine Velasquez song,
The Top 10 Most Entertaining Teleserye Weddings On Philippine Television
Here are the most dramatic 'I do's.'
Pinoys will always love teleseryes no matter how many times they watch the same tropes play out. You've got the surprise child, the car accident during a rainy night, the couples cheating on each other, the sudden amnesia-you know,
by Ida Aldana
Nadine Lustre, Vivoree Esclito, And Regine Velasquez Promote Self-Love In This Music Video
This will brighten up your day!
The world can be a cruel place, especially for women. From harassment, body shaming, to passive-aggressive comments about one's appearance, these are just some of the things that make us feel like we want to give up. But we&#
by Tisha Caedo
Janella Salvador Quotes 'Thank U, Next' In New Instagram Posts
Headlines, hot news, and conversation starters on November 12, 2018!
Janella Salvador might have just confirmed her relationship status via new Instagram posts. The Kapamilya star, who made headlines in the past month after coming out with physical abuse allegations towards love team partner and rumored boyfriend Elmo Magalona, quoted lines from
by Cosmopolitan Philippines
The Internet Thinks Maine Mendoza And Arjo Atayde Are In Bali Together
Headlines, hot news, and conversation starters on November 5, 2018!
The Internet is alive and well and apparently talking about rumored couple Maine Mendoza and Arjo Atayde once again. ICYMI, the two were spotted out on dates on two separate occasions. Now, netizens believe Maine and Arjo are both in Bali based


The School Loop mobile app keeps teachers, staff and school administrators in the loop when it comes to current news and LoopMail.
Available for both iPhone and Android phones in the U.S only.
Students and parents have more full featured mobile app.
LoopMail: User your mobile device to send and receive LoopMail messages.
News: All the current news published for you. Tap any news title to view its details.
Calendar: Basic list of events for now with upgrades planned for the near future.


The Bloor Group chooses WebAction in their list of 10 Companies to Watch in 2015. The yearly Inside Analysis blog highlights companies and technologies that exemplify innovation in the IT industry. Chief Analyst, Dr. Robyn Bloor, notes that "WebAction has built a coherent and easy to use platform primarily for developing real-time analytics applications." The WebAction Real-time App Platform can correlate data from multiple structured or unstructured data sources.


text:
Top 10 Free Things to do in Miami You Shouldn't Miss
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Visiting Miami on a budget? Fear not, there is no shortage of fun and free things to do in Miami for a vacation. The Magic City of Florida offers families the chance to have an amazing time without spending a single penny.
Miami is not a cheap place to visit in Florida but still, you will find endless free activities and attractions in Miami to enjoy if you know where to look. Whether it's strolling along the beaches or enjoy free concerts, movies, and museums, these are the best things to do for free in Miami.
This post may contain affiliate links. If you buy something through one of those links, you won't pay any extra penny, but I'll get a small commission that encourages me to deliver more helpful content for you.
If you are planning for a budget trip to Miami, the below articles may help you to save some serious bucks:
10 Crazy Tips to Find Insanely Cheap Flights
10 Great Hacks to Book Cheap Hotels
How to Eat Cheap While Traveling
#1 Relax in the South Beach: Free Things to do in Miami
While visiting Miami, you cannot miss its award-winning beaches. With a picture-perfect 6.4 km of coastline, South Beach is a popular beach in Miami that has something for everyone. Enjoy swimming in the warm water or just relax and soak up the sun on the white sand beach. When you're done with swimming and sunbathing, take a stroll up Ocean Drive, a place with neon lights and endless people watching.
If you are looking for free things to do in Miami with kids, then you must visit South Pointe Park which has a playground and splash fountain. Walk along the pier and enjoy the great views of cruise ships leaving the port.
Tip: Museums like the Holocaust Museum, the Wolfsonian-FIU Art Museum, and the Jewish Museum of Florida offer free admission on certain days.
South Beach, Miami
#2 Yoga Class at Bayfront Park
Miami has some amazing places that offer free yoga classes. It is not typical yoga tourism but you can stay in shape and become more flexible and stress-free in a pleasant atmosphere around the lush green park overlooking Biscayne Bay.
Bayfront Park Management Trust hoasts a free yoga class at the Tina Hills Pavilion from Monday to Saturday. Coconut Grove's Peacock Park also offers free yoga classes on Tuesday and Thursday nights and Saturday mornings. After the yoga session, when your mind is refreshed take a short stroll through the bayside marketplace.
READ NEXT: 10 Best California Ski Resorts You Must Visit This Winter
If you are looking for more options, there are plenty of free yoga classes up and down Miami Beach. Jackson Health System, North Miami Beach Yoga Studio, Dharma Studio offer free yoga sessions in the morning. Check their website for detailed venue and timing.
Please Note: You will have to bring your own yoga mat, towel and water.
Yoga Class at Bayfront Park
#3 Enjoy Live Music at Bayside Marketplace
Can't decide what to see in Miami at night? Look no further and head towards Bayside Marketplace if you're looking for free things to do in Miami at night. There are daily live concerts at the Marina Stage, right in front of Biscayne Bay. Watch the mindblowing performance from Brazilian and Latin tunes to pop, rock, jazz, and more with your family. Check the weekly music events from their website.
Jazz lovers must visit the Museum of Contemporary Art in North Miami that offers free entertainment at 8 pm on every last Friday of each month. All music lovers gather here on that night and the live jazz makes a festival feel. Grab a snack and enjoy the evening out in Miami at its fullest.
Live Music at Bayside Marketplace
#4 Art Deco Walking Tour at South Beach
There are many companies that offer paid Art Deco Tour in Miami. Why spend money when you can have more fun to go on your own. This large Art Deco district consists of more than 900 historic buildings that were constructed between 1923 and 1943. The vivid colors, striking lanes, curves, and gorgeous architectures are the main highlights of this tour.
Some of the most remarkable buildings and hotels are Sagamore Hotel, National Hotel, Senor Frog's, The cavalier, The Tides, and the Art Deco Welcome Center. You can learn a lot about the area and the origins and development of the Miami Beach area including its mob life, Hollywood glamour, and modern design and scandals. I will highly recommend to google the building you are visiting here to know more about it.
Art Deco Walking Tour
Book Your Cheap Accommodation in Miami
#5 Free Museum Admission in Miami
Perez Art Museum, formerly known as Miami Art Museum has no admission fee on the second Saturday and first Thursday of each month. The museum features more than 2000 modern and contemporary works.
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Another museum HistoryMiami offers a free family fun day on the second Saturday of each month from 10 am to 5 pm. Browse the interesting historic and cultural exhibits and programs related to art and culture with your kids.
The Wolfsonian Museum at Miami Beach has no admission fee on every Friday after 6 pm and include films, talks, and drinks specials. Another art museum, the Bass offers free admission on the last Sunday of every month.
#6 Watch a Movie at Soundscape Park
What can be more fun than watching a movie under the stars with your family or partner? It is one of the best free activities in Miami. Head to Soundscape Park on a selected Wednesday night. The cinema series starts at 8 pm and runs from October through June at the ExoStage, corner of 17th Street, and Washington Avenue in Miami Beach. Click here for the schedule.
Don't forget to bring a blanket, and a bucket full of snacks. Enjoy the sights and sounds of the New World Symphony with friends and family. You can also listen to a free multimedia WALLCAST concert presented by Citi.
Movie at Soundscape Park
#7 Ride the Metromover
Metromover can be an ideal option for budget travelers and backpackers who are looking for cheap transportation in the greater downtown area of Miami. This iconic metromover is electrically powered and completely free for the public.
The mover is a popular transportation mode for locals as well as tourists. It connects 20 different stations from the Financial District to the border of Edgewater. The metromover serves every 90 seconds during peak times and every three minutes off-peak.
You can also take one of the many free trolleys in Miami. Check out plenty of Miami attractions like Downtown Miami, Brickell, Coconut Grove, Miami Beach, Coral Gables, Wynwood, or Doral and take the advantage of the free trolley as many times as you need.
Please Note: Metromover is not available in the South Beach area. Try to avoid it during busy hours.
Metromover in Downtown Miami
#8 Little Havana: Free Miami Attractions
Looking for free things to do in South Florida? Visit the neighborhood of Little Havana to experience Cuban culture. The place is filled with unique shops, art galleries, craft, authentic Cuban restaurants, and bars. The best time to visit Little Havana is during Viernes Culturales (Cultural Fridays), on the third Friday of each month when the whole area gets a new vibe – the streets come alive with cigar rollers, domino games, dancing, and Cuban art.
READ NEXT: 15 Best Free Things to do in San Diego That You'll Love
Another highlight that you shouldn't miss is the Little Havana Paseo de las Estrellas (Walk of the Stars), which is basically a Latin American version of the Hollywood Walk of the Stars, commemorating Latin American writers, artists, and musicians.
Little Havana
#9 Eat Tacos at Wood Tavern
If you are looking for how to eat cheap in an expensive city like Miami, then this point is for you and especially for foodie traveler. Wood Tavern offers free tacos on each Tuesday from 5 pm to 8 pm. You have to wait in line to taste those tasty chicken, pork, and beef tacos for free.
It is a funky open-air food joint with picnic benches, string lights, and fun board games. The happy hour deals at Wood Tavern are massive. They also offer free drinks for ladies from 8 p to midnight. If you are unable to visit on Tuesday, head over any Wednesday through Friday and enjoy their 50 cents wings and $5 margarita.
Tip: Come early as the place can be packed on Tuesday evening and the queue can be pretty long.
Taco Tuesday at Wood Tavern
#10 Ogle the Art at Wynwood Wall
Another free stuff in Miami is the Wynwood Art Walk. Wynwood is one of the best and funky neighborhoods in Miami. You can see colorful mural and graffiti art at every single turn. These awe-inspiring street art were created by some of the world's most talented street artists.
Kids love colors and this art walk tour can be very delightful for your kids. The murals and graffitis are constantly being updated with old ones painted over with new graffitis. Take as many pictures as you want for your Instagram feed.
Wynwood Art Walk tour includes gallery visits also. Explore the world's greatest collection of street art on a self-guided tour. You can join a free one hour tour on two wheels on every Sunday at 11 am with one of the best graffiti guides of Miami. Check here for more details about the tour.
Wynwood Art Walk Tour
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Final real name anonymity applications for the Special Demonstration Squad published
Graham Buchanan2019-08-20T11:05:59+00:00
The Undercover Policing Inquiry has today published the final three anonymity applications for former Special Demonstration Squad (SDS) officers. They are accompanied by a direction that invites submissions concerning the orders the Chairman is minded to make in respect to the applications.
The applications request that the real names of three undercover police officers in the SDS are restricted. The Chairman has already issued notes stating that he is minded to accept the three applications.
The Inquiry has already published the cover names of the three officers.
The three undercover police officers are:
"Anthony ('Bobby') Lewis" (HN78)
"Paul Gray" (HN126)
"Geoff Wallace" (HN296)
The media and any core participant that wishes to take issue with these orders should submit written representations to the Inquiry by xx, setting out the grounds of the objection.
After the Chairman has considered any submissions received, he will issue a Ruling containing his final orders in respect to the real names of the three officers.
The publication of these documents represents a significant step towards concluding the anonymity process for SDS officers and ensuring evidential hearings can take place as soon as practically possible.
There are two other outstanding anonymity applications for former SDS officers. The first requests that the real name of "Rob Harrison" (HN18) is restricted and the second requests that the cover name of HN135 – whose real name will be published – is restricted. HN18's application – which the Chairman is minded to accept – has already been published alongside a direction, while HN135's application will be considered at a closed hearing.
In total, 165 SDS officers have been included in the anonymity process, and a further four have had their real and cover names published without being included in the process. Of the 169, 52 are management or back-office staff, and 117 are undercover police officers.
Sixty-eight cover names along with a list of 76 groups that the SDS was known to have infiltrated have now been published on our website. This is to enable members of the public to determine whether they have been affected by undercover policing and to come forward with evidence
The SDS was a covert unit that existed within the Metropolitan Police Service between 1968 and 2008.
Further information on the SDS anonymity process and the recent, current and planned work can be found in the Inquiry's Eighth Update Note, which was published on 16 July 2019.
Why anonymity is sometimes needed
The Inquiry aims to be as open and transparent as possible. However, to discover the truth about undercover policing, in some cases, evidence will need to be heard by the Inquiry without members of the public, or some core participants being present at the hearing.
This can be because:
Some core participants – including people who have been deceived into relationships with officers – want their privacy respected.
Exposure of identities could put individuals at a present and ongoing serious risk of injury, or in extreme cases, death, because of the nature of the deployments they have undertaken.
Revealing identities could damage individuals or their family's private life and contravene their human rights.
In these cases, anonymity can be granted by the Chairman through a restriction order, which is a protective measure under the Inquiries Act 2005.
Where individuals have been deceived into relationships, the Chairman has stated that, when the true identity of an undercover officer is not restricted, the deceived individuals have a right to know the real name. Should a deceived individual confirm they wish to know the unrestricted true identity of the officer who deceived them, the Inquiry provides the name to them with no terms of confidence applied. Wider publication of the true identity will take place in these cases by leaving the name un-redacted in documents when they are published or otherwise shared by the Inquiry.
The directions, rulings and orders webpage on the Inquiry website contains copies of any restriction orders made. Copies of the open versions of the anonymity application are also on the website.
Further background to the Inquiry can be found on the Inquiry website.
The Undercover Policing Inquiry is constituted under the Inquiries Act 2005
The Inquiry's terms of reference were announced by the Home Secretary on 16 July 2015.
The Inquiry's Strategic Review was published in May 2018.
The Inquiry's Frequently Asked Questions document provides more information on the Inquiry more generally, as do its published update notes.
The Inquiry's website is http://www.ucpi.orq.uk/ and the Inquiry can be found on Twitter @ucpinquiry.
For further information please contact the Inquiry's communications team:
Email: press.queries@ucpi.orq.uk
Chairman rules on anonymity applications from four undercover police officers
Eighth update note
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Inquiry update notes provide a snapshot of the Inquiry's recent, current and planned work in getting to the truth of undercover policing and delivering recommendations for the future. Download the latest update note from July 2019.


text:
Empty Stocking
ARGYLE played the part of the little boy that Santa forgot this Christmas...
...as they followed up Boxing Day's 2-0 Sky Bet League 2 reverse at Newport County with a 2-1 home defeat by Oxford United on Sunday.
Lewi Alessandra opened the scoring for the Pilgrims midway through a first half which they ended with only ten men following the dismissal, for a foul, of young centre-back Aaron Bentley.
Despite continuing to dominate proceedings, Argyle were condemned to only their second Home Park defeat of the campaign when Oxford substitute John Campbell and James Roberts scored late goals against the ten men to leave the Pilgrims pointless from their two holiday matches..
Defender Andy Kellett summed up the frustration – and determination – in the Pilgrims' dressing-room after the defeat, insisting all minds were already focused on their first game of 2015 at York on Saturday.
"All the lads are gutted," he said. "I thought we should have got points out of both games we have played so close together, Newport and Oxford, but it's just not meant to be. We'll kick on from it, like we've been doing all season, and hopefully push for promotion.
"With football, you have just got to move on to the next game and that's out next focus. We've lost two on the trot now, which is not like us at all.
"Both performances have been good. We could have actually won both. We've been missing our chances lately and I think that's what punished us, because we are always going to concede – everyone concedes."
Andy paid tribute to Home Park's second-biggest crowd of the season – 11,020 – for their support in the adverse circumstances.
"The crowd is fantastic all the time, home and away. Even when we went 2-1 down, they were still getting behind us. Hopefully, they'll stick with us through this tough bit of the season.
"We are confident in ourselves. Obviously, the fans have seen how well we are playing, but it's just not clicking with that end-product at the moment because we are controlling games.
"It's a little bit tough but it is something that is easily treatable."


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Pastor Finds Burned Cross Outside Historically Black Texas Church; Authorities Say Vandalism
Pastor Bill Burton of the St. Thomas African Methodist Episcopal Church, a historically black church in Alto, Texas, is convinced that a burned cross found near his church was the result of a hate crime, although local authorities are hesitant to label it as anything more than vandalism, CBS19 reports.
According to the news station, it was Burton who discovered the cross, constructed of four tree limbs laid on the ground, and he instantly recalled a darker time in the nation's history.
"When I saw the cross burning, it was heart-wrenching," Burton said. "Just brought back the '60s to my mind, back when they used to burn crosses at different churches."
Cherokee County Chief James Campbell acknowledged that the tree limbs were put together to look like a cross, but added to the news station that it didn't appear as if they were used to burn down the church. A water line to the church also appeared to be busted, and a rock was used to break one of the windows. However, the sheriff's office did not rush to label the incident a hate crime, saying that the crime didn't appear to be what it seemed to be.
St. Thomas has been around for more than 100 years and has never had to deal with an incident quite like this. However, despite what authorities may think, Burton said he remains unmoved in his opinion.
"The reality is, the truth of the facts speak for itself; when you burn a cross on church grounds, that speaks to itself," Burton said.
Open interactive.tegna-media.com
Read more at CBS19.
News Editor at The Root, animation nerd, soca junkie, yogi


1. Say no to doorstep callers. Do not buy goods or services at the door.
2. If you are considering having work done, always shop around first and get at least three quotes.
3. You can search for a Hertfordshire Trading Standards Approved Trader at www.trustedtraders.which.co.uk or by calling Trading Standards.
4. Honest businesses agree pricing beforehand, including VAT. There's no evidence without a written contract.
5. Avoid paying cash in hand. It's better to pay by bank transfer or cheque, as these can be traced.
6. If you think you or a vulnerable relative or neighbour has become the victim of a rogue trader, report it straight away.
David Russell, 67, from Ware, contacted a local trader when he had a problem with a drain in his back garden.
The trader quoted him £200, but David was charged almost £1,500 – for a job that wasn't done to a satisfactory standard.
David was lucky as he contacted Trading Standards quickly and was able to cancel his cheque before it was cashed. As the trader had failed to give cancellation rights or indicate VAT-inclusive prices, Trading Standards brought him to court, where he pleaded guilty and was fined a total of £2,400 for David's case and two others. The company he worked for was also fined a total of £5,600.


Traveling is exciting but can be stressful for anyone. If you are living with a disability, your stress may be amplified when you travel due to worries about accommodations, fears about what could go wrong, and concerns about managing your health in an unfamiliar area. But travel doesn't have to be anxiety-inducing. These tips will help you plan and enjoy a stress-free trip so you can focus on exploring the world.
Travel agents are experienced in planning trips to destinations all over the world. Many travelers work with a travel agent to take the stress out of planning, leaving the complex coordination of flights, rental cars, hotels, and more to the experts.
Some travel agencies specialize in planning trips for people with disabilities. These travel agents are knowledgeable about accommodations people with a variety of different disabilities may require and the transportation options, hotels, and activities that are best-equipped to meet these needs. Working with a travel agent experienced in planning trips for people with disabilities can reduce much of the worry associated with traveling.
The right luggage can make all the difference when it comes to getting from point A to point B in an airport. Choose luggage that meets airline requirements for size and has ample compartments to organize your clothing and other belongings.
You'll want to take advantage of your ability to take a carry-on bag onboard the flight as well as a personal item – which can be a purse or tote bag that contains other essentials that you might need during the trip. Wheeled luggage is a good option for larger bags that you plan to check, as you can wheel these bags easily through the airport without struggling to carry heavy bags.
Depending on your disability, you may use special equipment or take medications to help manage your condition. Pack enough medications to last several days in your carry-on bags, as well as copies of documentation from your physician explaining your disability and the equipment, medications, or other supplies that you rely on to manage your disability.
In the event that you need to see a doctor during your trip, your healthcare provider will have some background knowledge that enables them to provide the most appropriate treatment – or, they can get in touch with your primary physician to discuss the best course of treatment for the circumstances.
This is where planning ahead is a lifesaver: Call ahead (or have your travel agent call ahead) to discuss your specific needs with any transportation providers you'll be using on your trip. Arranging for a wheelchair or an attendant to help you get from one gate to another for a connecting flight can save you hours of time explaining your situation to attendants and waiting for the airport to provide what you need on travel day.
Likewise, you may be able to get special permission to take certain medications on board the flight. You or your travel agent can call ahead to your hotel and discuss the travel accommodations you require to see if they can provide an accessible shuttle.
Traveling with a disability doesn't have to be stressful nightmare. Planning ahead, advocating for yourself, and following some savvy travel strategies can help you get through travel days with minimal stress.
Rebecca Moore is currently studying health information science. She created AbleRise.net with a friend with the ultimate goal of fostering community mechanisms for seamless acceptance and assistance for those coping with any measure of disability.


The Potter's Wheel Christian Fellowship is a growing evangelical Christian assembly of approximately 75-80 believers committed to the call of Jesus Christ to reach out and minister to all people. Our ministries, gatherings and various outreaches are designed to encourage and grow our relationship with God, with our church family and with our community.
We offer a variety of weekly activities which include Sunday worship, children's church, Bible study and prayer, and a youth sports night. We also organize a variety of outreaches in the community and participate with and financially support various other local, national and international charities.
We also support and partner with other Christian assemblies, ministries and groups in the community. These collaborations help us reach out to the community in ways we could not do alone.
The Pentecostal Assemblies of Canada (PAOC) is a Fellowship of more than 1,100 churches across English- and French-speaking Canada. More than 235,000 people across the nation attend services in more than 40 languages, and we are pleased to provide ministerial credentials for more than 2,500 pastors and ministry leaders. They help facilitate the vitral work of spreading the Good News of the Gospel of our Lord Jesus Christ and bringing hope and help to those in need inn Canada and around the world.
The Quebec District of PAOC aims to develop a relational and intentional approach to its mission by focusing on seven values that emphasize and improve relationships.
Involvement in Missions at a local, national and international level in order to respond to Christ's commandment to make disciples of all nations.
The Quebec Council of Christian Charities works in close cooperation with the Canadian Council of Christian Charities, a charity servicing Christian charities throughout Canada for more than 30 years.
They are aware that many Christian churches and organizations are dismayed by all the government legislation governing charities. Organizations need to find experienced, specialized and competent professionals capable to offer the needed resources and a helping hand.
Their mission is to help those called to the ministry in their administrative burden and in so doing, help them to accomplish their mission of spreading the good news of Jesus Christ or any other calling they may have. In other words, they answer the administrative needs of Christian churches and organizations of Quebec that are registered as a charity or desiring to be have such a legal structure.
The Evangelical Fellowship of Canada (EFC) is the national association of evangelical Christians in Canada. It gathers Evangelicals together for impact, influence and identity in ministry and public witness. Since 1964 the EFC has provided a national forum for Evangelicals and a constructive voice for biblical principles in life and society. The EFC affiliates include denominations, ministry organizations, educational institutions and individual congregations, who uphold a common statement of faith. The EFC also has more than 15,000 supporting individuals.
Andrew Wommack Ministries takes life-changing truths from the Word of God to people around the world. This is achieved through radio, television, audio and video media, books, the Internet, conferences, personal speaking engagements and support of other Christian ministries. Their head office is located in Colorado Springs, Colorado, but they have satellite offices in many countries around the world, including Canada. The ministry also has Bible colleges located around the world which are a unique blend of the teaching of God's Word and practical on-the-job training.


text:
Ferland Mendy (Meulan-en-Yvelines, 1995. június 8. –) francia válogatott labdarúgó, hátvéd, a Real Madrid játékosa.

Pályafutása

Klubcsapatokban
Pályafutása kezdetén, ifjúsági korú labdarúgóként több csapat akadémiáján is megfordult. 2004-től 2012-ig a Paris Saint-Germain, majd egy évig a Football Club Mantois akadémiájának tagja volt, 2013-ban került a Le Havre csapatához.

A 2013-14-es szezonban az ötödosztályú tartalékcsapatban játszott, a felnőttek között 2015 áprilisában debütált az akkor másodosztályban szereplő csapatnál. A 2016-2017-es szezonban lett stabil tagja a kezdőcsapatnak, az idény során 35 bajnoki mérkőzésen két gólt szerzett, teljesítményével több európai élcsapat figyelmét felkeltette.

2017. június 29-én ötéves szerződést írt alá a Lyon csapatával, az első osztályú csapat ötmillió eurót fizetett a játékjogáért. 2017. augusztus 26-án debütált a Ligue 1-ben egy Nantes elleni találkozón. hamar alapembere lett a csapatnak, amelynek színeiben bemutatkozhatott az európai kupaporondon is. A 2017–2018-as Európa-liga-sorozatban hét alkalommal lépett pályára.

A 2018-2019-es szezonban 30 bajnoki mérkőzésen két gólt szerzett, a Bajnokok Ligájában nyolc mérkőzésen kapott lehetőséget.

2019 nyarán a Real Madrid igazolta le, Mendy öt évre írt alá a spanyol klubhoz, amely sajtóhírek szerint 48 millió eurót fizetett érte a Lyonnak.

A válogatottban
2018. november 20-án mutatkozott be a francia válogatottban Uruguay ellen.

Statisztika

Klubcsapatokban
2022. szeptember 18-án frissítve.

A válogatottban
2022. szeptember 25-én frissítve.

Sikerei, díjai

Real Madrid
Spanyol bajnok (2): 2019–20, 2021–22
Spanyol szuperkupa (2): 2019–20, 2021–22

Bajnokok Ligája (1): 2021–22
UEFA-szuperkupa: 2022

Egyéni elismerés
UNFP Ligue 2, Az év csapata: 2016–17
UNFP Ligue 1, Az év csapata: 2017–18, 2018–19

Jegyzetek

További információk

Francia labdarúgók
Labdarúgóhátvédek
1995-ben született személyek
A Le Havre labdarúgói
Az Olympique Lyonnais labdarúgói
A Real Madrid labdarúgói
A Ligue 2 labdarúgói
A Ligue 1 labdarúgói
A La Liga labdarúgói
Élő személyek

redpajama_set_name: RedPajamaWikipedia


text:
Влесінешть, Влесінешті () — село у повіті Ботошані в Румунії. Входить до складу комуни Влесінешть.

Село розташоване на відстані 393 км на північ від Бухареста, 26 км на північний схід від Ботошань, 101 км на північний захід від Ясс.

Населення
За даними перепису населення 2002 року у селі проживали  особи, усі — румуни. Усі жителі села рідною мовою назвали румунську.

Примітки

Села повіту Ботошань


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Fray Check will not discolor or stain most fabrics. Always test on an inconspicuous seam to be sure. 1.Place a piece of cardboard between area being treated and other fabric layers. 2.Unscrew blue cap and puncture tip with fine pin. 3.Gently squeeze bottle and apply very small amount of Fray Check. 4. Allow to dry for 15-30 minutes. 5. Always keep cap on Fray Check bottle when not in use. TIP-to remove unwanted spots of Fray Check, treat with rubbing alcohol. Test in an area to be sure there is no color change or ring formation.