How Can Personal Resource Use Have a Global Impact?
In this project students will use their knowledge of renewable vs. nonrenewable resources to study and analyze typical daily use of both types of resources both in school and at home. My wish is that students will start to see patterns of overuse,especially of nonrenewable resources; and will get excited about developing ideas for change. I also hope they will begin to see that change can start small, and that working together, change can cause a global reaction.
This project will get students thinking about real life issues that will have a lasting effect on themselves and the environment. I am hoping that students will then want to talk to family members, friends, and other community members, ultimately using the theme "knowledge is power" to encourage change and awareness. As a final activity, Students will design posters in groups to illustrate their positive message for change, and hope for the future.


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Come visit the 14 Vineyards & Wineries on the south coast of Massachusetts, southern Rhode Island and southern Conneticut. Take a day or weekend touring wineries in your backyard.
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No. 77: Life Partners—Latest Developments Relating to the Court-Ordered Death Sentence
Life Partners Holdings, Inc. (NYSE:LPHI) is a participant in the secondary market for life insurance. In No. 75 posted December 10, I said Senior U.S. District Court Judge James R. Nowlin handed down a "final judgment order" on December 2 in a lawsuit filed by the Securities and Exchange Commission (SEC) against LPHI and its two top officers: Brian D. Pardo, chief executive officer; and R. Scott Peden, general counsel. The order requires LPHI to pay the SEC $38.7 million (more than twice LPHI's total assets!) by December 16. I called the financial dimensions of the order a death sentence for LPHI. (SEC v. LPHI, U.S. District Court, Western District of Texas, Case No. 1:12-cv-33.)
Developments on December 10
On December 10, three things happened. First, Dana Livingston, a partner in the Austin firm of Alexander Dubose Jefferson & Townsend, appeared before the court as an attorney for LPHI.
Second, the defendants filed an "opposed emergency motion to extend stay of enforcement of the judgment." The motion is "opposed" because "the SEC is not willing to agree to any extension of the automatic stay [until December 16] at this time." The motion says the defendants intend to file by December 30 their post-judgment motions, such as motions to alter or amend the judgment and a motion for a new trial.
Third, Judge Nowlin granted LPHI's motion. He stayed execution of the judgment and any proceedings to enforce the judgment for an additional 14 days, until December 30.
Later Developments
On December 12, James Craig Orr, Jr., a partner in the Dallas firm of Heygood Orr & Pearson, sent a letter to Judge Nowlin on behalf of investors in LPHI's life settlements. Orr asks the judge to consider reducing the judgment against LPHI because the amount is far more than what LPHI possesses, and because LPHI would not be able to perform the ministerial services needed to protect the investors' funds.
On December 15, the court issued a deficiency notice because Orr's filing is in the form of a letter rather than a motion. The court asks Orr to refile immediately in the form of a motion.
LPHI's Nondisclosure
At the close of business on December 16, there is no press release on the LPHI website about the December 2 order. Also, there is no 8-K (material event) report on the SEC website, although such a report is supposed to be filed within four business days after the event.
LPHI's nondisclosure is not unusual. As I reported in No. 35 posted March 10, 2014, selective disclosure—prompt disclosure of good news and delayed disclosure of bad news—is standard practice at LPHI.
LPHI's Share Prices
Despite LPHI's nondisclosure, and despite the absence of news stories since shortly after the order, word got around. LPHI's share price declined sharply after the order—from a closing price of $1.43 on the day of the order to $1.10 the next day. Closing prices were $1.06 on December 4, $1.00 on December 11, $0.94 on December 12, $0.90 on December 15, and $0.78 on December 16.
Ministerial Fees
Meanwhile, in No. 74 posted November 25, I discussed LPHI's decision to begin charging its investors fees—through its newly formed subsidiary, LPI Financial Services, Inc.—for ministerial services relating to life settlements. On November 14, one month after the due date of the first annual fee payments, LPI sent investors a "past due" notice that reads:
PAST DUE. Please Disregard if Paid. Payment is due upon receipt. Delinquent payments will be subject to interest at the maximum rate permitted under law as well as reporting to credit bureaus. Failure or refusal may result in termination of access to platform services.
I am offering a complimentary 13-page PDF showing LPHI's seven-page motion for a stay, LPHI's one-page proposed order, the judge's one-page order granting a stay until December 30, Orr's three-page December 12 letter to the judge, and the court's one-page December 15 deficiency notice. In No. 75, I offered a complimentary 21-page PDF showing Judge Nowlin's December 2 final order; this PDF is still available. Send an e-mail to jmbelth@gmail.com and ask for the LPHI motion for stay, or the final order in the SEC lawsuit against LPHI, or both.
Email: jmbelth@gmail.com
Blog: www.josephmbelth.com
No. 77: Life Partners—Latest Developments Relating...
No. 76: Daniel Stallings and an Update on the Case...
No. 75: Life Partners Faces a Court-Ordered Death ...

redpajama_set_name: RedPajamaCommonCrawl


As I sat watching my daughter at gymnastics recently, I realised that there are many skills and abilities she has to have in order to be successful in her sport, that we could also equate to being a successful Small Business owner.
A gymnast will have their routine meticulously planned out, with every move structured to flow seamlessly into the next. If however, as the gymnast moves through their routine something unexpected happens, they must be able to remain open and adaptive, able to respond to what is happening in that moment.
It is the same for Small Business owners, for we must respond to what is happening in the marketplace and perhaps alter the course of our product or service accordingly.
Running a business is no different to being a gymnast in this regard – with a business plan and routine needed and goals to be set and focused on.
Flexibility alone however, is not enough – a successful gymnast also needs core strength and stability. If they are overly flexible without any inner strength, they may run the risk of pulling a muscle or doing more permanent damage.
Whilst it's good to have flexibility as a Small Business owner, it's vital that we are the strong and steady core strength of our business. If we fall apart, so does everything around us. We must always have a clear vision of why we do what we do – is it to make a difference in the world, to be of service to others, to pay for an annual holiday, to pay off the mortgage, to put the kids through college, or something else entirely?
Knowing our driving factor will help us to stay strong and stable.
My daughter cannot go to gymnastics only when she feels like it and expect to excel. She has to practice, day after day, week after week. She has to listen to her coach, watch how others succeed and get up every time she falls down. She has to go when she's tired, when she's fed up, when she's feeling lazy and when she has her cranky pants on.
It's no different when we're running a business – we don't wake up one day as a success (much to some people's surprise) – it takes dedication and time to learn the necessary skills. We all know that it's fun to spend hours watching cat videos on YouTube and checking out what our friends are doing on Facebook, but just as this won't make us a top gymnast, it won't make us a successful business owner either.
We need to have a plan and we need to work that plan – day after day after day! There's nothing wrong with watching a cat video or two, but one or two can easily turn into three hours of watching animal antics.
I watched my daughter learning to do what she calls a front walkover. When she first started she would do handstands up against the wall, then it progressed to going over onto a high sofa, then to a few cushions and eventually she was able to go straight over and land perfectly on her feet. It took weeks of practicing, every day, watching others do it and getting up every time she fell down.
To become proficient at running our own business will probably take more than a just a few weeks, but by practicing every day, learning from peers, coaches and mentors, eventually we will get there. The world changes constantly and we must change with it, continuing to learn and grow as we go. This is why sites like Smallville are perfect for business owners like you and me.
If you are on the balance beam and you lean too far one way, you will wobble and likely fall.
Running a business is much like performing on a balance beam – you have to walk a fine line, staying focused on the end result, but navigating the wobbles along the way. If you lose your balance, you are likely to fall.
This is a trap that many solopreneurs often fall into, with something eventually having to give. We think we don't have time for self-care, exercise, healthy food, time with loved ones, hobbies or even sometimes sleep and this can be our downfall.
Are you a business gymnast? I'd love to know how you practice consistency, with both flexibility and strength with balance in mind.
What Are Your Monthly Numbers?
What Kind Of Vibe Does Your Small Business Have?
Love it Sharon. Really good article.
Love this down to earth, tell it as it is approach to business. Off to limber up now!


This single serve cookie dough dip is low in carbs and packed with protein, but you'd never be able to tell! Thick, creamy and perfectly portioned, it is a quick snack or dessert to enjoy anytime, with or without dippers! It's also suitable for those following a vegan, gluten free, paleo, dairy free and sugar free lifestyle!
Chips and dip just got a sweet makeover and I ain't complaining.
To be completely honest, I'd never even had a sweet dip before until my first time in America.
One of my college friends invited me to a 'When I grow up' party in one of the off-campus Fraternity houses. He told me everyone had to dress up as what they envisioned themselves to be working in post-college.
My group of friends and I went as….well, whatever random costumes we could find at Walmart. I'm pretty sure I bought some generic mask and put on a suit and voila- My lame attempt of a costume.
My friends had the same idea.
I think (read- I HOPE) that the true party theme was taken very lightly… unless 90% of the guys and girls wanted to be lingerie models and/or shirtless football players.
Change of subject- The food!
Amongst the typical party foods (hot dogs, chips, chips, a bowl of Spongebob lollipops and more chips) was this huge bowl of dip. I first assumed it was some kind of hummus which someone had accidentally dropped chocolate chips into. However, upon further inspection, I saw a pattern of apple slices, cookie sticks and sugar pretzel rods around it.
Besides, who would hummus with chocolate chips?
My friend told me that it wasn't uncommon to have sweet dips at big parties, with peanut butter, honey yogurt, and oreo ones being the popular ones. Although it wasn't my usual salsa or guacamole, I was game to try it and must say….Us Aussies had been missing out! The dip was thick, creamy and had a similar texture to a cupcake frosting. It was also studded with chocolate chips (NOT spiked) and had a hint of vanilla throughout.
While I would totally have (and did!) enjoy the dip on its own, I know not everyone is as lame as me. As such, you are in for a double delight today with a special dipper recipe to go with it!
Long term readers know I'm a huge fan of Flatout flatbreads, due to their versatility, taste and the fact that wraps can be stuffed to the brim without falling apart! I've been trying to 'think outside the wrap' with them and come up with some fun flavors, albeit still being healthy.
One of my favorite flavors is without a doubt the infamous 'cinnamon roll', so what better way than to make healthy baked cinnamon roll pita chips? I simply baked them with some cinnamon and granulated sweetener and once they were baked, made a simple coconut oil drizzle and allowed it to cool.
Cinnabon, eat your heart out.
A healthy baked pita chip recipe which taste like cinnamon rolls- No added oils or butter!
Preheat the oven to 350 degrees fahrenheit. Spray a large baking tray/dish with cooking spray. Cut the Flatout wrap into squares and place on a single layer. Spray the squares lightly with more cooking spray and set aside.
In a small bowl, mix the cinnamon, sweetener of choice and sea salt until combined. Sprinkle over the pita chips and bake for 8-10 minutes, or until crispy and golden on the edges.
While the chips are cooking, make your glaze by whisking the coconut butter, milk of choice, cinnamon and lemon juice.
Once the chips have cooled, drizzle with coconut butter frosting until firmed up and enjoy!
What do healthy baked cinnamon roll pita chips need? A dip of course!
This healthy low carb cookie dough dip is smooth, thick and creamy and also specifically designed for one! Unlike traditional dessert style dips, this version contains no dairy, sugar, butter, cream or oil, but you'd never be able to tell! It is pretty customizable too- You can make it as thick as you want or if you prefer a thinner, creamier dip, that works well too. This dip has been tested to suit most dietary lifestyles out there- It can easily be gluten free, dairy free, sugar free, paleo and vegan- Just take note of the tested methods and options!
There are two key components here- Protein powder and chocolate chips coconut flour.
Protein powder helps thicken your base of choice (Greek yogurt, non-dairy yogurt or coconut yogurt), as long as you use a non-whey protein powder. I tried it using my standbys- This vegan protein powder, this casein protein powder, and this paleo protein powder. I never recommend whey protein powder, especially in a recipe like this (or my oatmeal recipes)- I find that it makes it somewhat sticky and produces the opposite effect of thickening- Not cool!
The second component here is coconut flour– Although this one isn't exactly necessary. If you are a fan of super thick dips, or one which is almost like a cake batter, you'll NEED this addition. It's because of the coconut flour that what you see pictured looks somewhat like mashed potatoes. If you aren't a fan of coconut flour or don't have any on hand, you can use gluten-free oat flour or even rolled oats. However, this will increase the carb count, if that is what you are on the watch for!
Okay, the REAL second component is chocolate chips– This isn't necessary, but well…it kind of is.
Chips and dip get a makeover = Healthy low carb cookie dough dip for one + cinnamon roll baked pita chips.
Only in the mood for crispy? The healthy baked cinnamon roll pita chips are for you.
A fan of the dip itself and watching your carbs (and portion control)? Call dibs on the healthy low carb cookie dough dip for one.
As for me? I will have both, and when I grow up, I want to be a popsicle.
This single serve cookie dough dip is low in carbs and packed with protein, but you'd never be able to tell! Thick, creamy and perfectly portioned, it is a quick snack or dessert to enjoy anytime, with or without dippers! It's also suitable for those following a vegan, gluten free, paleo, dairy free and sugar free lifestyle!
In a mixing bowl, add your yogurt of choice. Stir through your protein powder and sweetener of choice.
Slowly add your coconut flour until desired texture is achieved. Top with chocolate chips and enjoy!
** For a thinner dip, use a tablespoon and add milk of choice until desired texture is achieved.
More delicious low carb recipes? Gotcha covered!
This post is sponsored by Flatout Bread. Cheers, hugs and handshakes for supporting companies and brands which allow me to do what I'm passionate about every day and make The Big Man's World possible.
Have you ever had a dessert style dip before?
Are you a fan of the dipper or the dip itself? Niki eats all the corn chips and ignores the dip. I used to eat salsa and guac with a spoon. Okay, I still do.
On a side note, I'm pretty sure you guys were heading to a Halloween party…either that, or you wanted to grow up to be witches.
Had I been at that party, I would've dressed up as a Disney princess because that's what I wanted to do when I grew up. I literally envisioned myself performing as Belle at a Disney park. Then I realized they have super strict height requirements that I did not meet for those parts and that the costumes are super hot, so I just got a regular job instead.
My friend was Belle…and Jasmine? She had to be one in the morning and one in the afternoon!
I rarely had dessert style dips at a party, but regardless, I'd eat the whole bowls of dip! XD If someone makes a healthy chocolate hummus, then you'll bet that I'll demolish it!
Love it! That sounds pretty good right now!
Thank you for telling me that there is such a thing as oreo dip. I will now die very fat.
It's incredible- I made one for a house warming last week!
This is genius – and two recipes in one! The dip AND the dippers look sooo good… The dippers remind me of 'cinnamon grahams' (I don't know if you would have had them in Australia), which I always used to have for breakfast when I was little – if I cut the wrap into smaller squares, I can make a healthy replica of my old favourite cereal! I can sense the nostalgia already? Then I can smother them in the cookie dough dip!!
I think I prefer dip over dippers – guacamole, salsa, cookie dough dip….I mean, cookie dough dip with chocolate chips has just gotta be one of the best things ever, right?? Thanks for the recipe(s), Arman!
It's so fluffy and delicious looking; Arman, your friends are blessed with a really creative cook/baker that will always keep them guessing with delicious additions to the party.
I'm a dip freak and totally eat guac, salsa, hummus, and nut butter with spoons. I mean, I'm not gonna turn down dippers, but I don't need them. I NEED the dips. And this one. It's so fluffyyyyyyy.
Can I possibly make this without protein powder? I have whey vanilla, but I didn't like the taste of it in oatmeal, like you said kinda had the opposite affect.
I made this with peanut protein. Heaven! I also used chocolate protein powder with coconut flour and chopped almonds for an Almond Joy dip. I love how this recipe is so flexible and uses ingredients I always have on hand.


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The Pandemic Ushered In An Era Of Hybrid Work – And Hybrid Shopping
by Allison Schiff // Wednesday, November 24th, 2021 – 11:00 am
Many of the shopping behaviors that developed over the past couple of years due to COVID-19 have solidified and appear here to stay.
The majority of consumers (56%) say they plan to shop primarily or exclusively online this holiday season, and more than three-quarters say they'll use in-store pickup services this year as much or more than last year, according to recent research from performance marketing agency Tinuiti.
But many shoppers aren't just going to show up without confirming that what they want is in stock.
Forrester found that nearly one-third of US online holiday shoppers will check online first to see whether an item is available before heading to a physical store.
That means retailers should expect and prepare themselves for a sizable wave of in-store shoppers, an uptick in curbside pickup and a high volume of requests coming in from online shoppers looking to secure limited stock items, said Phil Melson, a retail client partner at data analytics provider Fractal Analytics.
"The mental math done by individual shoppers choosing to rush to a store to buy something off the shelf versus securing online and picking up later will be case by case and interesting to see," he said.
But retailers have their own mental math to do.
The average Black Friday discount offer this year will be lower than Black Fridays of yore, according to data from market intelligence platform StyleSage.
"Many retail stores won't be able to restock on the merchandise once they sell out of an item they have and will risk staying out of stock on those items for much longer than usual," said Wiley Zhang, COO of Acquco, a newly launched startup that acquires and scales third-party sellers on Amazon.
Supply-chain bottlenecks are largely to blame for this dynamic, he said. A lack of supply combined with high consumer demand is leading to product and labor shortages, and the overall increase in the price of raw materials is leading retailers to offset higher costs by reducing promotions and selling certain products at full price, Zhang said.
But some retailers responded by debuting their Black Friday deals last month to mollify "nervous online shoppers" who have been making their holiday purchases earlier this year, said Bryan Cano, director of media strategy at online retail advertising startup StitcherAds, which was acquired by Kargo in October.
"Digital is more critical than ever during a period like this because it's a more adaptive channel than brick and mortar," said Cano, who predicts a marked increase in the number of holiday sales offered on the web this year.
But of more importance to many online shoppers this season is the cost of shipping rather than the price of a product, according to a survey conducted by CommerceNext, which also found that around a third of merchants are cutting back on promotions and offers during Thanksgiving, Cyber Monday and throughout the month of December, presumably due to the shortage of inventory to promote, said Sucharita Kodali, a VP and principal analyst at Forrester.
And so "Cyber 5," the five-day stretch from Thanksgiving through Cyber Monday, might be softer this year, said Josh Brisco, VP of growth media at Tinuiti.
But marketers have been rolling with the punches, and they've "done well in attempting to navigate the macroeconomic challenges presented this year," he said.
"Whether that be forcing the narrative of the earlier promotional cycle to retailers or crafting creative ways to maximize marketing efforts based on existing and forecasted inventories of goods," Brisco said, "the marketer is an ever-important factor in a retailer's ability to find success in a holiday season with so many brand-new challenges."
And the balancing act will continue as retailers do the best they can to account for supply-chain snarls and marketers manage reduced promotional volume without sacrificing too much overall sales.
"I don't know that there is much else they can do," Kodali said. "These marketers are definitely making lemonade with lemons."
Shopify Pushes Further Into Social Channels, As The Hunt For Online Customers Intensifies
Why Spectrum Brands Is Bringing Its Amazon Advertising Approach To The Web
How Online Grocery Seller Hungryroot Benefits From Not Launching An Ad Platform
Supply Chain Shortage Hitting Ad Industry Hard; Google Bans Climate Change Misinformation
Hunger For New Subscribers Is Driving Down Prices As Brands Discard Acquisition Cost Models


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Elea Digital announces sustainability-linked bond issued by a data centre operator in Latin America
Data CentresTop Stories
Alix Pressley | 14 December, 2022
Elea Digital, a Brazilian Edge data centre ecosystem, has announced a R$ 200 million sustainability-linked bond to significantly reduce water usage in its operations, reaching ambitious targets that will place the company among the more efficient in the world.
Elea Digital will invest in more advanced and sustainable equipment that allows a more efficient use of water in the cooling process of its data centres while maintaining an efficient use of energy.
According to Alessandro Lombardi, Chairman of Elea Digital, the company, since its foundation, has been committed to positive socio-environmental actions.
"Today, Elea Digital takes the lead on the commitment with sustainability in the digital infrastructure sector in Brazil," said Lombardi. "We trust that other players may be inspired by our pioneer path."
The project had the support of three of the largest financial institutions in Brazil and showed adherence in the support of sustainability initiatives. The transaction can inspire other players to follow this sustainable direction.
"We are proud to be lead coordinator of the first sustainability-linked bond of Elea Digital which also is the first one in the data centre industry," said Rafael Garcia, Head of Fixed Income at Bradesco BBI. "By committing to environmental and social targets, the company innovates and fosters sustainable practices in a relevant sector."


text:
\section{Introduction}
\label{sect_intro}

Quiescent prominences, or filaments, are dynamic formations of relatively cool and dense plasma (T $\sim 10^4$~K, $\mathrm{n_{e}}\sim 10^{11}\pcmc$) extending into the much hotter and rarefied corona (T $\sim 10^6$~K, $\mathrm{n_{e}}\sim 10^{8}\pcmc$) over magnetic polarity boundaries far from active regions \citep{Martin:1998,TandbergHanssen:1995ud,Priest:1988,Schmieder:1984ul}. In the ``polar crown'' regions they are frequently observed in so-called ``coronal cavities,'' dark elliptical structures seen during eclipses or in extreme ultraviolet (EUV) and X-ray images of the corona \citep{Kucera:2012,Reeves:2012bu,Schmit:2011ix,Habbal:2010,Fuller:2009jm,Gibson:2006kr}.  Coronal cavities and prominences are the progenitors of coronal mass ejections (CMEs), with the overlying arcade loop system, the cavity, and the prominence comprising the leading dense shell, dark void, and bright trailing material, respectively \citep{Dere:1999ki,Gibson:1998ua,Illing:1986gq}.  Understanding the mechanisms of formation, evolution, and eventual eruption of this complex magnetic system is a central goal of solar physics.

Prominence formation mechanisms can be generally classified into chromospheric transport and coronal condensation \citep{Labrosse:2010bt,Mackay:2010fp}.  In the former, \emph{cool} plasma is lifted from the chromosphere into the corona by siphon flows \citep{PikelNer:1971ft}, magnetic reconnection \citep{Litvinenko:1999gc}, or magnetic flux emergence \citep{Okamoto:2008kg}.  In the latter, \emph{hot} plasma
 in the local corona condenses into a prominence \citep{Xia:2012,Luna:2012eb,Karpen:2008hc,Antiochos:1999ef,An:1985fa,1983SoPh...88..219P}. Confirming observations of any of these mechanisms have thus far been elusive.

Here we report the first analysis of {\it Solar Dynamics Observatory} Atmospheric Imaging Assembly \citep[SDO/AIA;][]{Lemen:2011} observations of  apparent \emph{in situ} formation of a quiescent prominence within a coronal cavity. The results are consistent with earlier studies of cloud prominence formation \citep{Liu:2012gq} and support the hypothesis that coronal cavities and prominences are not in magnetostatic equilibrium, but instead harbor a novel magneto-thermal convection \citep{Berger:2011eoa} with hot upflows and condensation downflows enabling the build-up of magnetic energy and helicity and culminating in an eruptive CME \citep{Zhang:2005dn}.  Recent theoretical analyses \citep{Low:2012tu,Low:2012tv} suggest that MHD condensation has a resistive origin due to runaway thermal collapse of condensing plasmas and spontaneous current sheets \citep{Parker:1994cs,Parker:1953}, leading to rapid condensation and cross-field transport of prominence plasma.

\section{Temporal Sequence of Events}
\label{sect_temporal}

\begin{figure*}
	\includegraphics[width=\textwidth]{f1.eps}
	\caption{Time sequence of SDO/AIA images in the 171~\AA\ (yellow) and 304~\AA\ (red) channels. Note the disappearance of the prominence from the cavity, (a)--(c), the appearance of a bright emission cloud, (d)--(e), and the formation and growth of a new prominence, (f)--(i). See also Movies 1a \& 1b, 304~\AA\ overlaid on 171 and 211~\AA, respectively.}
	\label{fig:171+304}
\end{figure*}

The event under study occurred on 27--28 April 2012 on the NW limb (heliographic x,y: +375\arcsec, +900\arcsec\ from disk center).
Beginning at 04/27 00:00 UT, a tall quiescent polar crown prominence was observed in the AIA \ion{He}{2} 304~\AA\ channel, extending approximately 150\arcsec\  (108 Mm) above the limb.  The prominence was surrounded by a large well-defined coronal cavity that shows maximum contrast in the \ion{Fe}{14} 211~\AA\ channel. The prominence gradually disappears from the 304~\AA\ channel over the course of the next 13 hours, due primarily to downward mass flows, as well as perhaps thermal ``Disparation Brusque'' \citep[DBt;][]{OfmanMouradian:1996}. We note that the time scale for the disappearance is much shorter than required for solar rotation to displace the prominence longitudinally from the limb. Also, STEREO/EUVI data establish that the cavity has a very large longitudinal extent, with prominence plasma remaining at other longitudes. However those same data show that the prominence we observe at the AIA limb is distinct from these other formations. Figures~\ref{fig:171+304}(a)--(c) show this temporal evolution in the AIA 304 and 171~\AA\ channels.

Following the disappearance, the cavity region near the limb remains prominence-free for some 5--6 hours. Meanwhile, a ``cloud'' of hot plasma gradually accumulates near the core of the cavity. The cloud has the highest contrast against the background in the \ion{Fe}{9} 171~\AA\ channel and develops into its brightest apparition by 04/28 01:28~UT. At about 04/27 22:00~UT there is an initial appearance of  304~\AA\ emission at the lower edge of the cloud. Figures~\ref{fig:171+304}(d)--(f) illustrate this initial cloud formation and prominence appearance sequence.

Figures~\ref{fig:171+304}(g)--(i) show that the 304~\AA\ emission continues to expand in both height and width over the next several hours. Simultaneously, the size of the 171~\AA\ emission cloud decreases markedly. By 04/28 04:00~UT the 171~\AA\ emission is confined largely to the region surrounding the growing prominence.
Thin threads of 171~\AA\ emission can be seen curving outward and upward from the prominence at this time. Such prominence ``horns'' have been observed in both prior AIA data \citep{Regnier:2011cr} as well as SOHO data \citep{Vourlidas:2012tz,Plunkett:2000ud}. In the final period of the observation, the 171~\AA\ emission is confined to a very narrow ``Prominence Corona Transition Region'' (PCTR) sheath \citep{Parenti:2007ba} with some residual projections upwards into the cavity. At this point, the coronal cavity is again well-defined in the 211~\AA\  channel. The total time from initial re-appearance in the 304~\AA\ channel to the fully extended prominence in Panel~(i) is approximately 18 hours.

\section{Multispectral Analysis of the Cooling Cloud}
\label{sect_cloud}

\begin{figure}
	\includegraphics[width=0.5\textwidth]{f2.eps}
	\caption{Comparison of coronal cavity emission cloud appearance in the 193~\AA\ (left) and 171~\AA\ (right) channels over time. Note that the emission cloud fades in the 193~\AA\ channel, (b)--(c), while it brightens in the 171~\AA\ channel, (f)--(g). See also Movie 2.}
	\label{fig:193+171}
\end{figure}

Figure~\ref{fig:193+171} shows a subset of the temporal sequence discussed above in the \ion{Fe}{12} 193~\AA\ and 171~\AA\ channels. The subset begins at 04/27 10:55~UT when there was no prominence visible in the 304~\AA\ channel, and shows a largely featureless, barely visible, coronal cavity in the 193~\AA\ channel while the center of the cavity is well-defined in the 171~\AA\ channel. The second row of Fig.~\ref{fig:193+171} shows the clearly developed cloud structure in both channels.  By 04/28 04:00~UT the cloud has decreased in contrast in the 193~\AA\ channel while remaining bright and high contrast in the 171~\AA\ channel (third row of Fig.~\ref{fig:193+171}).  The fourth row shows that the prominence has fully formed by 04/28 16:40~UT. Absorption of the 193~\AA\ emission by both the prominence and some of the residual horn structure (see Fig.~\ref{fig:171+304}(h)) is evident.

\begin{figure}
	\includegraphics[width=0.45\textwidth]{f3a.eps} \\
	\includegraphics[width=0.45\textwidth]{f3b.eps}
	\caption{Timeslice analysis of the emission cloud. (a) 211~\AA\ channel image taken when the prominence has fully formed. The cavity outline is well visible as is the absorption due to the prominence. The vertical dotted box indicates the region over which vertical columns of pixels are averaged to create timeslice images in the 211, 193, 171, and 304~\AA\ channels. The constant height dotted box ($h = 144\arcsec$ above the limb) is used in the timeslice of Fig.~\ref{fig:mass}.  White `\textsf{+}'s mark the lower left corners of the timeslices. (b)--(e):  base ratios with the reference image time for each panel indicated by a small circle. Colorbars indicate the intensity ratio ranges. Black `\textsf{X}'s mark the locations and times of peak emission in each panel. The yellow curves plot relative emission (arbitrarily scaled) along the horizontal dashed lines that traverse the cavity at heights corresponding to the peak emission in each channel. The white contour in all panels shows the outline of the prominence in the 304~\AA\ channel. The peak temperature of emission in each channel is indicated next to the wavelength identifier in units of $10^6$~K (MK).}
	\label{fig:timeslice}
\end{figure}

Figure~\ref{fig:timeslice} shows the emission in the 211, 193, 171, and 304~\AA\ channels averaged over slices taken from the vertical box that encloses the central region of the cavity shown in Panel~(a). Panels~(b)--(e) show the resulting ``timeslices'' in each channel. Emission in the 211~\AA\ channel is spatially concentrated and brightest (relative to the reference frame) at  04/27 13:30~UT. Emission in the 193~\AA\ channel is spatially most compact and brightest several hours later at 20:45~UT. Similarly the 171~\AA\ emission is compact and brightest at 04/28 01:28~UT. Finally, the prominence has its brightest, most compact 304~\AA\ emission at 04/28 07:10~UT. Note that the height of maximum emission steadily decreases with time and decreasing wavelength (and temperature) in the 211, 193, and 171~\AA\ sequence.  The first appearance of the 304~\AA\ prominence emission occurs only after the cloud has descended to a height of approximately 75~Mm in the 171~\AA\ channel.

\section{Filter Ratio Temperature Analysis}
\label{sect_temp}

\begin{figure}
	\includegraphics[width=0.48\textwidth]{f4.eps}
	\caption{Filter ratio analysis of emission cloud temperature.  (a) AIA temperature response curves for the five EUV wavelength channels used in the ratio analysis. (b)--(d) Example 171/211, 193/211, and 211/335 response ratio curves. For the three times in the timeslice sequence indicated by \textsf{X}-marks in Figs.~\ref{fig:timeslice}(b)--(d), we plot the corresponding ratios measured in the emission cloud. The colored horizontal dotted lines show the ratio measurements for each time while the vertical dashed lines indicate the intersection points with the ratio response curves. Colors delineate the times as shown in (b).  The histogram of intersection points is shown in (e)--(g) for the three times, respectively. In these panels, all ratio intersection points are shown at each time as short vertical bars (see text). The modal temperature for the hotter peak is indicated in $\log\mathrm{T}$ form in each panel. The histogram colors correspond to the times shown in (b).}
	\label{fig:twofilter}
\end{figure}

Given the wide spectral passbands of AIA, a detailed determination of the plasma temperature and density along the lines of  \cite{Heinzel:2008ig} is not possible. However we can use the known AIA instrument response functions to calculate a temperature range for the emitting cloud structure as a function of time.  While this method implicitly assumes an isothermal temperature distribution for the plasma \citep[which is unlikely to be valid in a complex coronal cavity, e.g.,][]{Kucera:2012}, it has the advantage of having no adjustable parameters and is not an ill-posed inversion problem.

Figure~\ref{fig:twofilter}(a) shows the measured temperature response curves of the AIA telescopes from \texttt{aia\_get\_response.pro}. Taking the ratios 171/211, 193/211, 211/335  gives the set of curves shown in Fig.~\ref{fig:twofilter}(b)--(d). The emission of the cloud in each channel is measured by averaging the emission of 3$\times$3 ``pixel'' samples around the \textsf{X}-marks shown at specific times in Fig.~\ref{fig:timeslice}(b)--(d)\footnote{The average is thus taken over the three images before, during, and after the peak emission times marked in Fig.~\ref{fig:timeslice}(b)--(d) and in three spatial pixel vertically centered on the location of the `\textsf{X}' marks.}. The ratios are then computed and plotted on Figs.~\ref{fig:twofilter}(b)--(d) as the dotted horizontal lines.

We measured all ten ratios from the set $\{131, 171, 193, 211, 335\}$\AA\ at each of the specific times above. The temperatures at the intersections of these ten ratios with the response curves are shown as short vertical bars on the axes of Figs.~\ref{fig:twofilter}(e)--(g). These measurements are binned in temperature to create histograms of inferred temperatures, showing that there are two most likely solutions around $\log\mathrm{T}\sim 5.35$ and $6.2$~K. The peak around $\log\mathrm{T}\sim 6.2$~K shows a larger degree of clustering than the lower temperature peak implying that it is the more likely solution. In addition, this peak shows a trend toward a cooler temperature over the three time steps sampled in the dataset. In particular, the mode of the peaks are $\log\mathrm{T}\sim 6.25$, $6.15$, and $6.15$~K for the times 04/27 13:30~UT, 04/27 20:45~UT, and 04/28 01:28~UT, respectively. The latter peak, while having the same mode as the previous time, shows a pronounced tail to the cooler temperature range. In contrast, the $\log\mathrm{T}\sim 5.35$~K peak does not show such a consistent trend.

Taken together, the filter ratio analysis implies that the initial temperature of the emission cloud is $\log\mathrm{T}\sim 6.25$~K with a cooling trend over time. Emission ultimately appears in the 304~\AA\ channel implying a very definite cooling trend, however this filter cannot be used in the foregoing filter ratio analysis because the plasma is optically thick in \ion{He}{2}, violating the optically thin assumption in the response curves of Fig.~\ref{fig:twofilter}.

\section{Prominence Mass and Cavity Contrast Comparison}
\label{sect_mass}

\begin{figure}
	\includegraphics[width=0.5\textwidth]{f5.eps}
	\caption{Coronal cavity contrast and prominence mass cycle.  (a) Timeslice image in the  211~\AA\ channel formed from the average of all constant height pixels in the dotted outline in Fig.~\ref{fig:timeslice}(a).  The thick white outline shows the coronal cavity as it reaches its highest contrast. The darkest central core of the cavity appears at a position of 340\arcsec, offset by approximately 40\arcsec\ from the location of the 304~\AA\ prominence indicated by the thin white contours. (b) 304~\AA\ ``plane-of-sky'' mass of the prominence as a function over the same time period. The POS mass increases roughly simultaneously with the increase in coronal cavity contrast.}
	\label{fig:mass}
\end{figure}

Figure~\ref{fig:mass} shows a contrast analysis of the coronal cavity in the 211~\AA\ channel along with a mass estimate in the quiescent prominence. Cavity contrast is calculated by examining the average emission in a timeslice of constant-height pixels (dotted outline in Fig.~\ref{fig:timeslice}(a)). Figure~\ref{fig:mass}(a) shows the timeslice and reveals that the core of the cavity darkens significantly beginning around 04/27 16:00~UT. This is several hours after the peak 211~\AA\ emission of the cooling cloud, but roughly coincides with the rise to maximum emission in the 193~\AA\ cloud, as shown in Fig.~\ref{fig:timeslice}. As the cloud emission intensifies in the cooler channels, the cavity darkens further until by about 04/28 16:00~UT, the cavity achieves maximum darkness in the core.  Although cavity contrast is a strong function of view angle and hence can be influenced by solar rotation, at the heliographic latitude of the cavity (N68), the rotation is only $6^\circ$ over the 12~h during which the cavity contrast changes significantly, too little to explain the observed contrast change. We note also that the darkest region of cavity extends over a larger region than the prominence absorption.

We estimate the prominence mass as the ``plane-of-sky'' (POS) mass, calculated by measuring the area of emission detected in the 304~\AA\ channel and assuming that the  prominence  is  a uniform thickness slab in the POS. This method grossly underestimates the true mass of the prominence since most prominences have significant longitudinal extent. Nevertheless, the method allows an analysis of prominence mass over time at a zero-order level of detail; changes in the assumed geometry of the prominence will alter only the absolute mass number and not the shape of the temporal curve. Here we assume a typical prominence density of $\mathrm{n_{e}} = 8\times 10^9 \pcmc$ \citep{Labrosse:2010bt} or $\rho = 1.3\times 10^{-14}\ \mathrm{g} \pcmc$ ,  and a thickness of 10\arcsec\ (7300~km) to arrive at the numbers shown in Fig.~\ref{fig:mass}(b).

The plot shows that the POS mass of the prominence steadily decreases at an average rate of approximately $2.4\times 10^{13}$~g~h$^{-1}$ from 00:00~UT to 12:00~UT on 27-April. Beginning at about 22:00~UT, the new prominence forms initially at about the same rate.
However the rate decreases after 04/28 3:00~UT and is highly variable thereafter. Note that the onset of rapid coronal cavity darkening in the 211~\AA\ channel corresponds well with the onset of prominence appearance in the 304~\AA\ channel and that the cavity core increases in darkness as the prominence continues to accumulate mass (see Movie 1b). Since coronal cavity core contrast is largely a function of plasma density relative to the surrounding corona \citep{Fuller:2009jm}, we interpret the darkening of the cavity core to indicate a loss of plasma from the region.

\section{Summary and Discussion}
\label{sect_discussion}

We have analyzed observations of the dynamic formation of a quiescent polar crown prominence in a coronal cavity. The sequence of events is summarized as follows:
\begin{enumerate}
\item A pre-existing prominence slowly disappears due mostly to drainage and lateral transport of plasma (Fig.~\ref{fig:171+304}).
\item A bright emission cloud forms in the upper regions of the coronal cavity (Figs.~\ref{fig:171+304} and \ref{fig:193+171}).
\item The cloud descends toward the lower region of the cavity while sequentially becoming brighter in the 211, 193, and 171~\AA\ channels (Fig.~\ref{fig:timeslice}).
\item A new prominence appears in the 304~\AA\ channel and rapidly grows in both vertical and horizontal extent (Figs.~\ref{fig:171+304} and \ref{fig:timeslice}).
\item The coronal cavity core above the prominence grows darker in the 211~\AA\ channel as the 304~\AA\ prominence grows (Fig.~\ref{fig:mass}).
\item When the prominence reaches its maximum size after approximately 18~h of growth, the emission cloud in the cavity is completely gone (Fig.~\ref{fig:171+304}).
\end{enumerate}

Taken together, these observations are consistent with the hypothesis that the quiescent prominence has formed via condensation from hotter plasma contained in the core of the coronal cavity. We interpret the EUV emission sequences in Figs.~\ref{fig:171+304},  \ref{fig:193+171}, and \ref{fig:timeslice} as evidence of radiative cooling and descent of the hot plasma in the coronal cavity core, first appearing bright in the hotter  211~\AA\ channel with a peak temperature of formation of $\log\mathrm{T_{max}}\sim 6.2$~K, followed by a shift to emission in the 193~\AA\ channel ($\log\mathrm{T_{max}}\sim 6.1$~K), followed by another shift to emission in the  171~\AA\ channel ($\log\mathrm{T_{max}}\sim 5.8$~K), and finally appearing in the ``chromospheric'' 304~\AA\ channel ($\log\mathrm{T_{max}}\sim 4.8$~K).

The profile of the hotter filter ratio histogram widens toward cooler temperatures over time (Fig.~\ref{fig:twofilter}(g)), further supporting our interpretation that the observed plasma radiatively cools to condense into the prominence.  The drop in height of the cloud further supports this hypothesis. Radiative cooling is proportional to $\mathrm{n_{e}}\!^2$ at corona temperatures and increases with decreasing temperature in the $\log\mathrm{T} \sim$ 5--7~K range. Therefore a ``runaway thermal instability'' is possible in which the plasma cools increasingly rapidly as it becomes denser and cooler \citep{Low:2012tu}. The increased density of the cloud naturally results in higher gravitational force countering the local Lorentz force of the cavity magnetic field. Thus the descent of the cloud is consistent with radiative cooling and condensation in a weakly magnetized environment as the plasma seeks a new equilibrium height, possibly through resistive reconnection \citep{Low:2012tv}. As the prominence gains mass at the expense of the hot cloud, the coronal cavity simultaneously becomes more sharply defined in the 211~\AA\ channel due to mass loss from the core region.

The observations shown here imply the possibility of \emph{in situ} formation of prominences in coronal cavities. Given the large density disparity, \cite{TandbergHanssen:1995ud} estimated that the entire coronal mass could only support such condensation for a few large prominences.  However this concern was based on the implicit assumption that prominences are magnetostatic suspensions of a fixed amount of plasma. But as shown by recent SDO/AIA and \emph{Hinode}/SOT observations, quiescent prominences are in constant motion via drainage downflows \citep{Liu:2012gq,Haerendel:2011de,Chae:2008ca} and re-supply of mass through various mechanisms \citep[e.g.,][]{Berger:2011eoa,Li:2012,Su:2012}.  \cite{Liu:2012gq} estimated the mass loss in prominence downflows  to be $10^{15}$~g/day or roughly the equivalent of a typical CME mass. Thus the mass in a prominence changes significantly with time and is not directly related to the mass in the global corona in a simple manner. Mass balance in prominences appears to be a cyclic process in which the mass transported into the coronal cavity determines how much can eventually condense to form prominences. Similar cyclic processes have been proposed for the quiet Sun coronal mass balance \citep{McIntosh:2012,Antolin:2012,Marsch:2008} and coronal rain condensation \citep{Landi:2009,Schrijver:2001}.

Observations at the limb necessarily integrate along heliographic longitude. Thus it is possible that the prominence that disappears is not at the same longitude as the new prominence that forms, or that the cloud and the new prominence are a line-of-sight coincidence. But the fact that the shrinkage of the cloud (darkening of the cavity), the descent of the cloud, the formation of prominence ``horns'', and the eventual formation of a PCTR sheath are all synchronized with the growth of the prominence in the 304~\AA\ channel argue against a line-of-sight coincidence. We note that the hot cloud itself exhibits no significant flows, other than its slow radial descent, during the condensation process. Thus it is unlikely that we are confusing \emph{in situ} condensation with flow-based formation mechanisms such as flows between disparate magnetic footpoints \citep[e.g.,][]{Xia:2012,Luna:2012eb,Karpen:2008hc,Antiochos:1999ef}.

{\scriptsize

redpajama_set_name: RedPajamaArXiv


text:
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Ever since the 2016 referendum, the United Kingdom has been divided. It has become clear that the Government and politicians in Westminster are unable to stop fighting long enough to reach a consensus, and whilst they squabble amongst themselves, Britain is breaking under the strain. Business is leaving, jobs are being lost and the extreme right and left wing are on the rise. The cause of this is Brexit, and if we want to see our country healed and renew our hope for the future, it must be stopped.
Britain is Better than this.
We believe that Britain is better than this. We believe that people deserve more. The lies told by those promoting Brexit have been exposed, along with the illegal funding and downright dodgy campaign methods employed. People deserve to have a chance to take another look at the Brexit deal on offer, and give their informed consent now they know more of the facts.
We are campaigning for a People's Vote referendum with an option to Remain, which we believe is the only chance we have of stopping Brexit. If, as we expect, we succeed in our objective, we will redirect our energies to campaigning for Remain.
We can stop Brexit and give our young people a brighter future. A future where Britain is not closed down and looking inward, but one where we are open and welcoming, working together with our nearest neighbours to tackle the global challenges facing us so that we can enjoy a more prosperous, peaceful and successful future.
But we need your help....
Goodwill and brave hearts only go so far. With only days remaining, we must work extra hard to stop Brexit. Campaigning takes time and money - and we are running out of both!
We need your help to support our work. If you want a final say on whatever dodgy deal gets offered to us, we need to up the ante and make our voices heard.
We urgently need funds to:
Hire coaches to ensure a Yorkshire presence outside Parliament
Sponsor students and the unwaged to cover their transport costs
Set up new local groups across North Yorkshire
Run regular street stalls in our towns
Meet the cost of holding rallies and debates
Design and print leaflets telling people the facts,
Buy flags and banners to make an impact on TV
March again on London to make our presence felt
Support the fight to win a second referendum vote
With your support we can do this and more. With your help we can Stop Brexit and Save Britain!
Adrian Cook
Richard Sadler
Sign up as a Fundraiser
We are North Yorkshire for Europe. We are campaigning for a People's Vote referendum with an option to Remain, which we believe is the only chance we have of stopping Brexit. We need your help!
North Yorkshire for Europe Harrogate, England, United Kingdom
Get in touch with Exit from Brexit! Support the Campaign for a People's Vote
Your message to James Roberts


BARTHEL, R; (2004) Standardization in e-Learning. The "Sharable Content Object Reference Model (SCORM)". InWent Capacity Building: Cologne.
Batty, M; (2004) Dissecting the streams of planning history: technology versus policy through models. ENVIRONMENT AND PLANNING B-PLANNING & DESIGN , 31 (3) pp. 326-330. 10.1068/b3103ed.
Batty, M; (2004) Distance in space syntax. (CASA Working Papers 80). Centre for Advanced Spatial Analysis (UCL): London, UK.
Batty, M; (2004) Faster or complex? A calculus for urban connectivity. ENVIRONMENT AND PLANNING B-PLANNING & DESIGN , 31 (6) pp. 803-804. 10.1068/b3106ed.
Batty, M; (2004) Hierarchies in cities and city systems. (CASA Working Paper Series 85). Centre for Advanced Spatial Analysis (UCL): London, UK.
Batty, M; (2004) Large Scale Disasters in Small Scale Spaces: Simulating Crowd Movements, Congestion, and Panic. In: (Proceedings) Ninth International Seminar on GIS: Emergency and Disaster Response with GIS. (pp. pp. 1-25). : Korean Research Institute for Human Settlements.
Batty, M; (2004) Michael Batty on 'Wilson's Entropy in Urban and Regional Modelling'. Papers in Regional Science , 83 pp. 74-76.
Batty, M; (2004) Wilson's Entropy in Urban and Regional Modelling'. Papers in Regional Science , 83 pp. 74-76.
Batty, M; (2004) The coming oil crisis. ENVIRONMENT AND PLANNING B-PLANNING & DESIGN , 31 (5) pp. 645-646. 10.1068/b3105ed.
Batty, M; (2004) A new theory of space syntax. (CASA Working Papers ). Centre for Advanced Spatial Analysis (UCL): London, UK.
Batty, M; (2004) Contributions to Part 4: Looking To The Future. In: Gilfoyle, J and Thorpe, P, (eds.) Geographic Information Management in Local Government. (pp. 205-212). CRC Press: Boca Raton, FL.
Batty, M; Besussi, E; Maat, K; Harts, JJ; (2004) Representing multifunctional cities: Density and diversity in space and time. Built Environment , 30 (4) pp. 324-337. 10.2148/benv.30.4.324.57156.
Carvalho, R; (2004) The dynamics of the linear random farmer model. In: Barnett, WA and Deissenberg, C and Feichtinger, G, (eds.) Economic Complexity: Non-linear Dynamics, Multi-agents Economies and Learning. Elsevier: New York.
Carvalho, R; Batty, M; (2004) Automatic Extraction of Hierarchical Urban Networks: A Micro-Spatial Approach. In: Computational Science - ICCS 2004. (pp. 1109-1116). Springer: Berlin.
Carvalho, R; Penn, A; (2004) Scaling and universality in the micro-structure of urban space. PHYSICA A-STATISTICAL MECHANICS AND ITS APPLICATIONS , 332 pp. 539-547. 10.1016/j.physa.2003.10.024.
Cheng, J; Masser, I; (2004) Integrating spatially and temporally explicit decision-making processes into cellular automata modelling, Environment and Planning, B, 31, 167-194. Environment and Planning B , 31 (167) 194-.
Dodge, Martin; Kitchin, Rob; (2004) Code, space and everyday life. (CASA Working Papers 81). Centre for Advanced Spatial Analysis (UCL): London, UK.
Dodge, Martin; Kitchin, Rob; (2004) Codes of Life: Identification Codes and the Machine-Readable World. (CASA Working Papers 82). Centre for Advanced Spatial Analysis (UCL): London, UK.
Dodge, Martin; Kitchin, Rob; (2004) Net:Geography Fieldwork Frequently Asked Questions. (CASA Working Papers 83). Centre for Advanced Spatial Analysis (UCL): London, UK.
Gabrielli, A; Masucci, AP; Labini, FS; (2004) Gravitational force in weakly correlated particle spatial distributions. PHYS REV E , 69 (3) , Article 031110. 10.1103/PhysRevE.69.031110.
Kitazawa, K; Batty, M; (2004) Pedestrian Behaviour Modelling. In: Van Leeuwen, JP and Timmermans, HJP, (eds.) (Proceedings) 7th International Conference on Design & Decision Support Systems in Architecture and Urban Planning. (pp. pp. 111-126).
Li, C; (2004) Spatial ability, urban wayfinding and location-based services:a review and first results. (CASA Working Paper Series 77). Centre for Advanced Spatial Analysis (UCL): London, UK.
Oh, Kyushik; Jeong, Yeunwoo; Lee, Dongkun; Lee, Wangkey; (2004) Determining Sustainable Development Density using the Urban Carrying Capacity Assessment System. (CASA Working Papers 78). Centre for Advanced Spatial Analysis (UCL): London, UK.
Rana, S.; (2004) Two approximate solutions to the Art Gallery Problem. Presented at: International Conference on Computer Graphics and Interactive Techniques, Los Angeles.
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This list was generated on Sun Apr 21 06:32:44 2019 BST.


Home » American Payroll Posts » What Are Quarterly Wage Reports and Why Do They Matter?
Update: New York passed new wage requirements that go into effect for quarters beginning January 1, 2019. The new requirements accelerate filing for Part C on NYS-45 and NYS-45-ATT forms to a quarterly basis (previously annual). The first quarter return due date with the new requirements is April 30, 2019.
Your Federal Employer Identification Number (FEIN) as well as your relevant state identification number(s).
By automating your payroll tax calculations and deductions, small business payroll software, like Wagepoint, helps gather the information needed to complete the reports. Many providers, like us, are also able to help you pay and report your payroll taxes as well. We'd love for you to pick us, but regardless of who you choose — automating your payroll taxes will take a huge burden off your shoulders — giving you more time to focus on building and growing your business.
Got questions about wage reports, payroll taxes... your favorite sports team? Just ask and we'll help you find the answers.


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Statement of changes to the Immigration Rules introducing new EU Settlement Scheme
On the 20th July 2018 Parliament presented the Statement of changes to the Immigration Rules introducing new EU Settlement Scheme for post Brexit status confirmation. The new Appendix EU describes the rules under which EU citizens and their family members can obtain a settled status in the UK after Brexit. These changes take effect on the 28th of August 2018 for the purpose of initial trial.
Appendix EU is the legislation under which EU citizens and their families can apply for leave to remain in the UK under the Immigration Rules of Great Britain. The trial period of the new EU Settlement Scheme should set up the mechanism of application process.
EU citizens and members of their families, who were permanently settled in the UK for five years by the 31st of December 2020, will be eligible for 'settled status' (indefinite leave to remain in the UK). Those who lived in the UK for less than 5 years by the 31st of December 2020, will be able to obtain a 'pre-settled status' (five years' limited leave to remain in the UK). Once they reach 5 years threshold they will be able to apply for "settled status".
After 31st of December 2020, close family members of an EU citizen (spouse, civil partner, long-term partner, dependent child or grandchild, dependent parent or dependent grandparent) residing abroad can join the main applicant in the UK. They will need to prove that their relationship existed on the 31st of December 2020 and continues to exist while the person moves to the UK.
In terms of domestic policy, it was also decided that family members of British citizens who lawfully resided in the UK until 31st of December 2020 under Regulation 9 of the 2016 Immigration Regulations (EU), will have the right to apply for "settled status" in accordance with Appendix EU.
The testing of the new EU Settlement Scheme will begin on the 28th of August 2018. At the first stage, EU citizens residing in the north-west of England from 12 NHS organizations, as well as students and staff from three Liverpool universities will participate in the pilot version. They are the first to submit electronic applications to obtain immigration status in the UK. In total 4000 people will participate in the pilot version. This will allow those working on the scheme to test it in real time and make the necessary improvements before the launch of the system, which will begin in phases in late 2018. The program will be fully available to all applicants by 30th of March 2019.
Posted in English on Jul 22, 2018.


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Forgotten Audiences: Women, Mobile, and Gaming
Posted bygavinjohnston67	 April 28, 2019 Leave a comment on Forgotten Audiences: Women, Mobile, and Gaming
You can find any number of articles online that will trumpet the news that nearly half of the world's gamers are female. But what does that figure really tell us? What the data often miss is that this side of the gaming world skews considerably older than the male equivalent; the average woman playing video games is 37 and financially independent. And in fact, women outnumber male gamers in the 50-64 and 65+ demographics.
With an audience of adult women gamers whose numbers are nearly double those of boys under 18, it is important to question why so many games seem designed with adolescent males as the default audience. But just as critical is the question of why middle-aged and older women don't seem to be targeted for any gaming news or entertainment content of their own. What sets them apart and makes the industry as a whole feel comfortable ignoring them?
The key to this mystery is the perceived divide between "hardcore" and "casual" (terms that seem suspect from the outset), with middle-aged women relegated to the latter category. And while it's wrong to assume that casual gamers don't deserve our attention, it is true that their tastes are very different from the (largely young and male) hardcore gamers. This older segment of women prefers to play mostly puzzle and strategy games, most often on a mobile device. They gravitate toward the type of "snackable" games that can be picked up and put down at a moment's notice.
Historically, women have not been particularly well-served by the sedentary nature and limited distribution of traditional games. But casual mobile games have made inroads with women who previously never had the opportunity or inclination to set aside time for lengthy gaming sessions. Prior to the advent of mobile, a person might sit in their basement and play for an hour at a time. Now, the games are always with us.
Many studies that examine the role of women as video game consumers approach them fundamentally as a single monolithic audience, which runs the risk of erasing the distinctive qualities and needs of middle-aged and older women. When you read that 30% of people watching YouTube gaming videos are female or that 21 million people subscribe to the top 10 female gamers on the platform, it might be easy, though debatable, to come away with the impression that women are already reasonably well served and well represented in the world of gaming content. But to what extent do these figures only reflect engagement of younger women? Without studies that break down these numbers across different age demographics, it's difficult to say.
There is an increasing number of influencers on YouTube or Twitch who focus on mobile gaming, but these rising stars are largely male and almost always young. And an examination of the most popular female streamers doesn't appear to overlap much with the age range or game preferences of the women who are devoting the most time and money to video games. This shouldn't come as a surprise, either, since we know that middle-aged women are playing on their phones and often on the go. How many of them are interested in sitting down for hours to watch never-ending game streams? And how interesting would it really be to watch someone else play Pokémon Go for hours? Games like this are only expected to hold players' attention for a few minutes at a time.
Middle-aged women who play casual mobile games deserve to have gaming content that speaks to them on their own terms, and it's not likely that streaming video is going to do the trick. Dedicated websites focused on mobile game news and reviews would likely do well, especially if they were optimized for reading on mobile devices. Smartphone apps that allow users to rate and review their favorite casual games with a social dimension (think Goodreads for games) would also have the potential to be more accessible than YouTube or Twitch. Middle-aged women have shown that they are willing to spend plenty of time and money on their favorite casual games, so why force them to rely on word of mouth to discover new favorites?
The media is paying lots of attention, especially in the wake of Gamergate, to the issue of how to make gaming a more inclusive space for women. And while this impulse is welcome and important, it tends to be concerned with girls and younger women who are actual or potential members of the hardcore gamer audience. Recruiting more female developers and creating games with woman-oriented narratives might revolutionize gaming culture, but it won't necessarily change the lives of women who enjoy stealing a few spare moments to play Candy Crush. Identifying middle-aged women who like mobile games as "casual" gamers shouldn't be a reason to write them off or neglect their unique information needs. But just as gaming culture hasn't been quick to embrace them, they haven't tended to identify with the culture. That's why it will be easier to create new gaming content hubs from scratch with female casual gamers as the target audience than to rope in middle-aged women with a new Rooster Teeth series or a special section on Kotaku.
Just as the average middle-aged female gamer isn't likely to join an Overwatch league, she probably won't be well served by the type of gaming content that speaks to the people who do. But she represents a huge and well-off market segment whose spending power has yet to be fully tapped. King, the hugely successful developer of Candy Crush Saga and other popular casual games, was acquire by Blizzard for $5.9 billion. But the games themselves are only the tip of the iceberg. Content creators have the opportunity to create an entirely independent media ecosystem for casual gamers and her friends if they're brave enough to throw away the blueprint and try some new ideas.
Posted bygavinjohnston67 April 28, 2019 Posted inUncategorizedTags: ad campaign, advertising, advertising insights, advertising strategy, applied anthropology, audiences, casual gamers, consumer insights, consumers, demographics, game platforms, gaming, gaming culture, hardcore gamers, inclusion, market insights, market research, market segment, marketing, marketing communications, marketing platform, marketing strategy, mobile games, mobile gaming, mobile technology, segmentation, strategy, technology, women
Published by gavinjohnston67
Take an ex-chef who's now a full-fledge anthropologist and set him free to conduct qualitative research, ethnography, brand positioning, strategy and sociolinguistics studies and you have Gavin. He is committed to understand design and business problems by looking at them through an anthropological lens. He believes deeply in turning research findings into actionable results that provide solid business strategies and design ideas. It's not an insight until you do something with it. With over 18 years of experience in strategy, research, and communications, he has done research worldwide for a diverse set of clients within retail, legal, banking, automotive, telecommunications, health care and consumer products industries.	View more posts
Food is Storytelling: Easter Ham, Culture, and Marketing
Is the Local Food Movement Over? Hardly
anthrostrategist, Blog at WordPress.com.


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Q: How do you configure xdebug to work with https? I can't get xdebug to catch on a breakpoint using https, but it works fine with http.  Here is the xdebug config in php.ini:
xdebug.remote_enable=on
xdebug.remote_handler=dbgp
xdebug.remote_host=localhost
xdebug.remote_port=9000
xdebug.remote_autostart = 0
xdebug.remote_connect_back = 0
xdebug.idekey = "netbeans-xdebug"

I've looked over the xdebug docs but can't find any mention of https.  Is there any way to make this work?

A: I had the same issue with PHPStorm/IDEA. Had to change host port from 80 to 443 in Servers settings
Preferences -> Languages & Frameworks -> PHP -> Servers

A: Xdebug shouldn't behave differently over SSL, so I suspect the problem to be in NetBeans. Can you try another client and see if that works? You can find a list of clients here: http://xdebug.org/docs/remote

A: Turned out to be an issue with curl passing the request along in the environment.  See here for more help with that.

redpajama_set_name: RedPajamaStackExchange


Physical pain is a part of everyone's life. You can't imagine a life where there would be no cuts or scratches or bruises. However, that doesn't mean if you have to rush to the doctor every time your ankle pains or get yourself a cut. Yes, you heard it right and that also doesn't mean you won't do anything to heal your pain. There are ease pain spells that help one to get rid of the pain conveniently. The post here offers a brief on such spells.
First of all, you should know that such spells are a part of healing spells or cure spells which are one of the most beneficial and powerful spells practiced over years. You can use these spells to heal your bruises or cuts or there are even some pain relief spells that can be used to help another person in your family. There are various ways, methods or chants for pain relief spells.
One of them counts on the power of rain to heal the pain. You have to practice it during some rainy night and outdoors so that the heavy shower gets to touch you physically. Wear something light or thin and avoid thick clothing. Do not draw any circle around you as you pray for the rain to pour harder as otherwise your pain would get trapped in that circle. Concentrate hard and then start chanting the maxim for the pain relief spell. You will get such spells and chants online. Stretch out your arms wide to the sky and let the heavy shower wash your entire body. Keep on chanting the maxim and visualize the pain slowly leaving the body.
You can even cast the pain relief spell indoors. One of the ways is to sit in an empty large room & start deep breathing till you feel some aura surrounding you. Now, concentrate on the pained area & visualize green light travelling to it from the heart. Now, envision the pain as a dark ball which is being drawn out from its source as the green beam waits to engulf it. Once you visualize the entire thing successfully, get back to breathing & relax.
Added to the above mentioned spells, there are spell methods for pain relief which works by you visualizing energy from universe getting absorbed into body completely till its inside you & also surrounds you. Then, you will place hand on the bruised or pained area and start chanting the spell maxim. As you chant, you will have to visualize the energy getting to the wound from your hands which then releases the pain from the body. There are some spells that need to be cast with some props like rose quartz.
It's to mention here that such pain relief spells work mostly on the power of visualization and deep concentration. Moreover, to ensure a successful visualization, you have to have faith in the spell as otherwise it won't work. The stronger your belief is, better would be your healing power.


Woodland Pond At New Paltz is a senior living facility located at 100 Woodland Pond Circle, inside 12561 zip code in Ulster county and offers senior housing in New Paltz, New York. It has capacity of 60 senior citizens. Woodland Pond At New Paltz is licensed with the state of New York, with license number AF0677A.
Culinarians' Home Foundation is a 55 and over senior housing complex situated at 71 Old Tschirky Road in Ulster county and offers senior living in New Paltz, New York. It has capacity of 18 senior apartments. Culinarians' Home Foundation is licensed with the state of New York, with license number AF0229A.
Hudson Valley Senior Residence is a pet-friendly 55+ senior apartment facility located at 80 Washington Avenue, 12401 zip code in Ulster county. Hudson Valley Senior Residence provides senior citizen apartments in Kingston, NY. It includes a total of 48 senior apartment units. It's also a licensed facility, with license # AF0270B.
Valley Vista Adult Home And Assisted Living Program is a senior living community situated at 141 North Road, inside 12528 zip code in the Ulster county. Valley Vista Adult Home And Assisted Living Program offers multiple apartment options for the elderly in Highland, NY, including studio and 1 bedroom. Its New York state license number is AF0429B. Valley Vista Adult Home And Assisted Living Program can accommodate up to 89 senior citizens in total.
Morans Rest Home is a 55 plus senior living community located at 1741 State Route 32 in the 12548 zip code. Morans Rest Home offers New York seniors looking for Ulster County area apartments multiple housing options. Morans Rest Home contains 32 apartments for older adults in total.
Ivy Lodge is a retirement living community in 12477 zip code area, situated at 108 Main Street in the Ulster county. Seniors looking for affordable retirement options in Saugerties, New York will find Ivy Lodge as an excellent option. It has a maximum capacity of 40 senior living apartments.
The New Village View Sp is a 55 and older residence for seniors located at 1 Grove Street, 12528 zip code, belonging to the Ulster area. The New Village View Sp provides housing for senior citizens in Highland, NY. Its full capacity is 80 apartments for the aged. The New Village View Sp is registered in New York under AF0266C license number.
Mountain Valley Manor is a senior apartment facility situated at 373-421 Wilbur Avenue, 12401 zip code. Mountain Valley Manor offers Ulster County residents looking for senior living near Kingston, New York multiple senior housing options. Mountain Valley Manor provides a total of 53 55+ senior apartments. Its New York license # is AF0658A.
Are you in search of assisted senior living in Ulster County? If so, see Assisted Living in Ulster County, NY for all assisted living facilities in the area.
If you are trying to locate a nursing home in Ulster County, please see Nursing Homes in Ulster County, NY for all skilled nursing facilities in the county.
Does your loved one have dementia or Alzheimer's disease? If so, please see Dementia Care in Ulster County, NY and explore all memory care options for dementia and Alzheimer's disease.


text:
Portrait of John Evelyn
John Evelyn (1620 - 1706, British) , Diarist
Robert Nanteuil (1623 - 1678, French) , Artist
Manuscript page number
v3 p83
height (Plate): 244mm
width (Plate): 174mm
Portrait of John Evelyn, engraved by Robert Nanteuil in 1650.
Framed with coloured slips of decorative pattern.
John Evelyn FRS was a founding member of the Royal Society and is well-known for his diaries and his interest in numismatics and antiquities. He published a book on the history and art of copper engraving in 1662, and was the first to give a description in English of the method of engraving called mezzotint. He also published a translation into English of Roland Fréart's works on architecture and painting.
From a set of albums known as Collectanea Newtoniana, a selection of prints, original artwork and manuscripts relating to Newton, collected by Charles Turnor (1768-1853). Turnor was an astronomer, collector and Fellow of the Royal Society. He owned Woolsthorpe Manor (Newton's birthplace).


Luxembourg, November 6, 2018. The quest for a spot in the group stage of the 2019 CEV Volleyball Champions League – Women resumes on Wednesday with two 3rd Round fixtures. Last year's silver medallists CSM Volei Alba BLAJ of Romania host Germany's Allianz MTV STUTTGART while Poland's Budowlani LODZ take on France's ASPTT MULHOUSE VB. There is already much at stake even ahead of the return matches coming up next week with the eventual winners of these double headers qualifying for the 4th Round where they will be joining Europe's top 18 teams. Make sure you follow the CEV's social media channels for further updates under the official hashtag #CLVolleyW!
Last year's silver medal winners CSM Volei Alba BLAJ of Romania could go for a repeat of the 2018 gold medal match with VakifBank ISTANBUL if they edge their German opponent in the 3rd Round. The side emerging victorious from this double header will indeed move to Pool A for the 4th Round of the competition, playing there titleholders VakifBank as well as BEZIERS VB of France and Bulgaria's Maritza PLOVDIV.
The organisers expect many fans to flock to Transilvania Hall on Wednesday night so that the home team will enjoy the perfect ambiance to make it a step further towards reaching the pool stage of Europe's elite club competition.
CSM Volei Alba BLAJ have a perfect record of four wins in as many matches they have contested this season so far – two in the CEV Volleyball Champions League and another two in the Romanian national league.


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Knights of Malta elect new leader
The Order elected Fra' Giacomo dalla Torre, an Italian, to be its interim leader for the next year.
Mon May 1, 2017 - 10:46 am EST
By Claire Chretien
Follow Claire
ROME, April 29, 2017 (LifeSiteNews) – The Order of Malta elected Fra' Giacomo dalla Torre, an Italian, to be its interim leader for the next year.
The Order of Malta, which is a sovereign state, has been in turmoil after it sacked a high-ranking official for distributing condoms and contraceptives in the developing world through its international charity. The official, Albrecht von Boeselager, had refused to step down so was fired for violating his vow of obedience.
Pope Francis then personally asked the order's highest leader, Fra' Matthew Festing, to resign. He did, and then Pope Francis reinstated the condom promoter and took over the sovereign order. He appointed a papal delegate to oversee it; the order's Cardinal Patron, Cardinal Raymond Burke, is "de facto" suspended, according to von Boeselager.
Pope Francis asked Festing not to come to Rome for his successor's election, but then reversed this decision. Members of the order told the National Catholic Register's Ed Pentin that Festing's absence would have invalidated the election. There were rumors Festing was favored to be re-elected, but he didn't make it onto the ballot of three finalists.
Giacomo dalla Torre's title will be Lieutenant of the Grand Master. Grand Master is a lifelong position, which was one of the reasons why the Pope asking Festing to resign was so shocking.
Matthew Festing's name not on the "terna" of list of three candidates for tomorrow's Knights of Malta vote.
— Hilary White (@Hilarityjane66) April 28, 2017
Three names:
Fra Carlo d'Ippolito di Sant'Ippolito
Fra' Ludwig Hoffmann von Rumerstein
Fra' Giacomo Dalla Torre del Tempio di Sanguinetto
#KnightsofMalta elect Fra Giacomo della Torre of Rome to lead order as Lieutenant of the Grand Master for 1 year period pic.twitter.com/rCvEcZmYGO
— Junno Arocho Esteves (@arochoju) April 29, 2017
#PopeFrancis has been informed of election of Fra Giacomo Dalla Torre. Photo of new head & today's election released by #KnightsofMalta pic.twitter.com/ghC6oOpwnl
albrecht von boeselager, catholic, catholic church, giacomo dalla torre, knights of malta, matthew festing, order of malta, pope francis, sovereign military order of malta
Knights of Malta elect new leader Knights of Malta elect new leader News By Claire Chretien


Your Townships adventure starts here.
Take your pick: adrenaline packed or slow and contemplative?
Choose from a wide array of indoor and outdoor activities to please young and old.
Treat yourself to massages, body treatments, Nordic baths and other sensory delights.
Discover our cultural vitality with a wide range of special events.
Let your imagination run free at galleries, theatres, museums and workshops.
All are sure to please even the most discerning of palates. Bon appétit!
Scour our markets, boutiques and other hidden gems to score incredible finds.
To each mountain its experience! Skiing or snowboarding, you will love hitting the slopes, whichever the ski resort you will vote for!
Explore our great outdoor spaces at your own beat. Let yourself be charmed by our landscapes. And breathe!
Enjoy a traditional meal and maple taffy on snow.
What to do this weekend?
Lodging options to suit any taste and budget.
Stunning locations and outstanding service come together for a bliss-inducing stay.
Get up close and personal with life in the Townships.
Think outside the box with out of the ordinary accommodations.
Custom comfort near the city or in nature.
Abundant amenities in the heart of nature.
Kick back and relax as a family with all-inclusive vacation options.
Experience something different by choosing unique lodging.
The only thing better than a day at the spa? Several days at the spa!
If you, like thousands of visitors annually, plan on hiking in the region, know that your efforts will be rewarded by our world-class hospitality.
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