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ANU database
Biagi (transcription of data from SF Biagi's Fortran code, Magboltz.)
Biagi-v7.1 (Magboltz version 7.1)
Bordage database
BSR (Quantum-mechanical calculations by O. Zatsarinny and K. Bartschat)
Budapest (Budapest Drift Tube Database)
CCC database
CDAP (State-to-state electron-impact excitation rate coefficients)
Christophorou database
COP (Complex Optical Potential)
Dutton database
eMol-LeHavre (eMol group LeHavre)
ETHZ (ETH Zurich, High Voltage Laboratory)
FLINDERS database
Hayashi database
Heidelberg database
IST-Lisbon database
Itikawa database
LAPLACE (measurements after 1975)
Laporta (Laporta_DB)
Morgan (Kinema Research & Software)
NGFSRDW database
Phelps database
Puech database
QUANTEMOL database
SIGLO database
TRINITI database
UBC database
UNAM database
UT (University of Tartu)
Viehland database
XJTUAETLab (Xi'an Jiaotong University, Advanced Electrical Technology Laboratory)
BOLSIG+ solver
PERMLINK: www.lxcat.net/ANU
DESCRIPTION: Data compilation from the Australian National University
CONTACT: Stephen Buckman, stephen.buckman@@anu.edu.au
DIFFERENTIAL SCATTERING CROSS SECTIONS
Species: e + Ar [10], C2F4 [28], C2H4 [26], C4F8 [26], C4H8O [8], C4H8O2 [5], C6F6 [10], C6H6 [15], CH4 [17], CO [20], CO2 [17], COF2 [17], F6S [11], H2 [14], H2O [9], H2S [12], HCOOH [7], He [8], Kr [6], N2 [28], N2O [38], Ne [8], NH3 [9], NO [23], O2 [12], SO2 [8], Xe [15]
Updates: 2014-11-07 … 2015-12-08
Downloads: 2017 times from 2016-10-11
PERMLINK: www.lxcat.net/Biagi
DESCRIPTION: These data were transcribed from S.F. Biagi's FORTRAN code, MagBoltz, versions 8.9 and later. The exact version number is given for each species. At this time, the Biagi database contains cross sections for rare gases, for a few simple molecules, and for SF6. The transcription of cross sections for other gases is in progress. These data were compiled for use a Monte Carlo simulation (or multi-term Boltzmann code), but their use in a 2-term Boltzmann solver gives reasonably accurate results in most cases. The the LXCat data tables do not always have the same energy resolution as the original data in the MagBoltz code. This limited energy resolution can introduce small (1%) differences in the calculated drift velocity at low E/N. For history and detailed notes, see http://consult.cern.ch/writeup/magboltz/ Oct 2011 : update of Ar and Kr data taken from MagBoltz version 8.97 Nov 2011 : small changes in Xe ionization cross sections, taken from MagBoltz v8.97 March 2015: cross sections for SF6 were transcribed from Magboltz version 10.6 from February 2014.
CONTACT: email Stephen.biagi@@hotmail.co.uk
HOW TO REFERENCE: Fortran program, MAGBOLTZ, S.F. Biagi. The version number of MAGBOLTZ from which the cross sections were transcribed is provided in the comment for each species. This version number must be included in the reference.
SCATTERING CROSS SECTIONS
Species: e + Ar [46], CO2 [92], CO2(bend mode) [1], D2 [15], H2 [105], He [51], Kr [53], N2 [46], Ne [47], O2 [15], SF6 [50], Xe [52]
Downloads: 44732 times from 2010-11-24
PERMLINK: www.lxcat.net/Biagi-v7.1
DESCRIPTION: For the moment, this data base contains cross sections for the rare gases. The excitation cross sections are grouped into a few effective excitation levels. For more detailed cross sections with multiple levels, see Biagi 8.9. These cross sections were compiled for use in a Monte Carlo (or multi-term Boltzmann) code. For history and detailed notes, see http://consult.cern.ch/writeup/magboltz/
CONTACT: COPYRIGHT 2004 STEPHEN FRANCIS BIAGI
HOW TO REFERENCE: Cross sections extracted from PROGRAM MAGBOLTZ, VERSION 7.1 JUNE 2004
Species: e + Ar [5], He [4], Kr [6], Ne [11], Xe [6]
PERMLINK: www.lxcat.net/Bordage
DESCRIPTION: All the cross sections were derived by using a multiterm solution of the Boltzmann equation in the approximation of the hydrodynamic regime. (see for exemple Ségur P., Yousfi M., Kadri M. and Bordage M.C., "A survey of the numerical methods currently in use to describe the motion of an electron swarm in a weakly ionised gas", Transport Theory and Statistical. Physics, Vol-15, Issue-6&7, pp-705-757, 1986. And Ségur P. and Bordage M.C., "Recent advances in the solution of the Boltzmann equation for the motion of electrons in a weakly ionized gas", Invited paper, XIX ICPIG, Belgrade, 86-107, 1989.)
CONTACT: Marie-Claude Bordage,
Laplace Laboratory Toulouse, France.
Email: marie-claude.bordage@@laplace.univ-tlse.fr
Species: e + CF4 [7], CHF3 [8], Si(CH3)4 [6]
PERMLINK: www.lxcat.net/BSR
DESCRIPTION: The results in this database are from non-relativistic (LS-coupling), semi-relativistic (Breit-Pauli), and full-relativistic (Dirac) B-spline R-matrix (close-coupling) treatments of electron collisions with a number of species. Individually optimized, term-dependent sets of non-orthogonal valence orbitals are used to account for the potentially strong term dependence in the one-electron valence orbitals, especially for the heavy noble gases. The predictions have been validated against a number of benchmark experimental data measured in crossed-beam setups. Very good agreement is generally achieved in the near-threshold resonance regime, where the excitation process is often dominated by negative-ion resonances. For e-Ar collisions, angle-differential cross sections are also available. These were obtained in the semi-relativistic framework.
CONTACT: Kathryn R. Hamilton or Klaus Bartschat
Dept. of Physics & Astronomy; Drake University
Des Moines, Iowa 50311, USA
Email: kathryn.hamilton@drake.edu; klaus.bartschat@drake.edu
HOW TO REFERENCE: "BSR: B-spline atomic R-matrix codes." O. Zatsarinny 2006 Comp. Phys. Commun. 174 273.
"The B-spline R-matrix method for atomic processes: application to atomic structure, electron collisions and photoionization."
O. Zatsarinny and K. Bartschat 2013 J. Phys. B: At. Mol. Opt. Phys. 46 112001.
The BSR codes are publicly available through https://github.com › zatsaroi › BSR3. Compiled versions with instructions and test cases are available from the Atomic and Molecular Gateway at https://ampgateway.org/home/home1/homec1/documentation_copy/bsr-documentation/.
Species: e + Ar {30} « Ar [67], Ar(3d'[3/2]2) [2], Ar(3d'[5/2]2) [3], Ar(3d'[5/2]3) [1], Ar(3d[1/2]0) [15], Ar(3d[1/2]1) [14], Ar(3d[3/2]1) [6], Ar(3d[3/2]2) [13], Ar(3d[5/2]2) [8], Ar(3d[5/2]3) [7], Ar(3d[7/2]3) [10], Ar(3d[7/2]4) [12], Ar(4p'[1/2]0) [16], Ar(4p'[1/2]1) [17], Ar(4p'[3/2]1) [19], Ar(4p'[3/2]2) [18], Ar(4p[1/2]0) [20], Ar(4p[1/2]1) [25], Ar(4p[3/2]1) [22], Ar(4p[3/2]2) [21], Ar(4p[5/2]2) [23], Ar(4p[5/2]3) [24], Ar(4s'[1/2]0) [27], Ar(4s'[1/2]1) [26], Ar(4s[3/2]1) [28], Ar(4s[3/2]2) [29], Ar(5s'[1/2]0) [5], Ar(5s'[1/2]1) [4], Ar(5s[3/2]1) [9], Ar(5s[3/2]2) [11] », Be {19} « Be [24], Be(2p(2)1D2) [14], Be(2p(2)3P2) [12], Be(2s_2p_1P) [20], Be(2s_2p_3P) [21], Be(2s_3d_1D) [9], Be(2s_3d_3D) [10], Be(2s_3p_1P) [11], Be(2s_3p_3P) [13], Be(2s_3s_1S) [15], Be(2s_3s_3S) [16], Be(2s_4d_1D) [1], Be(2s_4d_3D) [4], Be(2s_4f_1F) [2], Be(2s_4f_3F) [3], Be(2s_4p_1P) [5], Be(2s_4p_3P) [6], Be(2s_4s_1S) [7], Be(2s_4s_3S) [8] », C {63} « C [68], C(2p(2)_1D) [24], C(2p(2)_1D2) [40], C(2p(2)_1S) [23], C(2p(2)_1S0) [39], C(2p(2)_3P1) [42], C(2p(2)_3P3) [41], C(2p3d_1Do) [8], C(2p3d_1Fo) [3], C(2p3d_1Po) [2], C(2p3d_3Do) [5], C(2p3d_3Fo) [6], C(2p3d_3Po) [1], C(2p3p_1D) [11], C(2p3p_1P) [15], C(2p3p_1S) [10], C(2p3p_3D) [14], C(2p3p_3P) [12], C(2p3p_3S) [13], C(2p3s_1Po) [19], C(2p3s_3Po) [20], C(2p4s_1Po) [4], C(2p4s_3Po) [7], C(2p_3d_1D2) [16], C(2p_3d_1F3) [5], C(2p_3d_1P1) [4], C(2p_3d_3D1) [10], C(2p_3d_3D2) [8], C(2p_3d_3D3) [7], C(2p_3d_3F2) [12], C(2p_3d_3F3) [11], C(2p_3d_3F4) [9], C(2p_3d_3P0) [1], C(2p_3d_3P1) [2], C(2p_3d_3P2) [3], C(2p_3p_1D2) [21], C(2p_3p_1P1) [29], C(2p_3p_1S0) [20], C(2p_3p_3D1) [28], C(2p_3p_3D2) [27], C(2p_3p_3D3) [26], C(2p_3p_3P0) [24], C(2p_3p_3P1) [23], C(2p_3p_3P2) [22], C(2p_3p_3S1) [25], C(2p_3s_1P1) [33], C(2p_3s_3P0) [36], C(2p_3s_3P1) [35], C(2p_3s_3P2) [34], C(2p_4s_1P1) [6], C(2p_4s_3P0) [15], C(2p_4s_3P1) [14], C(2p_4s_3P2) [13], C(2s2p(3)_3Do) [18], C(2s2p(3)_3Po) [9], C(2s2p(3)_5So) [21], C(2s_2p(3)_3D1) [32], C(2s_2p(3)_3D2) [31], C(2s_2p(3)_3D3) [30], C(2s_2p(3)_3P0) [19], C(2s_2p(3)_3P1) [18], C(2s_2p(3)_3P2) [17], C(2s_2p(3)_5S2) [37] », F {8} « F [28], F(2p^4(^1D)3s) [17], F(2p^4(^3P)3d) [69], F(2p^4(^3P)3p) [123], F(2p^4(^3P)3s) [49], F(2p^4(^3P)4p) [33], F(2p^4(^3P)4s) [31], F(2p^4(^3P)5s) [3] », Kr [70], N {27} « N [29], N(2p2_1D_3s_2De) [15], N(2p2_3P_3d_2De) [7], N(2p2_3P_3d_2Fe) [9], N(2p2_3P_3d_2Pe) [12], N(2p2_3P_3d_4De) [8], N(2p2_3P_3d_4Fe) [11], N(2p2_3P_3d_4Pe) [10], N(2p2_3P_3p_2Do) [17], N(2p2_3P_3p_2Po) [16], N(2p2_3P_3p_2So) [21], N(2p2_3P_3p_4Do) [20], N(2p2_3P_3p_4Po) [19], N(2p2_3P_3p_4So) [18], N(2p2_3P_3s_2Pe) [23], N(2p2_3P_3s_4Pe) [24], N(2p2_3P_4p_2Do) [3], N(2p2_3P_4p_2Po) [1], N(2p2_3P_4p_2So) [6], N(2p2_3P_4p_4Do) [5], N(2p2_3P_4p_4Po) [4], N(2p2_3P_4p_4So) [2], N(2p2_3P_4s_2Pe) [13], N(2p2_3P_4s_4Pe) [14], N(2p3_2Do) [28], N(2p3_2Po) [27], N(2s_2p4_4Pe) [22] », Ne [34], Xe [76]
Species: e + Ar [62]
PERMLINK: www.lxcat.net/Budapest
DESCRIPTION: This database containes experimental swarm data obtained with a Scanning Drift Tube apparatus operated at the Wigner Research Centre for Physics, Budapest, Hungary.
CONTACT: Zoltan Donko, donko.zoltan@wigner.hu
HOW TO REFERENCE: The description of the experimental apparatus is given in [I. Korolov, M. Vass, N. Kh. Bastykova and Z. Donko: "A scanning drift tube apparatus for spatiotemporal mapping of electron swarms" Rev. Sci. Instrum. 87, 63102 (2016)]. For an update on the details of the data acquisition see [N. R. Pinhao, D. Loffhagen, M. Vass, P. Hartmann, I. Korolov, S. Dujko, D. Bosnjakovic, Z. Donko: "Electron swarm parameters in C2H2, C2H4 and C2H6: measurements and kinetic calculations" Plasma Sources Sci. Technol. 29, 045009 (2020)].
SWARM / TRANSPORT DATA
Species: e + C2H2 [3], C2H4 [4], C2H6 [4], CH4 [3], CO [4], CO2 [3], D2 [3], N2:O2 [1]
Downloads: 454 times from 2021-05-12
PERMLINK: www.lxcat.net/CCC
DESCRIPTION: The convergent close-coupling method (CCC) is a non-relativistic formulation of the close coupling equations that solves for the scattering T-matrix in momentum space. The CCC database contains angle-integrated cross sections of electron scattering from atomic hydrogen H [1] and helium He [2] atoms and the molecular hydrogen ion H2+ [3]. For H and He the full set of cross sections (elastic, momentum-transfer, excitation, and ionization cross sections) are available for scattering from the ground state. The angle-differential cross sections and cross sections for scattering from excited states are available on request from the authors. For H2+ the CCC data base provides results from adiabatic-nuclei close-coupling calculations of hot (vibrationally excited) H2+. Collision data of H2+ and its isotopologues was obtained for scattering from each vibrational state of the electronic ground state and for the distribution of vibrational levels weighted according to the Frank-Condon (FC) factors. In the near future the CCC database will add comprehensive collision data of electron scattering from molecular hydrogen H2. Presently the database contains total cross section and cross sections for elastic scattering and ionization in the energy range from 0.1 to 300 eV and differential cross sections at 17.5 eV for the first seven states of H2 [4].
CONTACT: Igor Bray and Dmitry V Fursa
HOW TO REFERENCE: 1. "Convergent close-coupling calculations of electron-hydrogen scattering" Igor Bray and Andris T. Stelbovics, Phys Rev A, 46, 6995-7011 (1992) 2. "Calculation of electron-helium scattering" Dmitry V. Fursa and Igor Bray, Phys. Rev. A 52, 1279-1297 (1995). 3. "Electron scattering from the molecular hydrogen ion and its isotopologues" Mark C. Zammit, Dmitry V. Fursa, and Igor Bray, Phys. Rev. A 90, 022711 (2014). 4. "Complete Solution of Electronic Excitation and Ionization in Electron-Hydrogen Molecule Scattering" Mark C. Zammit, Jeremy S. Savage, Dmitry V. Fursa, and Igor Bray, accepted: Phys. Rev. Lett. 116, 233201 (2016)
Species: e + D2 [1], DT [1], H {10} « H(1S) [11], H(2P) [11], H(2S) [11], H(3D) [11], H(3P) [11], H(3S) [11], H(4D) [11], H(4F) [11], H(4P) [11], H(4S) [12] », H2 [25], HD [1], He(s1S) [20], HT [1], T2 [1], D2+ {15} « D2+(1sSg,v=0) [4], D2+(1sSg,v=1) [4], D2+(1sSg,v=10) [4], D2+(1sSg,v=11) [4], D2+(1sSg,v=12) [4], D2+(1sSg,v=13) [4], D2+(1sSg,v=2) [4], D2+(1sSg,v=3) [4], D2+(1sSg,v=4) [4], D2+(1sSg,v=5) [4], D2+(1sSg,v=6) [4], D2+(1sSg,v=7) [4], D2+(1sSg,v=8) [4], D2+(1sSg,v=9) [4], D2+(1sSg,v=FC) [4] », DT+ {16} « DT+(1sSg,v=0) [4], DT+(1sSg,v=1) [4], DT+(1sSg,v=10) [4], DT+(1sSg,v=11) [4], DT+(1sSg,v=12) [4], DT+(1sSg,v=13) [4], DT+(1sSg,v=14) [4], DT+(1sSg,v=15) [4], DT+(1sSg,v=2) [4], DT+(1sSg,v=3) [4], DT+(1sSg,v=4) [4], DT+(1sSg,v=5) [4], DT+(1sSg,v=6) [4], DT+(1sSg,v=7) [4], DT+(1sSg,v=8) [4], DT+(1sSg,v=9) [4] », H2+ {11} « H2+(1sSg,v=0) [4], H2+(1sSg,v=1) [4], H2+(1sSg,v=2) [4], H2+(1sSg,v=3) [4], H2+(1sSg,v=4) [4], H2+(1sSg,v=5) [4], H2+(1sSg,v=6) [4], H2+(1sSg,v=7) [4], H2+(1sSg,v=8) [4], H2+(1sSg,v=9) [4], H2+(1sSg,v=FC) [4] », HD+ {12} « HD+(1sSg,v=0) [4], HD+(1sSg,v=1) [4], HD+(1sSg,v=10) [4], HD+(1sSg,v=11) [4], HD+(1sSg,v=2) [4], HD+(1sSg,v=3) [4], HD+(1sSg,v=4) [4], HD+(1sSg,v=5) [4], HD+(1sSg,v=6) [4], HD+(1sSg,v=7) [4], HD+(1sSg,v=8) [4], HD+(1sSg,v=9) [4] », HT+ {13} « HT+(1sSg,v=0) [4], HT+(1sSg,v=1) [4], HT+(1sSg,v=10) [4], HT+(1sSg,v=11) [4], HT+(1sSg,v=12) [4], HT+(1sSg,v=2) [4], HT+(1sSg,v=3) [4], HT+(1sSg,v=4) [4], HT+(1sSg,v=5) [4], HT+(1sSg,v=6) [4], HT+(1sSg,v=7) [4], HT+(1sSg,v=8) [4], HT+(1sSg,v=9) [4] », T2+ {19} « T2+(1sSg,v=0) [4], T2+(1sSg,v=1) [4], T2+(1sSg,v=10) [4], T2+(1sSg,v=11) [4], T2+(1sSg,v=12) [4], T2+(1sSg,v=13) [4], T2+(1sSg,v=14) [4], T2+(1sSg,v=15) [4], T2+(1sSg,v=16) [4], T2+(1sSg,v=17) [4], T2+(1sSg,v=2) [4], T2+(1sSg,v=3) [4], T2+(1sSg,v=4) [4], T2+(1sSg,v=5) [4], T2+(1sSg,v=6) [4], T2+(1sSg,v=7) [4], T2+(1sSg,v=8) [4], T2+(1sSg,v=9) [4], T2+(1sSg,v=FC) [4] »
Species: e + H2 [19]
PERMLINK: www.lxcat.net/CDAP
DESCRIPTION: State-to-state electron-impact excitation rate coefficients of atoms, ions, and small molecules can be obtained by examining collisional-radiative modelling by plasma experiments under specific conditions with combination of OES, LAS, probe, and microwave experiments. This method orignied from the so-called CDAP method in afterglow discharge of argon CCP and is expended to other kinds of miniaturized ECR and ICP.These rate coefficient data are available for modelling of non-equlibrium plasma with excited state kinetics considered as well as for determining electron temperature and density by the OES line-ratio method.
Xi-Ming Zhu (simon.ximing.zhu@outlook.com) ,Yan-Fei Wang (arvin.yanfei.wang@outlook.com) and Lu Wang (hans.lu.wang@outlook.com) Harbin Institute of Technology, Harbin 150080, China
Yi-Kang Pu (puyikang@mail.tsinghua.edu.cn) Tsinghua University, Beijing 100084, China
HOW TO REFERENCE:
Xi-Ming Zhu, Yan-Fei Wang, Yang Wang, Da-Ren Yu, Oleg Zatsarinny, Klaus Bartschat, Tsanko Vaskov Tsankov, and Uwe Czarnetzki 2019 Plasma Sources Sci. Technol. 28 105005.
Xi-Ming Zhu, Zhi-Wen Cheng, Emile Carbone, Yi-Kang Pu, and Uwe Czarnetzki 2016 Plasma Sources Sci. Technol. 25 043003.
Species: e + Ar {4} « Ar(1s2) [7], Ar(1s3) [10], Ar(1s4) [10], Ar(1s5) [21] », Xe+ (5p5 E=0eV) [21], Xe+ {22} « Xe+(5p46p E=13.860eV) [2], Xe+(5p46p E=13.881eV) [2], Xe+(5p46p E=14.074eV) [2], Xe+(5p46p E=14.094eV) [2], Xe+(5p46p E=14.098eV) [2], Xe+(5p46p E=14.479eV) [2], Xe+(5p46p E=14.93eV) [2], Xe+(5p46p E=15.024eV) [2], Xe+(5p46p E=15.08eV) [2], Xe+(5p46p E=15.264eV) [2], Xe+(5p46p E=15.282eV) [2], Xe+(5p46p E=15.41eV) [2], Xe+(5p46p E=15.445eV) [2], Xe+(5p46p E=15.977eV) [2], Xe+(5p46p E=16.077eV) [2], Xe+(5p46p E=16.126eV) [2], Xe+(5p46p E=16.356eV) [2], Xe+(5p46p E=16.392eV) [2], Xe+(5p46p E=16.458eV) [2], Xe+(5p46p E=18.378eV) [2], Xe+(5p46p E=18.497eV) [2], Xe+(5p5 E=1.3064eV) [21] »
Downloads: 75 times from 2017-08-13
PERMLINK: www.lxcat.net/Christophorou
DESCRIPTION: A compilation of molecular data assembled and evaluated by Loucas G. Christophorou and collaborators.
CONTACT: These data were imported into LXCat by Sergey Pancheshnyi, ABB Switzerland Ltd., 2015-2016.
HOW TO REFERENCE: Please refer to these data using the sources cited for each gas.
Species: e + CF3I [9], SF [1], SF2 [1], SF3 [1], SF4 [1], SF5 [1], SF6 [14]
Species: e + CF3I [8], SF6 [21]
Species: e + SF6 [9]
PERMLINK: www.lxcat.net/Community
DESCRIPTION: This database contains data from various contributors who have not yet set up an individual database. This is usually for contributors who have small amounts of data to upload to LXCat.
CONTACT: The LXCat team maintains this database. Contact info@lxcat.net.
HOW TO REFERENCE: The references are included in each data group and for each species.
Species: e + CH4 [16]
Downloads: 1 times from 2022-02-19
PERMLINK: www.lxcat.net/COP
DESCRIPTION: The Complex Optical Potential (COP) data includes cross sections for total elastic, momentum transfer and viscosity cross sections for elastic scattering of electrons from the heavy noble gases from threshold at zero energy to 1 keV. This method allows for the loss of flux from the incident channel into the excitation and ionization channels when these inelastic processes are energetically possible. The publications which include these results also contain analytic fits to the data over the whole energy range. These calculations were carried out by R. P. McEachran, Australian National University, Canberra, Australia and A. D. Stauffer, York University, Toronto, Canada.
CONTACT: Please contact A. D. Stauffer (stauffer@yorku.ca) for further information.
Species: e + Ar [3], Kr [3], Xe [3]
PERMLINK: www.lxcat.net/Dutton
DESCRIPTION: This is an experimental database which includes, at present, data for rare gases from J. Dutton, "Survey of Electron Swarm Data", J. Phys. Chem. Ref. Data, 4, 577, 1975. This publication also includes data for molecular gases, and their transcription into this database is in progress. These data were imported into LXCat by Sanchita Chowdhury, LAPLACE, Toulouse, France, 2010-2011.
HOW TO REFERENCE: Jack Dutton, "Survey of Electron Swarm Data", J. Phys. Chem. Ref. Data, 4, 577, 1975
Species: e + Air [10], Ar [17], CO [9], CO2 [20], H2 [33], He [13], Kr [4], N2 [36], Ne [8], O2 [27], Xe [4]
PERMLINK: www.lxcat.net/eMol-LeHavre
DESCRIPTION: A compilation of atomic and molecular data, calculated within eMol LeHavre group. The data were obtained for the electron temperature range up to 5 eV in electron scattering processes in cold plasma. The database contains cross sections sets and Maxwell rate coefficients. Data are permanently updated. These data were imported into LXCat by Felix Iacob.
CONTACT: Felix Iacob, West University of Timisoara, email: felix.iacob@e-uvt.ro
HOW TO REFERENCE: Please refer to these data using the sources cited for each species.
Species: e + BeH+ [1], N2+ [1]
Species: e + BeH+ [1]
PERMLINK: www.lxcat.net/ETHZ
DESCRIPTION: This is a database of electron swarm parameters obtained with pulsed Townsend experiments at the High Voltage Laboratory of ETH Zurich, Switzerland. These experiments enable us to measure electron and ion swarm parameters in arbitrary gases, such as the reaction rates of ionization, attachment, detachment and conversion, the electron and ion mobilities, and the longitudinal electron diffusion coefficient. Our group is open for joint projects where such measurements are needed. Please contact us (cfranck@ethz.ch) in case you are looking for data on gases that are not available or need updates. Currently, the database contains the swarm parameters of atmospheric gases, fluorinated gases, and gas mixtures. Measurements are ongoing and the database is regularly updated.
CONTACT: A. Chachereau (alisec@ethz.ch), C. M. Franck (cfranck@ethz.ch)
Species: e + 2-C4F8:Ar [5], 2-C4F8:CO2 [6], 2-C4F8:N2 [5], Ar [12], c-C4F8O:Ar [4], c-C4F8O:CO2 [8], c-C4F8O:N2 [7], C3HF5 [10], C3HF5:CO2 [47], C3HF5:N2 [61], C4F7N [15], C4F7N:CO2 [64], C4F7N:CO2:O2 [36], C4F7N:N2 [40], C5F10O [5], C5F10O:CO2 [28], C5F10O:CO2:O2 [18], C5F10O:N2 [33], C5F10O:N2:O2 [33], CF3-O-CF=CF2 [4], CH3CN [1], CO2 [31], CO2:N2 [60], CO2:O2 [43], HFC227ea [27], HFC227ea:CO2 [61], HFC227ea:N2 [84], HFO1234ze [14], HFO1234ze:Ar [9], HFO1234ze:CO2 [36], HFO1234ze:N2 [42], HFO1234ze:SF6 [42], HFPO:CO2 [12], HFPO:N2 [12], N2 [21], N2:O2 [17], N2O [13], O2 [6], SF5CF3 [6], SF5CF3:CO2 [24], SF5CF3:N2 [45]
PERMLINK: www.lxcat.net/FLINDERS
CONTACT: Laurence Campbell, Flinders University
Species: e + CO2 [8], N2 [48], NO [12], O2 [10]
PERMLINK: www.lxcat.net/Hayashi
DESCRIPTION: These data sets were derived by comparing calculated swarm parameters, using as input the cross sections sets in this database, with measurements.
CONTACT: leanne.pitchford@@laplace.univ-tlse.fr
Species: e + Ar [27], C2H2 [8], C2H4 [7], C2H6 [7], CCl2F2 [6], CCl4 [8], CF4 [7], CH4 [6], CO2 [11], H2O [8], HCl [6], N2O [9], NH3 [8], NO [10], Si2H6 [7], SiH4 [7], SO2 [6], Xe [16]
PERMLINK: www.lxcat.net/Heidelberg
DESCRIPTION: This is a database of electron transport parameters measured at the University Heidelberg in the years 1978 to 1996. Different electron swarm experiments were setup by Bernhard Schmidt and co-workers which allowed to measure electron transport parameters in pure electric and perpendicular crossed electric and magnetic fields. This database contains only those data for B=0. Additional swarm data for non-zero B fields will be made available in tabular and graphical form in the NOTES section of LXCat when resources become available.
CONTACT: Malte Hildebrandt, malte.hildebrandt@psi.ch
Species: e + Ar:C2H6O [1], C2H4 [3], C2H6 [5], C2H6O [1], C3H6 [6], C3H8 [3], C4H10:Ar [3], C4H10:He [3], CH4 [8], CO2 [3], CO2:Ar [3], CO2:Ne [3], D2 [2], H2 [7], H2:Ar [1], H2:Kr [1], H2:Xe [1], N2 [3], N2:Ar [3]
PERMLINK: www.lxcat.net/IST-Lisbon
DESCRIPTION: IST-Lisbon database contains up-to-date electron-neutral scattering cross sections (together with the measured swarm parameters used to validate these data), resulting from the research effort of the Group N-Plasmas Reactive: Modelling and Engineering (N-PRiME) with IPFN/IST (Instituto de Plasmas e Fusao Nuclear / Instituto Superior Tecnico), Lisbon, Portugal.
The data, compiled from the literature, correspond to contributions from different authors (see detailed references in the database). For each gas the database presents a COMPLETE SET of cross sections, validated against measured swarm parameters by solving the two-term homogeneous electron Boltzmann equation. In most cases, predictions are in agreement with measurements within 1-20%, for reduced electric fields E/N ~ 1e-4 - 500 Td. To improve predictions at low E/N, some sets need to be completed with rotational cross sections, also available in the database.
CONTACT: LL Alves and V Guerra
e-mail: llalves@@tecnico.ulisboa.pt
HOW TO REFERENCE: L.L. Alves, ''The IST-Lisbon database on LXCat'' J. Phys. Conf. Series 2014, 565, 1
Species: e + Ar [39], CH4 [9], CO [21], CO-rot [17], CO2 [16], CO_anis [80], H2 [22], He [44], Hydrogen [82], N2 [26], Nitrogen [85], O2 [15], Oxygen [912]
Species: e + Ar [17], CH4 [16], H2 [7], He [21], N2 [11]
PERMLINK: www.lxcat.net/Itikawa
DESCRIPTION: A set of recommended cross section data (angle integrated) for electron collisions with H2, N2, O2, CO, H2O, and CO2. The data are taken from the tables in the references listed for each species. The recommendations are based on available experimental data. In that sense, the present sets of cross sections are not complete. Uncertainty estimates are given in the references.
CONTACT: Yukikazu Itikawa
Species: e + CO [18], CO2 [16], H2 [17], H2O [28], N2 [22], NO [17], O2 [21]
PERMLINK: www.lxcat.net/LAPLACE
DESCRIPTION: These data were extracted from articles published after the 1975 or not appearing in the review article by Dutton (and the associated "Dutton" database). The data in this database were digitized by S Chowdhury (LAPLACE, Toulouse) from figures in the publications or from data tables if tables were provided in the publications.
Species: e + Air [2], Air:H2O [6], Ar [27], C2F6 [3], C2H4 [3], C2H6 [3], C3F8 [2], C3H6(Cyclo) [3], C3H6(Propene) [3], C3H8 [3], CF3I [2], CF4 [24], CH4 [8], CHF3 [2], CO [6], CO2 [5], CO2:Ar [4], H2 [4], H2:Ne [2], H2O [3], He [20], He:H2 [1], Kr [19], n-C4F10 [1], N2 [18], N2:Ar [3], N2O [2], N2O:Ar [2], Ne [8], O2 [17], O2:Ar [6], Xe [27], Xe:H2 [3], Xe:N2 [3]
PERMLINK: www.lxcat.net/Laporta
DESCRIPTION: A compilation of vibrationally resolved cross sections for electron-molecule scattering based on R-Matrix calculation
CONTACT: Vincenzo Laporta, vincenzo.laporta@cnr.it
HOW TO REFERENCE: Please use the references cited for each species.
Species: e + D2 {71} « D2(B,v=0) [53], D2(B,v=1) [52], D2(B,v=10) [43], D2(B,v=11) [42], D2(B,v=12) [41], D2(B,v=13) [40], D2(B,v=14) [39], D2(B,v=15) [38], D2(B,v=16) [37], D2(B,v=17) [36], D2(B,v=18) [35], D2(B,v=19) [34], D2(B,v=2) [51], D2(B,v=20) [33], D2(B,v=21) [32], D2(B,v=22) [31], D2(B,v=23) [30], D2(B,v=24) [29], D2(B,v=25) [28], D2(B,v=26) [27], D2(B,v=27) [26], D2(B,v=28) [25], D2(B,v=29) [24], D2(B,v=3) [50], D2(B,v=30) [23], D2(B,v=31) [22], D2(B,v=32) [21], D2(B,v=33) [20], D2(B,v=34) [19], D2(B,v=35) [18], D2(B,v=36) [17], D2(B,v=37) [16], D2(B,v=38) [15], D2(B,v=39) [14], D2(B,v=4) [49], D2(B,v=40) [13], D2(B,v=41) [12], D2(B,v=42) [11], D2(B,v=43) [10], D2(B,v=44) [9], D2(B,v=45) [8], D2(B,v=46) [7], D2(B,v=47) [6], D2(B,v=48) [5], D2(B,v=49) [4], D2(B,v=5) [48], D2(B,v=6) [47], D2(B,v=7) [46], D2(B,v=8) [45], D2(B,v=9) [44], D2(X,v=0) [75], D2(X,v=1) [74], D2(X,v=10) [65], D2(X,v=11) [64], D2(X,v=12) [63], D2(X,v=13) [62], D2(X,v=14) [61], D2(X,v=15) [60], D2(X,v=16) [59], D2(X,v=17) [58], D2(X,v=18) [57], D2(X,v=19) [56], D2(X,v=2) [73], D2(X,v=20) [55], D2(X,v=3) [72], D2(X,v=4) [71], D2(X,v=5) [70], D2(X,v=6) [69], D2(X,v=7) [68], D2(X,v=8) [67], D2(X,v=9) [66] », N2 {59} « N2(X,v=0) [60], N2(X,v=1) [59], N2(X,v=10) [50], N2(X,v=11) [49], N2(X,v=12) [48], N2(X,v=13) [47], N2(X,v=14) [46], N2(X,v=15) [45], N2(X,v=16) [44], N2(X,v=17) [43], N2(X,v=18) [42], N2(X,v=19) [41], N2(X,v=2) [58], N2(X,v=20) [40], N2(X,v=21) [39], N2(X,v=22) [38], N2(X,v=23) [37], N2(X,v=24) [36], N2(X,v=25) [35], N2(X,v=26) [34], N2(X,v=27) [33], N2(X,v=28) [32], N2(X,v=29) [31], N2(X,v=3) [57], N2(X,v=30) [30], N2(X,v=31) [29], N2(X,v=32) [28], N2(X,v=33) [27], N2(X,v=34) [26], N2(X,v=35) [25], N2(X,v=36) [24], N2(X,v=37) [23], N2(X,v=38) [22], N2(X,v=39) [21], N2(X,v=4) [56], N2(X,v=40) [20], N2(X,v=41) [19], N2(X,v=42) [18], N2(X,v=43) [17], N2(X,v=44) [16], N2(X,v=45) [15], N2(X,v=46) [14], N2(X,v=47) [13], N2(X,v=48) [12], N2(X,v=49) [11], N2(X,v=5) [55], N2(X,v=50) [10], N2(X,v=51) [9], N2(X,v=52) [8], N2(X,v=53) [7], N2(X,v=54) [6], N2(X,v=55) [5], N2(X,v=56) [4], N2(X,v=57) [3], N2(X,v=58) [2], N2(X,v=6) [54], N2(X,v=7) [53], N2(X,v=8) [52], N2(X,v=9) [51] », NO {54} « NO(v=0) [58], NO(v=1) [57], NO(v=10) [48], NO(v=11) [47], NO(v=12) [46], NO(v=13) [45], NO(v=14) [44], NO(v=15) [43], NO(v=16) [42], NO(v=17) [41], NO(v=18) [40], NO(v=19) [39], NO(v=2) [56], NO(v=20) [38], NO(v=21) [37], NO(v=22) [36], NO(v=23) [35], NO(v=24) [34], NO(v=25) [33], NO(v=26) [32], NO(v=27) [31], NO(v=28) [30], NO(v=29) [29], NO(v=3) [55], NO(v=30) [28], NO(v=31) [27], NO(v=32) [26], NO(v=33) [25], NO(v=34) [24], NO(v=35) [23], NO(v=36) [22], NO(v=37) [21], NO(v=38) [20], NO(v=39) [19], NO(v=4) [54], NO(v=40) [18], NO(v=41) [17], NO(v=42) [16], NO(v=43) [15], NO(v=44) [14], NO(v=45) [13], NO(v=46) [12], NO(v=47) [11], NO(v=48) [10], NO(v=49) [9], NO(v=5) [53], NO(v=50) [8], NO(v=51) [7], NO(v=52) [6], NO(v=53) [5], NO(v=6) [52], NO(v=7) [51], NO(v=8) [50], NO(v=9) [49] », O2 {42} « O2(v=0) [44], O2(v=1) [43], O2(v=10) [34], O2(v=11) [33], O2(v=12) [32], O2(v=13) [31], O2(v=14) [30], O2(v=15) [29], O2(v=16) [28], O2(v=17) [27], O2(v=18) [26], O2(v=19) [25], O2(v=2) [42], O2(v=20) [24], O2(v=21) [23], O2(v=22) [22], O2(v=23) [21], O2(v=24) [20], O2(v=25) [19], O2(v=26) [18], O2(v=27) [17], O2(v=28) [16], O2(v=29) [15], O2(v=3) [41], O2(v=30) [14], O2(v=31) [13], O2(v=32) [12], O2(v=33) [11], O2(v=34) [10], O2(v=35) [9], O2(v=36) [8], O2(v=37) [7], O2(v=38) [6], O2(v=39) [5], O2(v=4) [40], O2(v=40) [4], O2(v=41) [3], O2(v=5) [39], O2(v=6) [38], O2(v=7) [37], O2(v=8) [36], O2(v=9) [35] »
PERMLINK: www.lxcat.net/Morgan
DESCRIPTION: Assembled over the course of 30 years WL Morgan and suitable for use with 2-term Boltzmann solvers.
CONTACT: W. Lowell Morgan, Kinema Research & Software
Species: e + Ar [4], C [4], C2H2 [8], C2H4 [7], C2H6 [7], C3H8 [7], CF4 [7], CH [3], CH2 [3], CH3 [3], CH4 [11], Cl2 [7], CO [18], CO2 [13], F2 [11], H [4], H2 {3} « H2 [17], H2(p) [2], H2(s) [2] », H2O [10], HCl [8], He [4], Kr [4], N [2], N2 [25], N2(a) [4], Ne [4], NH3 [8], NO [10], O [5], O2 {3} « O2 [18], O2(a1D) [4], O2(B1S) [4] », O3 [4], SF6 [9], SiH4 [7], Xe [4], O- [2]
PERMLINK: www.lxcat.net/NGFSRDW
DESCRIPTION: A set of excitation cross section to individual fine-structure levels of the noble gases.
CONTACT: Al Stauffer, Dept. of Physics and Astronomy, York University, Toronto, Canada.
stauffer@@yorku.ca
Species: e + Ar {14} « Ar(3p5 4p J = 0 2p5) [4], Ar(3p5 4p J = 1 2p10) [9], Ar(3p5 4p J = 1 2p2) [1], Ar(3p5 4p J = 1 2p4) [3], Ar(3p5 4p J = 1 2p7) [6], Ar(3p5 4p J = 2 2p3) [2], Ar(3p5 4p J = 2 2p6) [5], Ar(3p5 4p J = 2 2p8) [7], Ar(3p5 4p J = 3 2p9) [6], Ar(3p5 4s J = 0 1s3) [19], Ar(3p5 4s j = 1 1s2) [10], Ar(3p5 4s J = 1 1s4) [12], Ar(3p5 4s J = 2 1s5) [24], Ar(3p6 J = 0) [40] », Kr {14} « Kr [40], Kr(1s2) [10], Kr(1s3) [18], Kr(1s4) [12], Kr(1s5) [23], Kr(2p10) [9], Kr(2p2) [1], Kr(2p3) [2], Kr(2p4) [3], Kr(2p5) [4], Kr(2p6) [5], Kr(2p7) [6], Kr(2p8) [7], Kr(2p9) [8] »
PERMLINK: www.lxcat.net/Phelps
DESCRIPTION: A compilation of atomic and molecular data, assembled and evaluated by A.V. Phelps and collaborators. Please refer to these data using the sources cited for each gas. We make no claims for these cross sections beyond those stated in the papers where they are published or cited. In most cases these cross sections were assembled in the 1970's and 1980's. In only a few cases have they been modified or tested since that time. I do not plan any updates. Additions have been made when cross sections have been assembled for other purposes. Since the JILA information center was closed by NIST, there is no one there to help you. Opinions expressed are those of AV Phelps and do not imply JILA, CU, or NIST approval.
CONTACT: A.V. Phelps, Fellow Adjoint of JILA
e-mail: avp@@jila.colorado.edu
HOW TO REFERENCE: http://jilawww.colorado.edu/~avp/
Species: Ar+ + Ar [2]; e + Ar [3], CO [18], CO2 [14], H2 [17], H2O [10], He [3], Mg [4], N2 [27], Na [7], Ne [8], NO [10], O2 [18], SF6 [9]; He+ + He [2]; Xe+ + Ne [1], Xe [2]
Species: Ar+ + Ar [4]; He+ + He [2]; N2+ + N2 [2]; Ne+ + Ne [2]; N+ + N2 [2]
PERMLINK: www.lxcat.net/Puech
DESCRIPTION: Cross section sets assembled by V Puech and colleagues in late 1980's and 1990's. Ne : updated and corrected on Dec 11 2012
CONTACT: Vincent Puech, LPGP, Orsay, France
Species: e + Ar [42], C2H4 [8], C3H6 [6], Ne [26], Xe [15]
PERMLINK: www.lxcat.net/QUANTEMOL
DESCRIPTION: Data calculated and published by Quantemol Ltd. and associated researchers using Quantemol-N software/expert system. Quantemol Ltd is based in University College London initiated by Professor Jonathan Tennyson FRS and Dr. Daniel Brown in 2004. The company initially developed a unique software tool that brings full accessibility to the highly sophisticated UK molecular R-matrix code, which is used to model electron polyatomic molecule interactions. What makes the software unique is that it requires no expertise in quantum scattering theory, and very accurate calculations can be performed on a simple desktop machine or laptop. Since then Quantemol has widened to further types of simulations with plasmas and industrial plasma tools.
HOW TO REFERENCE: http://quantemol.com
Species: e + BF3 [3], C2 [2], C2H2 [1], C2H2+ [1], C2OH6 [1], C3 [1], C3H4 [1], C3N [2], CaF [1], CaF+ [1], CF [2], CF2 [1], CF4 [1], CH [1], CH+ [1], CH4 [1], CNH [2], CO [3], CO2 [2], CO2+ [1], CONH3 [1], COS [2], CS [2], F2O [2], H2 [1], H2+ [1], H2O [5], H2S [2], H4C [2], HBr [3], HCHO [2], HCN [1], HCP [2], Kr [1], N2 [1], N2O [1], NH3 [2], NO2 [1], O2 [1], O3 [2], PH3 [2], SiF2 [2], SiH4 [2], SiO [4], SO2 [2]
PERMLINK: www.lxcat.net/SIGLO
DESCRIPTION: The SIGLO database is the "in-house" data used by the group GREPHE at LAPLACE in Toulouse. The data are taken from different sources as indicated for each gas. Please refer to original sources in publications. An early version of this data file, "siglo.sec", was distributed with BOLSIG. The main changes in the present version are :
The format has been changed to be compatible with BOLSIG+.
Scale factors have been incorporated in the data and no longer appear explicitly.
We have removed the CF4 cross section data because of their limited precision (probably due to digitization errors). For the moment our recommendation is to use the dataset in the Morgan database.
He : The present data are from the compilation of A.V. Phelps (see reference in the Phelps data base).
O2 : We recommend using the data in the Phelps database for this species.
H2 : We recommend using the data in the Phelps database for this species.
Cl2 : The present data are an updated compilation (Jan 2012) by J Gregorio and LC Pitchford.
Cu : Feb 2012. Digitized from Tkachev A N, Fedenev A A and Yakovlenko S I, Laser Phys. vol.17, p. 775 (2007)
Kr : Nov 2012. We re-digitized the data from figs. 1 and 5 in H. Date, Y. Sakai and H. Tagashira, J. Phys. D 22 1478 (1989). With respect to the previous data from this same reference in the SIGLO database, there are some changes in the threshold values and in the magnitudes of the inelastic cross sections.
CONTACT: LC Pitchford and JP Boeuf
pitchford@@laplace.univ-tlse.fr and jpb@@laplace.univ-tlse.fr
Species: e + Ar [3], Cl2 [16], CO2 [13], Cu [6], F2 [11], HCl [8], He [3], Hg [6], Kr [7], N2 [25], Ne [8], Ne(3P2) [1], SF6 [9], SiH4 [7], Xe [8], Xe(1s5) [1]
PERMLINK: www.lxcat.net/TRINITI
DESCRIPTION: These cross sections retrieved from the EEDF software package for calculations of electron energy distribution function developed by Prof. Napartovich A. P. and Drs. Dyatko N. A., Kochetov I. V., Sukharev A. G. from The State Science Center Troitsk Institute for Innovation and Fusion Research, Russia
CONTACT: Contact person is Dr. Igor Kochetov kochet@@triniti.ru
Species: e + Ar [8], Ar* [1], BCl [1], BCl2 [1], BCl3 [10], CF3I [12], CF4 [6], CH4 [5], CO [20], CO2 [20], CS [3], Cs* [1], F2 [8], H [3], H(2S) [1], H2 {11} « H2 [15], H2(+) [1], H2(v=1) [1], H2(v=2) [1], H2(v=3) [1], H2(v=4) [1], H2(v=5) [1], H2(v=6) [1], H2(v=7) [1], H2(v=8) [1], H2(v=9) [1] », H2O [8], HCl {4} « HCl [7], HCl(v=1) [2], HCl(v=2) [2], HCl(v=3) [1] », He [9], He* [1], N2 [24], Na {4} « Na [6], Na(3d) [1], Na(3p) [3], Na(4s) [1] », Ne {5} « Ne [8], Ne(1s2) [1], Ne(1s3) [1], Ne(1s4) [1], Ne(1s5) [1] », NF3 [3], O [12], O(0.02) [1], O2 {4} « O2 [11], O2(0.98) [8], O2(1.63) [7], O2(VSUM) [7] », SF6 [7], Xe [25], Xe* [1]
PERMLINK: www.lxcat.net/UBC
DESCRIPTION: The UBC database consists of Absolute Dipole (Optical) Oscillator Strengths as a function of Photon Energy for 65 neutral atoms and molecules for photoabsorption in the vacuum UV and soft X-ray regions of the electromagnetic spectrum. The data were obtained in both the discrete and continuum regions by fast electron scattering using electron energy loss spectroscopy (EELS) at zero degrees scattering angle. This method, known as Dipole (e,e) Spectroscopy, involves Bethe-Born conversion of the electron scattering intensities and Sum-Rule normalization to give absolute scales. The technique utilizes the virtual photon field created by a fast electron scattered in the forward direction (i.e. at negligible momentum transfer). Under these conditions the electron energy loss is equivalent to the photon energy and the method gives results entirely equivalent to those that could be obtained using continuum light sources such as monochromated synchrotron radiation. It is important to note that our data do not suffer from the linesaturation effects (linewidth-bandwidth interactions) which can cause large errors in optically determined oscillator strengths for discrete transitions with narrow natural linewidths. Our experimental methods, data processing and some corrections to earlier data are presented in the following publications: (1) W.F. Chan, G. Cooper and C.E. Brion, Absolute Oscillator Strengths for the Electronic Excitation of Atoms at High Resolution: Experimental Methods and Measurements for Helium. Phys. Rev. A 44,186-204 (1991). (2) W.F. Chan, G. Cooper, X. Guo, G.R. Burton and C.E. Brion, Absolute Oscillator Strengths for the Electronic Excitation of Atoms at High Resolution. Part III: The Photoabsorption of Argon, Krypton and Xenon. Phys. Rev. A 46, 149-171 (1992); 48, 858-860 (1993). (3) T.N. Olney, N.M. Cann, G. Cooper, and C.E. Brion. Absolute Scale Determination for Photoabsorption Spectra and the Calculation of Molecular Properties using Dipole Sum-Rules. Chem.Physics, 223, 59-98 (1997) and references therein. Both "low" ( typically 1.0 eV fwhm) and "high" ( typically 0.048 eV fwhm) resolution data are tabulated and can be plotted. These data are derived from a series of measurements made by Professor Chris Brion and his group at the University of British Columbia (UBC) between 1991 and 2002. References to their publications for specific neutral species should be included in all publications making use of these data. See the UBC database for specific references. Occasionally, the tabulated values of oscillator strength are negative below and close to threshold for inelastic scattering. This simply reflects the statistical accuracy of the data.
OSCILLATOR STRENGTHS
Species: e + (C2H5)2O [2], Ar [3], Br [3], C2H2 [2], C2H4 [2], C2H4O [2], C2H5OH [2], C2H6 [2], C2H6O [2], C2H7N [2], C3H6O [2], C3H8 [2], C3H9N [2], C4H10 [2], C5H12 [2], C5H5N [2], C6H14 [2], C6H6 [2], C7H16 [2], C8H18 [2], CCl4 [2], CF2Cl2 [2], CF3Cl [2], CF4 [2], CFCl3 [2], CH2O [2], CH3Br [3], CH3Cl [2], CH3F [2], CH3I [2], CH3OC3H7 [2], CH4 [2], CH4O [2], CH5N [2], Cl2 [2], CNBr [5], CNI [5], CO [2], CO2 [2], COS [2], D2 [1], H2 [2], H2O [2], H2S [2], HBr [3], HCl [2], He [3], HI [3], I2 [2], Kr [3], N2 [2], N2O [2], Ne [3], NH3 [2], NO [2], NO2 [2], O2 [2], PCl3 [4], PF3 [3], PF5 [3], PH3 [1], SiF4 [3], SiH4 [4], SO2 [2], Xe [3]
PERMLINK: www.lxcat.net/UNAM
DESCRIPTION: Electron swarm data derived from a pulsed Townsend experiment at UNAM, México.
CONTACT: J. de Urquijo
Species: CF3+ + CF4 [1]; CHF2+ + CHF3 [1]; C+ + Ar [1]; e + Ar [3], C2F4 [5], C2F4:Ar [19], C2F4:Xe [4], C2F6 [3], C2F6:Ar [18], C2F6:N2 [18], CF3I [3], CF3I:N2 [21], CF3I:SF6 [14], CHF3 [6], CHF3:Ar [18], CHF3:N2 [15], CO2 [5], N2 [3], SF6 [7], SF6:Ar [15], SF6:CF4 [18], SF6:CHF3 [12], SF6:CO2 [18], SF6:He [12], SF6:N2 [15], SF6:N2O [12], SF6:O2 [14], SF6:Xe [14]
PERMLINK: www.lxcat.net/UT
DESCRIPTION: A compilation of molecular data determined by Plasma Physics laboratory in University of Tartu
CONTACT: Indrek Jogi, indrek.jogi@ut.ee
Species: e + Air [3], Ar [4], Ar:N2 [28], Ar:O2 [32], C5F10O [4], C5F10O:Air [9], He [5], He:N2 [28], N2 [4], O2 [5]
PERMLINK: www.lxcat.net/Viehland
DESCRIPTION: The data here are from the Gaseous Ion Transport and Rate Coefficient Database, Software Release 4.1 (March, 2006), as extended and updated on a regular basis.
CONTACT: Larry A. Viehland, Viehland@Chatham.edu
HOW TO REFERENCE: L. A. Viehland and C. C. Kirkpatrick, Int. J. Mass Spectrom. Ion Proc. 149/150 (1995) 555.
Species: Ag+(1S0) + Ar [90], He [90], Kr [30], Ne [90], Rn [30], Xe [30]; Ag+(3S1) + Ar [60], He [60], Ne [60]; Ag-(1S0) + Ar [60], He [60], Ne [60]; Al+(1S0) + Ar [30], He [30], Kr [30], Ne [30], Rn [30], Xe [30]; Al3+(1S0) + He [30], Ne [30]; Ar+(2P) + He [30], Ne [30]; Ar+(2P1/2) + He [30], Ne [30]; Ar+(2P3/2) + He [30], Ne [30]; Au+(1S0) + Ar [90], He [90], Kr [30], Ne [90], Xe [30]; Au+(3S0) + Ar [60], He [60], Ne [60]; Au-(1S0) + Ar [60], He [60], Ne [60]; Ba+(2S1/2) + Ar [60], He [60], Kr [60], Ne [60], Rn [30], Xe [60]; Ba2+(1S0) + Ar [60], He [60], Kr [60], Ne [60], Rn [30], Xe [60]; Be+(2S1/2) + Ar [90], He [60], Kr [90], Ne [60], Rn [60], Xe [90]; Be2+(1S0) + Ar [30], He [30], Ne [30]; Br+(3P0) + Ar [30], He [30], Ne [30]; Br+(3P1) + Ar [30], He [30], Ne [30]; Br+(3P2) + Ar [30], He [30], Ne [30]; Br-(1S0) + Ar [30], He [30], Kr [30], Ne [30], Rn [30], Xe [30]; B+(1S0) + Ar [30], He [30], Kr [30], Ne [30], Rn [30], Xe [30]; Ca+(2S1/2) + Ar [30], He [30], Kr [30], Ne [30], Rn [30], Xe [30]; Ca2+(1S0) + Ar [30], He [30], Kr [30], Ne [30], Rn [30], Xe [30]; Cd+(2S1/2) + Ar [30], He [30], Kr [30], Ne [30], Rn [30], Xe [30]; Cl-(1S0) + Ar [60], He [60], Kr [60], Ne [60], Rn [60], Xe [60]; Co+(3F4) + He [30], Ne [30]; Co+(5F5) + He [30], Ne [30]; Cr+(6D9/2) + He [30], Ne [30]; Cr+(6S5/2) + He [30], Ne [30]; Cs+(1S0) + Ar [30], He [30], Kr [30], Ne [30], Rn [30], Xe [30]; Cu+(1S0) + Ar [90], He [90], Kr [30], Ne [90], Rn [30], Xe [30]; Cu+(3S1) + Ar [60], He [60], Ne [60]; Cu-(1S0) + Ar [60], He [60], Ne [60]; C+(2P) + Ar [30], He [30], Kr [30], Ne [30], Rn [30], Xe [30]; C+(2P1/2) + Ar [30], Kr [30], Ne [30], Rn [30], Xe [30]; C+(2P3/2) + Ar [30], He [30], Kr [30], Ne [30], Rn [30], Xe [30]; C+(2Pi1/2) + He [30]; C+(4P) + He [30]; C+(4P1/2) + He [30]; C+(4P3/2) + He [30]; C+(4P5/2) + He [30]; Eu+(9S4) + Ar [90], He [60], Kr [60], Ne [60], Xe [60]; Eu2+(8S7/2) + Ar [30], He [30], Kr [30], Ne [30], Xe [30]; Eu3+(7F0) + Ar [30], He [30], Ne [30]; Fr+(1S0) + Ar [30], He [30], Kr [30], Ne [30], Rn [30], Xe [30]; F-(1S0) + Ar [30], He [30], Kr [30], Ne [30], Rn [30], Xe [30]; Ga+(1S0) + Ar [30], He [30], Kr [30], Ne [30], Rn [30], Xe [30]; Gd+(10D5/2,ASO) + Ar [30], He [30]; Gd+(10D5/2,ASR) + Ar [30], He [30]; Gd+(10D5/2,ISO) + Ar [30], He [30]; Gd+(10D5/2,ISR) + Ar [30], He [30]; Gd+(10D7/2,ASO) + Ar [30], He [30]; Gd+(10D7/2,ISO) + Ar [30], He [30]; Ge+(2P) + Ar [30], He [30], Kr [30], Ne [30], Rn [30], Xe [30]; Ge+(2P1/2) + Ar [30], He [30], Kr [30], Ne [30], Rn [30], Xe [30]; Ge+(2P3/2) + Ar [30], He [30], Kr [30], Ne [30], Rn [30], Xe [30]; He+(2S1/2) + Ar [30], He [180], Ne [90]; Hg+(2S1/2) + Ar [30], He [60], Kr [30], Ne [30], Rn [30], Xe [30]; H+ + Ar [30], He [90], Ne [30]; In+(1S0) + Ar [30], He [30], Kr [30], Ne [30], Rn [30], Xe [30]; I+(3P2) + Ar [30], He [30], Ne [30]; I-(1S0) + Ar [30], He [30], Ne [30]; Kr+(2P) + He [30], Ne [30]; Kr+(2P1/2) + He [30], Ne [30]; Kr+(2P3/2) + He [30], Ne [30]; K+(1S0) + Ar [30], He [30], Kr [60], Ne [30], Rn [30], Xe [60]; Li+(1S0) + Ar [60], He [30], Kr [90], Ne [30], Rn [30], Xe [60]; Lu+(1S0) + Ar [30], He [30], Kr [30], Ne [30], Xe [30]; Mg+(2S1/2) + Ar [30], He [150], Kr [30], Ne [30], Rn [30], Xe [30]; Mg2+(1S0) + Ar [30], He [60], Kr [30], Ne [30], Rn [30], Xe [30]; N+(3P0) + He [30]; Na+(1S0) + Ar [30], He [30], Kr [60], Ne [30], Rn [30], Xe [60]; Ne+(2Pi_1/2) + He [30]; Ne+(2Pi_3/2) + He [30]; Ne+(2Sigma_1/2+) + He [30]; Ni+(2D5/2,2D3/2) + He [30], Ne [30]; Ni+(4F9/2) + He [30], Ne [30]; N+(3P0) + He [30]; O+(4S3/2) + Ar [30], He [30], Ne [30]; O-(2P) + Ar [30], He [30], Kr [30], Ne [30]; O-(2P1/2) + Ar [30], He [30], Kr [30], Ne [30]; O-(2P3/2) + Ar [30], He [30], Kr [30], Ne [30]; Ra+(2S1/2) + Ar [30], He [30], Kr [30], Ne [30], Rn [30], Xe [30]; Ra2+(1S0) + Ar [30], He [30], Kr [30], Ne [30], Rn [30], Xe [30]; Rb+(1S0) + Ar [30], He [30], Kr [30], Ne [30], Rn [30], Xe [30]; Rn+(2P) + Ar [30], He [30], Ne [30], Xe [30]; Rn+(2P1/2) + Ar [30], He [30], Ne [30], Xe [30]; Rn+(2P3/2) + Ar [30], He [30], Ne [30], Xe [30]; Si+(2P) + Ar [30], He [30], Kr [30], Ne [30], Rn [30], Xe [30]; Si+(2P1/2) + Ar [30], He [30], Kr [30], Ne [30], Rn [30], Xe [30]; Si+(2P3/2) + Ar [30], He [30], Kr [30], Ne [30], Rn [30], Xe [30]; Sr+(2S1/2) + Ar [30], He [30], Kr [30], Ne [30], Rn [30], Xe [30]; Sr2+(1S0) + He [30], Kr [30], Ne [30], Rn [30], Xe [30]; S-(2P) + He [30]; S-(2P1/2) + He [30]; S-(2P3/2) + He [30]; Tl+(1S0) + Ar [30], He [30], Kr [30], Ne [30], Xe [30]; U+(4I9/2) + Ar [30], He [30], Kr [30], Ne [30], Xe [30]; Xe+(2P) + Ar [30], He [30], Kr [30], Ne [30]; Xe+(2P1/2) + Ar [30], He [30], Kr [30], Ne [30]; Xe+(2P3/2) + Ar [30], He [30], Kr [30], Ne [30]; Yb+(2S1/2) + Ar [60], He [30], Kr [30], Ne [30], Xe [30]; Zn+(2S1/2) + Ar [30], He [30], Kr [30], Ne [30], Rn [30], Xe [30]
INTERACTION POTENTIALS
Species: Ag+(1S0) + Ar [3], He [3], Kr [1], Ne [3], Rn [1], Xe [1]; Ag+(3S1) + Ar [2], He [2], Ne [2]; Ag-(1S0) + Ar [2], He [2], Ne [2]; Al+(1S0) + Ar [1], He [1], Kr [1], Ne [1], Rn [1], Xe [1]; Al3+(1S0) + He [1], Ne [1]; Ar+(2P) + He [3]; Ar+(2Pi1/2) + He [4], Ne [1]; Ar+(2Pi3/2) + He [4], Ne [1]; Ar+(2Sigma) + He [4], Ne [1]; Au+(1S) + Ar [2], He [2], Ne [2]; Au+(1S0) + Ar [1], He [1], Kr [2], Ne [1], Rn [1], Xe [1]; Au+(3S0) + Ar [2], He [2], Ne [2]; Au-(1S0) + Ar [2], He [2], Ne [2]; Ba+(2S1/2) + Ar [2], He [2], Kr [2], Ne [2], Rn [1], Xe [2]; Ba2+(1S0) + Ar [2], He [2], Kr [2], Ne [2], Rn [1], Xe [2]; Be+(2S1/2) + Ar [3], He [2], Kr [3], Ne [2], Rn [2], Xe [3]; Be2+(1S0) + Ar [1], He [1], Ne [1]; Br+ + Ar [14], He [11], Ne [10]; Br-(1S0) + Ar [5], He [4], Kr [3], Ne [3], Rn [1], Xe [3]; B+(1S0) + Ar [1], He [1], Kr [1], Ne [1], Rn [1], Xe [1]; C(2Pi1/2)+ + Ar [1], He [1], Ne [1]; C(2Pi3/2)+ + Ar [1], He [1], Ne [1]; C(2Sigma1/2)+ + Ar [1], He [1], Ne [1]; Ca+(2S1/2) + Ar [1], He [1], Kr [1], Ne [1], Rn [1], Xe [1]; Ca2+(1S0) + Ar [1], He [1], Kr [1], Ne [1], Rn [1], Xe [1]; Cd+(2S1/2) + Ar [1], He [1], Kr [1], Ne [1], Rn [1], Xe [1]; Cl-(1S0) + Ar [10], He [4], Kr [7], Ne [6], Rn [1], Xe [4]; CO+ + He [5]; Co+(3F4) + He [1], Ne [1]; Co+(5F5) + He [1], Ne [1]; Cr+(6D9/2) + He [1], Ne [1]; Cr+(6S5/2) + He [1], Ne [1]; Cs+(1S0) + Ar [2], He [2], Kr [3], Ne [2], Rn [1], Xe [3]; Cu+(1S0) + Ar [2], He [2], Kr [1], Ne [2], Rn [1], Xe [1]; Cu+(3S1) + Ar [2], He [2], Ne [2]; Cu-(1S0) + Ar [2], He [2], Ne [2]; C+(2P) + Ne [1]; C+(2Pi1/2) + Kr [1], Rn [1], Xe [1]; C+(2Pi3/2) + Kr [1], Rn [1], Xe [1]; C+(2Sigma1/2) + Kr [1], Rn [1], Xe [1]; C+(4Pi-1/2) + He [1]; C+(4Pi1/2) + He [1]; C+(4Pi3/2) + He [1]; C+(4Pi5/2) + He [1]; C+(4Sigma1/2) + He [1]; C+(4Sigma3/2) + He [1]; Eu+(9S4) + Ar [3], He [2], Kr [2], Ne [2], Xe [2]; Eu2+(8S7/2) + Ar [1], He [1], Kr [1], Ne [1], Xe [1]; Eu3+(7F0) + Ar [1], He [1], Ne [1]; Fr+(1S0) + Ar [1], He [1], Kr [1], Ne [1], Rn [1], Xe [1]; F-(1S0) + Ar [8], He [7], Kr [4], Ne [6], Rn [1], Xe [4]; Ga+(1S0) + Ar [1], He [1], Kr [1], Ne [1], Rn [1], Xe [1]; Gd+(10D5/2,ASR) + Ar [1], He [1]; Gd+(10D5/2,ISO) + Ar [1], He [1]; Gd+(10D5/2,ISR) + Ar [1], He [1]; Gd+(10D5/2,OMEGA=1/2) + Ar [1], He [1]; Gd+(10D5/2,OMEGA=3/2) + Ar [1], He [1]; Gd+(10D5/2,OMEGA=5/2) + Ar [1], He [1]; Gd+(10D7/2,OMEGA=1/2) + Ar [1], He [1]; Gd+(10D7/2,OMEGA=3/2) + Ar [1], He [1]; Gd+(10D7/2,OMEGA=5/2) + Ar [1], He [1]; Gd+(10D7/2,OMEGA=7/2) + Ar [1], He [1]; Ge+(2Pi1/2) + Ar [1], He [1], Kr [1], Ne [1], Rn [1], Xe [1]; Ge+(2Pi3/2) + Ar [1], He [1], Kr [1], Ne [1], Rn [1], Xe [1]; Ge+(2Sigma1/2) + Ar [1], He [1], Kr [1], Ne [1], Rn [1], Xe [1]; He+(2S1/2) + Ar [1], He [7], Ne [4]; Hg+(2S1/2) + Ar [1], He [1], Kr [1], Ne [1], Rn [1], Xe [1]; H+ + Ar [1], He [3], Ne [1]; In+(1S0) + Ar [1], He [1], Kr [1], Ne [1], Rn [1], Xe [1]; I+(3P2) + Ar [1], He [1], Ne [1]; I-(1S0) + Ar [6], He [3], Kr [2], Ne [6], Xe [1]; Kr+(2P) + Ar [3], He [7], Ne [3]; K+(1S0) + Ar [3], He [6], Kr [3], Ne [4], Rn [1], Xe [3]; Li+(1S0) + Ar [4], He [7], Kr [6], Ne [7], Rn [1], Xe [3]; Lu+(1S0) + Ar [1], He [1], Kr [1], Ne [1], Xe [1]; Mg+(2S1/2) + Ar [2], He [7], Kr [3], Ne [2], Rn [2], Xe [2]; Mg2+(1S0) + Ar [1], He [2], Kr [1], Ne [1], Rn [1], Xe [1]; Na+(1S0) + Ar [1], H2 [1], He [2], Kr [2], Ne [2], Rn [1], Xe [3]; Ne+(2Pi_1/2) + He [2]; Ne+(2Pi_3/2) + He [2]; Ne+(2Sigma_1/2+) + He [2]; Ni+(2D5/2,2D3/2) + He [1]; Ni+(4F9/2) + He [1]; N+(3P0) + He [1]; O+(4S3/2) + Ar [1], He [9], Ne [3]; O-(2P) + Ar [8], He [6], Kr [3], Ne [5]; Ra+(2S1/2) + Ar [1], He [1], Kr [1], Ne [1], Rn [1], Xe [1]; Rb+(1S0) + Ar [2], He [2], Kr [2], Ne [2], Rn [1], Xe [2]; Rn+(2P) + Ar [3], He [3], Kr [3], Ne [3], Xe [3]; Si+(2Pi1/2) + Ar [1], He [1], Kr [1], Ne [1], Rn [1], Xe [1]; Si+(2Pi3/2) + Ar [1], He [1], Kr [1], Ne [1], Rn [1], Xe [1]; Si+(2Sigma1/2) + Ar [1], He [1], Kr [1], Ne [1], Rn [1], Xe [1]; Sr+(2S1/2) + Ar [1], He [1], Kr [1], Ne [1], Rn [1], Xe [1]; Sr2+(1S0) + Ar [1], He [1], Kr [1], Ne [1], Rn [1], Xe [1]; S+ + He [2]; S-(2P) + He [2]; S-(2Pi1/2) + He [2]; S-(2Pi3/2) + He [1]; Tl+(1S0) + Ar [2], He [2], Kr [2], Ne [2], Xe [2]; U+(4I9/2) + Ar [1], He [2], Kr [1], Ne [1], Xe [1]; Xe+(2P) + Ar [3], He [3], Kr [3], Ne [3]; Yb+(2S1/2) + Ar [3], He [2], Kr [2], Ne [1], Xe [1]; Zn+(2S1/2) + Ar [1], He [1], Kr [1], Ne [1], Xe [1]; Zn2+(1S0) + Ne [1]
Species: (CH2)2O+ + He [1]; (SF6)2- + SF6 [1]; (SF6)3- + SF6 [1]; 11B+(1S0) + He [1]; 127I+ + He [1]; 127I- + Ar [1], He [1]; 12C(2P)+ + Ar [170], He [175], Kr [122], Rn [122], Xe [122]; 12C(2P1/2)+ + Ar [170], He [170], Kr [122], Ne [122], Rn [122], Xe [122]; 12C(2P3/2)+ + Ar [170], He [170], Kr [122], Ne [122], Rn [122], Xe [122]; 12C(4P)+ + He [4]; 12C+ + Ar [1], CO [2], He [3]; 132Xe(A)2+ + Xe [1]; 132Xe(B)2+ + Xe [1]; 132Xe(P1)+ + Xe [2]; 132Xe(P3)+ + Xe [2]; 132Xe+ + Ar [1], He [2], Ne [1], Xe [2]; 132Xe2+ + He [2]; 133Cs+ + Ar [3], CO [2], CO2 [2], H2 [2], He [2], Kr [3], N2 [2], Ne [3], O2 [2], Xe [3]; 138Ba+(2S1/2) + Ar [3], He [2]; 13C(2P)+ + Ar [122], Kr [122], Ne [122], Rn [122], Xe [122]; 13C(2P1/2)+ + Ar [122], He [170], Kr [122], Ne [122], Xe [122]; 13C(2P3/2)+ + Ar [122], He [170], Kr [122], Ne [122], Rn [122], Xe [122]; 13C(4P)+ + He [170]; 13C(4P1/2)+ + He [170]; 13C(4P3/2)+ + He [170]; 13C(4P5/2)+ + He [170]; 14N16O+(v=0) + Ar [124], He [172], Kr [124], Ne [124], Xe [124]; 14N+(3P0) + Ar [1], He [3], N2 [4]; 16O(2D)+ + Ne [1]; 16O(4S)+ + He [1], Ne [1]; 16O*+ + Ar [1], He [1]; 16O+(4S3/2) + Ar [2], He [7], Ne [3]; 16O-(2P1/2) + Air [1], CO2 [2], He [4], O2 [4]; 16O2+ + He [1], Ne [1]; 19F+ + He [1]; 19F- + Ar [1], He [6], Kr [2], SF6 [2], Xe [2]; 1H+ + H2 [4], He [2], Ne [1]; 1H- + H2 [4], He [1]; 202Hg(1S)2+ + He [1]; 202Hg(3D)2+ + He [1]; 202Hg+ + He [1], Ne [1]; 205Tl+ + Ar [4], He [4], Kr [4], Ne [4], O2 [1], Xe [4]; 20Ne+(2P1/2) + Ne [2]; 20Ne+(2P3/2) + Ne [2]; 20Ne+(mix) + Ar [1], He [13], Ne [7]; 21Ne+(2P1/2) + Ne [1]; 21Ne+(2P3/2) + Ne [1]; 21Ne+(mix) + He [1]; 22Ne+(mix) + He [2]; 238U+ + He [4]; 23Na+(1S0) + Ar [8], CH4 [2], CO2 [4], D2 [3], H2 [2], He [6], Kr [5], Ne [9], O2 [1], SF6 [1], Xe [4]; 28Si+ + He [1]; 28Si+(2P) + Kr [122], Rn [122], Xe [122]; 28Si+(2P1/2) + Kr [122], Rn [122], Xe [122]; 28Si+(2P3/2) + Kr [122], Rn [122], Xe [122]; 29Si+(2P) + Kr [122], Rn [122], Xe [122]; 29Si+(2P1/2) + Kr [122], Rn [122], Xe [122]; 29Si+(2P3/2) + Kr [122], Rn [122], Xe [122]; 2H+ + D2 [4], He [2], Ne [1]; 2H- + D2 [3]; 30Si+(2P) + Kr [122], Rn [122], Xe [122]; 30Si+(2P1/2) + Kr [122], Rn [122], Xe [122]; 30Si+(2P3/2) + Kr [122], Rn [122], Xe [122]; 32S+ + He [2]; 32S-(2P) + He [1]; 35Cl-(1S0) + Air [1], Ar [3], He [4], Kr [4], N2 [2], Ne [3], Xe [3]; 35Cl+ + He [1]; 39K+ + Ar [5], CH4 [1], CO [4], CO2 [2], D2 [1], H2 [3], He [9], Kr [3], N2 [3], Ne [2], NO [2], O2 [4], Xe [2]; 40Ar(D1)2+ + Ar [1]; 40Ar(P3)2+ + Ar [1]; 40Ar+ + Ar [6], He [9], Ne [1]; 40Ar+(2P) + Ar [1], He [1]; 40Ar2+ + Ar [3], He [1]; 4He+ + He [12], Ne [2]; 4He2+ + He [1]; 70Ge+(2P) + Ar [122], He [146], Kr [122], Ne [122], Rn [122], Xe [122]; 70Ge+(2P1/2) + Ar [122], He [146], Kr [122], Ne [122], Rn [122], Xe [122]; 70Ge+(2P3/2) + Ar [122], He [146], Kr [122], Ne [122], Rn [122], Xe [122]; 72Ge+(2P) + Ar [122], He [146], Kr [122], Ne [122], Rn [122], Xe [122]; 72Ge+(2P1/2) + Ar [122], He [146], Kr [122], Ne [122], Rn [122], Xe [122]; 72Ge+(2P3/2) + Ar [122], He [146], Kr [122], Ne [122], Rn [122], Xe [122]; 73Ge+(2P) + Ar [122], He [146], Kr [122], Ne [122], Rn [122], Xe [122]; 73Ge+(2P1/2) + Ar [122], He [146], Kr [122], Ne [122], Rn [122], Xe [122]; 73Ge+(2P3/2) + Ar [122], He [146], Kr [122], Ne [122], Rn [122], Xe [122]; 74Ge+(2P) + Ar [122], He [146], Kr [122], Ne [122], Rn [122], Xe [122]; 74Ge+(2P1/2) + Ar [122], He [146], Kr [122], Ne [122], Rn [122], Xe [122]; 74Ge+(2P3/2) + Ar [122], He [146], Kr [122], Ne [122], Rn [122], Xe [122]; 76Ge+(2P) + Ar [122], He [146], Kr [122], Ne [122], Rn [122], Xe [122]; 76Ge+(2P1/2) + Ar [122], He [146], Kr [122], Ne [122], Rn [122], Xe [122]; 76Ge+(2P3/2) + Ar [122], He [146], Kr [122], Ne [122], Rn [122], Xe [122]; 79Br+ + Ar [1]; 79Br- + Ar [6], He [2], Kr [4], Ne [3], Xe [4]; 7Li+(1S0) + Ar [11], C2H6(CH3)COH [1], CH4 [2], CO [2], CO2 [2], D2 [1], H2 [4], HBr [1], HCl [1], He [19], HI [1], Kr [3], N2 [5], Ne [10], O2 [3], Xe [3]; 84Kr(2P1/2)+ + Kr [1]; 84Kr(2P3/2)+ + Kr [1]; 84Kr(2P3/2)2+ + Kr [1]; 84Kr(A)2+ + Kr [1]; 84Kr(B)2+ + Kr [1]; 84Kr+(2P) + Ar [2], He [5], N2 [1]; 84Kr2+ + He [2], Kr [1]; 85Rb+ + Ar [4], CO2 [5], H2 [4], He [5], Kr [5], N2 [5], Ne [5], O2 [4], Xe [6]; Ar2+ + Ar [2]; ArH+ + He [1]; C10H8+ + He [1]; C2H2- + He [1]; C2H3N+ + He [1]; C2H5+ + CH4 [2]; C2N2+ + He [1]; C2N+ + He [1]; C2O2+ + CO [3]; C2O4+ + CO2 [1]; C3H5+ + CH4 [2]; C3H7+ + D2 [1]; C6H6+ + He [1]; C6H7+ + He [1]; CF3+ + CF4 [1]; CH2CHOH+ + He [1]; CH2+ + He [4]; CH3CHOH+ + He [1]; CH3O2+ + He [1]; CH3OCH2+ + He [1]; CH3+ + Ar [2], He [4]; CH4+ + He [2]; CH5+ + CH4 [2], He [1]; CHF2+ + CHF3 [1]; CH+ + He [4]; CN+ + He [1]; CO*+ + He [1]; CO2+ + Ar [1], CO2 [1], He [3], N2 [2], Ne [1]; CO3- + Ar [1], CO2 [2], He [1], O2 [2]; CO4- + O2 [2]; COH+ + Ar [1], He [1]; CO+ + Ar [1], CO [5], He [5], Ne [1]; C+(2P) + He [1]; D3+ + D2 [4]; H2CN+ + He [1]; H2O+ + Ar [1], He [1], Ne [1]; H2+ + He [1]; H3O+ + Ar [1], CH4 [1], He [1], N2 [1]; H3+ + H2 [5], He [1]; H5O2+ + He [1], N2 [1]; H7O3+ + He [1], N2 [1]; HCN+ + He [2]; He2+ + He [2]; HeH+ + He [1]; He+(2S1/2) + He [1]; Kr2+ + Kr [2]; LiCH4+ + D2 [1]; LiCO2+ + CO2 [1]; LiCO+ + CO [1]; LiN2+ + N2 [1]; N2Ar+ + He [1]; N2H+ + Ar [1], He [1], N2 [2]; N2O2+ + NO [1]; N2OH+ + Ar [1], He [1]; N2O+ + Ar [2], He [2], N2 [1], Ne [1]; N2+ + Ar [1], He [3], Kr [1], N2 [9], Ne [1]; N3+ + N2 [2]; N4+ + He [1], N2 [3]; Ne2+ + Ne [3]; Ne+(2Sigma_1/2+) + Ar [1], He [1], Ne [1]; Ne2+(D1) + Ne [1]; NH2+ + He [1]; NH3+ + He [1]; NH4+ + He [1]; NO2+ + Air [1], Ar [1], He [1], N2 [1]; NO2- + Air [1], He [1], N2 [1]; NO3- + N2 [1]; NOH2O+ + He [1]; NO+ + Air [1], CO2 [1], He [3], NO [2]; O2*+ + Ne [1]; O2H2+ + He [1]; O2H+ + He [1]; O2+ + Air [1], Ar [1], CO2 [1], He [1], Kr [1], Ne [1], O2 [10]; O2- + Air [1], He [3], O2 [4]; O22+ + Ar [1]; O3- + Air [1], Ar [1], He [1], O2 [2]; O4+ + O2 [2]; O4- + O2 [1]; OD- + He [3]; OH- + He [4]; S2F7+ + SF6 [1]; S2- + He [1]; SF3+ + SF6 [2]; SF4+ + SF6 [1]; SF5+ + SF6 [2]; SF5- + He [1], SF6 [2]; SF6- + He [1], SF6 [2]; SH- + He [1]; SO2F- + He [1]; SO2+ + Ar [1], He [1]; SO3- + He [1]
PERMLINK: www.lxcat.net/XJTUAETLab
DESCRIPTION: This database is an open-access database for sharing Fundamental Physicochemical Properties of Gas Discharges and Plasma. Since 2007, these data were obtained gradually via experiments or theoretical calculations conducted by more than ten PhD students from our Lab. This database includes electron and ion scattering cross sections, swarm parameters (ionization coefficients, attachment coefficients, electron mobility, diffusion coefficient, etc.), dielectric breakdown strength, chemical reaction rates, equation of state (EOS), and other data required for modeling gas discharges and plasma. We hope our database can help to promote the innovative development of relevant fundamental research.
CONTACT: Boya Zhang (zhangby@xjtu.edu.cn) Huantong Shi (htshi@mail.xjtu.edu.cn) Jian Wu (jxjawj@mail.xjtu.edu.cn) Xingwen Li(xwli@mail.xjtu.edu.cn)
Species: e + C4F7N [3], C4F7N:CO2 [27], C4F7N:N2 [27], C5F10O [3], C5F10O:Air [24], C5F10O:CO2 [24]
DESCRIPTION: On-line BOLSIG+ solver
HOW TO REFERENCE: G.J.M. Hagelaar and L.C. Pitchford, "Solving the Boltzmann equation to obtain electron transport coefficients and rate coefficients for fluid models", Plasma Sci Sources and Tech 14, 722 (2005)
Copyright © 2009-2023, the LXCat team. The use without proper referencing to databases and software used is prohibited. All Rights Reserved. You currently use FR | NL | US mirror site.


What is the "Red Hat Enterprise Linux for SAP Solutions" subscription?
Does RHEL for SAP Solutions subscription provides access to the new Update Services for SAP Solutions?
Update Services for SAP Solutions, that provides support on specified minor releases for 4 years from General Availability. See the RHEL Life Cycle page for details.
Update Services for SAP Solutions is only provided with RHEL for SAP Solutions and for customers running either SAP HANA or SAP Applications. It is not available on any other RHEL products, or for customers not running SAP workloads.
Update Services for SAP Solutions is only provided on specified minor RHEL releases, which may be different than the EUS releases.
RHEL for SAP Solutions subscription may be used with Red Hat Enterprise Linux 6 , but does not include Insights and Update Services for SAP Solutions. However, EUS is available on specific RHEL 6 releases, and can be used under the RHEL for SAP Solutions subscription to allow for easier migration.
sapconf: provides an automated RHEL provisioning solution for SAP including kernel parameters, additional rpms, network settings etc. Can be integrated into kickstart and Satellite Server.
compat-sap-c++ : Provides additional runtime compatibility libraries required by the newer NetWeaver releases . These libraries are installed independently of the standard runtime libraries provided by RHEL.
tuned-profiles-sap: provides the "sap-netweaver" profile (based on the "enterprise-storage" profile) to tune RHEL for running SAP NetWeaver based applications.
resource-agents-sap: provides Pacemaker cluster resource agents (SAPDatabase and SAPInstance) to set up high available SAP NetWeaver environments.
compat-locales-sap: enables Legacy SAP locales to easily migrate non-unicode SAP NetWeaver installations from UNIX/Windows to Linux (see SAP Note 187864). Also provides additional locales for customers still running non-Unicode SAP applications. For example a "de_DE@HPUX" locale is provided that changes the sorting for German on RHEL to match the sorting on HP-UX to avoid sorting issues as described in SAP Note 952625.
vhostmd/vm-dump-metrics monitoring daemon and client required by SAP for KVM support (see SAP Note 1400911).
Future solutions. All future solutions for SAP applications will be added to the RHEL for SAP Applications channel.
Scalable File System Add-On (XFS) at no additional charge.
compat-sap-c++: Provides additional runtime compatibility libraries required by the newer NetWeaver releases . These libraries are installed independently of the standard runtime libraries provided by RHEL.
resource-agents-sap-hana: resource agents for managing SAP HANA instance in a pacemaker cluster environment.
Future solutions. All future solutions for SAP HANA will be added to the RHEL for SAP HANA channel.
SAP Solutions Subscription includes Red Hat Enterprise Linux High Availability Add-on. Red Hat Enterprise Linux High Availability provides all necessary packages for configuring pacemaker based cluster that provides reliability, scalability, and availability to critical production services.
SAP Solutions Subscription includes Smart Management Add-on. Smart Management Add-on is required for each Red Hat Enterprise Linux system that you want to manage with Red Hat Satellite. It allows one to easily manage an organization and update Red Hat Enterprise Linux systems using Red Hat Satellite.
How to subscribe SAP Applications system to the new Update Services for SAP Solutions ?
How to subscribe the SAP HANA system to the new Update Services for SAP Solutions ?
I was told that "Red Hat Enterprise Linux for SAP Solutions" was not available on 7.5, but this article says 7.2+ and above is supported. Is 7.5 currently supported for "Red Hat Enterprise Linux for SAP Solutions"?
RHEL 7.5 has been certified for SAP HANA.
I'm assuming that by 'extended support' you mean the 'extended update support'. In any case please note the difference between extended update support (EUS) and Update services for SAP Solutions (E4S). While EUS is available as of now for RHEL 7.5 (ends April 30, 2020), the E4S is not available for RHEL 7.5 minor version. We are working on explaining the reasons why the RHEL 7.5 is not part of E4S and once we have a proper statement for that we will update it here and other places.
This KB refers to RHEL for SAP HANA, which has been deprecated. Is the table still accurate for RHEL for SAP Solutions, which is the replacement for both the old SAP Applications and HANA versions? RHEL for SAP Applications is still available for subscription to support non-HANA SAP deployments (SAP ERP on ORACLE, for instance) but it is not our go-forward advice.


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text:
Guest View: Jim Tripp ~ The Rest of the Iceberg. Part 2: Do State Land Department Site Specific Plans Help or Hurt K-12 Education Funding?
Bankruptcy is achieved by habitually incurring expenses in excess of revenues. Despite having been granted 9.3 million acres of Federal land to sell and lease in order to fund K-12 education, the Arizona State Land Department (ASLD) still cannot generate enough revenue to cover costs. How severe is the gap?
• Local school districts were recently forced to sue the state for adequate funding
• From 1966 to 2006, AZ dropped from 130% of the national average to 80% in K-12 education expenditures (Chart 12, p. 33)
• AZ currently now ranks 48th in K-12 education funding and many quality metrics (pp. 5, 6, 43, 44, 50, 53 in the above link)
How did ASLD manage to fail so miserably in its purpose? By getting the green light from the courts to seek maximum selling price for K-12 Trust Lands, regardless of K-12 funding liabilities incurred during rezoning for highest price. This legal policy has enriched real estate developers, but impoverished school districts.
Case in Point: the Annexation at Tangerine and Thornydale
The Site Specific Plan for the Tangerine and Thornydale annexation (page 75) says that 1,767 K-12 students will be added to the Marana School District if Oro Valley should annex and develop the land using the recommended zoning. I wondered why the Marana Unified School District (MUSC) would accept such a burden and, after multiple discussions with different officials, I got the answer: MUSC will get its ~$8500/student/year from the State, or ~$15 million/year, regardless of the selling price of this tract of land.
Where will this ~$15 million/year come from? Well, if the ~3100 houses in the plan pay a similar school tax to me in Sky Ranch, each household will contribute ~$1400/yr in school taxes, for a total of ~$4.3 million. That means, for this annexation to make financial sense for K-12 education, the revenue stream from the sale of the land needs to be ~$10.7 million/year.
What selling price is required to generate annual interest revenue of $10.7 million/year? First, we need to know a safe interest rate, so let's try 2-4%. At 4% interest, the sale price would need to be $267 million, or ~$302,000/acre, given that the annex is 885 acres in size. At 2%, those figures have to double to $534 million dollars or ~$604,000/acre. Is anyone going to pay ~$300,000 to $600,000/acre for that land?
In my opinion, this is why AZ K-12 education funding is in crisis. The crisis will only deepen, and beneficiaries of the Trust will be more and more harmed, if Site Specific Plans like this are applied to the millions of acres of State Trust Land.
Solution: Future Revenue Stream Must Cover Future Expenses
When ASLD demands aggressive rezoning from a Town in order to achieve the highest selling price for a tract of State Trust Land, ASLD should be required by affected towns and school districts to demonstrate, from its appraisals and data on K-12 education costs, that the predicted future revenue stream will equal the predicted future expense stream. The farce of ASLD simply trumpeting their record-breaking revenue additions through land sales without revealing that it was accomplished by taking on more student expenses than the expected revenue and school tax stream will support has got to stop.
Parting Shot: Don't Forget Water Liabilities Either
The 860,000 gallons/day required by this plan (p. 75, Water, 2nd paragraph) is another piece of "the rest of the iceberg." What is going to happen with regard to AZ water demand if this pilot project goes Statewide, with Towns and developers eagerly adopting its aggressive rezoning and entitlement techniques? With Arzona currently under a Drought Contingency Plan, this is, in my opinion, another reason for Oro Valley to reject this pilot plan out of concern for the whole State, and take it up only after the overallocation of the Colorado has been dealt with.
The little-known "pilot plan" aspect of this annexation should have been discussed with the public and their elected officials before trying to push it through a struggling Town approaching buildout.
View the Site Specific Plan HERE
Jim Tripp has a Bachelor's degree in Biological Sciences from Cornell University and a Ph.D. in Molecular and Cellular Biology from Oregon State University. Prior to retirement, he was employed as a Federal Regulations Analyst for Wisconsin Power and Light and as a Research Scientist at UC Santa Cruz and Berkeley National Labs. He has over 30 scientific publications to his credit.
Labels: ASLD, Site Specific Plan, State Trust Land, Tangerine State Land Annexation
Guest View: Jim Tripp ~ The Rest of the Iceberg. Part 1: Fear Mongering by Solomon and Rodman
One June 17th, LOVE published a Guest View by Jim Tripp entitled, "The Tip of the Iceberg." It included a wealth of previously unknown information on the proposed annexation of State Land at Tangerine and Thornydale including the blatant conflict of interest of two people involved in the project. If you missed it, you can read it HERE
We now present "The Rest of the Iceberg"
What's the rest of the iceberg?
Take a look at this video of Rodman and this video of Solomon warning the Oro Valley Town Council to rezone the Trust Land at Tangerine and Thornydale to the State's satisfaction, or suffer the consequences at the hands of the town of Marana.
Rodman video at 31 seconds in:
"We should consider the fact that if we don't do it, Marana will. I mean, we've heard those words directly."
Note his stress on the word directly.
Solomon video at 5 seconds in:
"This land will be developed, and the odds are if it's developed outside of Oro Valley, it's gonna be at a higher intensity, with less restrictions than what Oro Valley would have, and all that development is going to have an impact on Oro Valley..."
What facts does Solomon have to back up this opinion?
No Need to Fear: Marana Can't Deliver Water
In a nutshell, I had two lengthy phone conversations with Marana Town Mayor Ed Honea to fact-check Marana's interest in the Tangerine and Thornydale annexation. Honea said that Marana has no interest whatsoever in the land because Marana cannot deliver an adequate water supply. In contrast, Oro Valley can easily deliver water via two, 12" potable water mains. Honea told Satish Hiremath long ago that Oro Valley was welcome to annex the State Land.
Please visit this facebook post of mine to learn more.
Marana Town Finance Director, Yiannis Kalaitzidis, approached me as I was leaving a Marana Town meeting. He asked what had prompted me to ask a question related to K-12 population projections for Marana. I said that it was in connection with the proposed annexation at Tangerine & Thornydale. During the course of the conversation, he reiterated what Ed Honea had said: only Oro Valley can deliver water to the annex, and if Oro Valley doesn't annex, it will be decades before Marana can get enough water there to make development economically possible.
So who are the powerful people in Marana who have said directly that Marana will snap up the land and intensely develop it, if Oro Valley doesn't?
Please visit this facebook post as well.
No Need to Fear: Mayor Honea Respects the Sonoran Desert Conservation Plan
During the May 14, 2019 study session on the Marana 2040 General Plan, Mayor Honea fought hard for "low density 2-RAC" (no more than 2 residences per acre) in environmentally sensitive areas like Tangerine from I-10 to Twin Peaks. In defense of continuing the extensive use of "2-RAC" from the 2010 General Plan, rather than pitching it in the 2040 Plan, Honea said:
"When we developed the low density 2-RAC, we had buy-in from the Sonoran Desert Conservation Group, Carolyn Campbell, [and others]; they helped approve that. And you know why, when we developed everything along Twin Peaks, and we did 2-RAC, and we didn't have the environmental community down our necks, is because they were involved in the process, for the 2-RAC...when you take that away, I can assure you, they will be back."
You can watch it HERE (Time mark 51:23 on the video)
The Sonoran Desert Conservation Plan was a landmark achievement for Northwest Tucson. When was the last time you heard an Oro Valley Mayor or Council Person worry about the consequences of not honoring that plan? Does anyone in Oro Valley remember that plan? It was never mentioned in any of the meetings I've been to in Oro Valley. Ed Honea remembers, and he got the message the first time: don't antagonize Dove Mountain area citizens with high intensity development.
Dove Mountain Marana citizens are environmentally conscious. In Sky Ranch and at The Preserve, we are fiercely protective of the low-density nature preserves on which we live. We love watching the bobcats, javelinas, coyotes, hawks, and owls that patrol the open spaces beyond our backyards, and we will fight to protect them.
Supply and Demand: Marana Has Plenty of Annex Opportunities Other Than This One
Figure 4, page 2-7 (below) of the current Marana 2040 General Plan shows an ocean of grey shaded land, especially adjacent to I-10 in the North. That's all vacant and undeveloped land. Marana will have no need, for many decades to come, to force high intensity development at Tangerine and Thornydale.
You can view the Marana 2040 General Plan HERE
Oro Valley has the only game in town when it comes to annexation of the State Trust Land at Tangerine and Thornydale. There is no reason to fear competition from Marana.
Part 2 will be published next Monday.
Labels: Bill Rodman, Sonoran Desert Conservation Plan, Steve Solomon, Tangerine State Land Annexation
LOVE returns on July 8th
For the month of July, we will be taking a "mini-vacation" and publishing only on Mondays.
We wish all our readers a Happy 4th of July!
Below is a list of Town events for the July 4th holiday.
More information is available HERE
Behind the Scenes...
LOVE has recently begun receiving letters from residents who live along the golf courses complaining about the content of the Watchdog Reports. Just prior to this, Mike Zinkin shared with us a portion of an email that he received from an Oro Valley resident informing him that his Watchdog Reports, "will no longer go unnoticed nor unchallenged" and that "a significant number of very talented individuals have come forward in that regard."
While LOVE has no issue with presenting opposing sides (and we have done so many times as long as the letters are respectful), we believe it is best when an individual presents their views as an individual and not as part of a cabal that has been formed to gang up on one person. We also believe that if a writer has a personal stake in the topic being discussed, that they should disclose this information upfront rather than presenting themselves as an objective bystander.
We find these truths to be…
What we have seen in the majority of letters submitted to LOVE (and in many of the letters submitted to the Explorer as well) is that the letter writer makes no mention of having a personal stake in the issue. But a little investigating on our part always unearths these truths.
LOVE received a letter from George and Sheila Lindsay (the same letter that was published in the Explorer last week). Their letter asserted that the Town needs to keep the golf courses because "the El Conquistador has hosted at least 13 charitable tournaments so far this fiscal year" and that these fundraisers "help the community." And while no one would argue with hosting charitable events, the Lindsay's made no mention of the fact that they have a personal stake in this issue as they own a home along the golf course.
The elephant in the letter
While Edward Cooke, whose letter we published yesterday, did sign his name as being the "former president of the Canada Hills Master Association" he did not state what his current connection was to the golf courses…which is that his home is adjacent to one of them. His letter discussed loss of tax revenue, winter visitors no longer visiting Oro Valley for golf, and that restaurants, hotels, and OV Marketplace "will suffer greatly" and "people will lose their jobs" should the golf courses close.
The burden of proof for those assertions is on the writer. Is there any evidence that when golf courses closed in other cities/towns, that it led to businesses and hotels suffering greatly, which in turn, led to people losing their jobs?
It's fine to have concerns about all of those things, but we found it suspicious that a person who owns a home along the golf course would just happen to not mention anything in his letter about concerns of loss of property value. It was the "elephant in the letter" that no one was supposed to notice.
The difference between Naranja Park and the Golf Courses
Mr. Cooke also asked why spending tax dollars on Naranja Park was any different from spending tax dollars on the golf courses. He wrote:
"Why is the O.V. Council spending money ($1.350M) on Naranja Park when the residents of O.V have voted the park down on numerous occasions? How many dollars does Naranja Park generate for the town? How much are we spending to maintain this park annually?"
Our response is that Naranja Park is free and available to every citizen of Oro Valley. This is not the case for the 18-hole dedicated golf course for the golf members. Residents have to pay a "daily fee" to use the golf courses if they are not a golf club member. Both Naranja Park and the Aquatic Center also host events that bring families and out-of-towners into Oro Valley where they stay at our hotels (bed tax revenue) and eat in our restaurants and shop in our stores (sales tax revenues). This is something that an 18-hole dedicated golf course does not do. There is a big difference between a public park and a private golf course.
Remember…Golf was at the bottom of the list
LOVE believes that the majority of the 43,000 Oro Valley residents think a town-owned golf course is a bad idea. That's why they came out in great numbers to speak against it when it was first brought to the public's attention in December 2014, and have continued speaking against it in numerous LOVE Guest Views and letters to the editor. It's also why golf placed 33 out of 34 amenities that Oro Valley residents requested in the Town-sponsored Parks and Recreation Survey in June 2014.
LOVE Editor
Labels: Canada Hills, El Con Golf Courses, Naranja Park
Guest View-Edward Cooke: "Get The Facts On The Golf Course"
We received the following email from an individual who lives on Carmel Pointe Drive along the golf course, though he does not state such in his email.
LOVE is based on full-disclosure and honesty.
To us this means that people who have a self interest in the result of an event should disclose such in their communications to us. Submitting emails to us that pretend to be altruistic, when they are indeed self-serving is, indeed, wrong.
We're publishing this as an illustration of what is being "tossed around" out there.
"LOVE needs to be more fair with their articles regarding the Oro Valley golf courses.
I really believe that all the Oro Valley Parks and Recreation financials need to be included in your articles, not just the lambasting of the golf courses. You would be surprised how many people I have spoken to that have no idea how much money Oro Valley is losing on the Aquatic Center.
Why is the Oro Valley Council spending money ($1.350M) on Naranja Park when the residents of Oro Valley have voted the park down on numerous occasions? How many dollars does Naranja Park generate for the town? How much are we spending to maintain this park annually?
[Comments derogatory to the writer of a previous LOVE guest view were removed. We do not publish personal attacks]. I ask that all Oro Valley residents ... get the true facts and to decide for themselves what the actual numbers are. You will be very surprised.
Lastly, remember if the golf courses are shutdown the town of Oro Valley will suffer substantial tax revenue losses. Winter visitors who rent the golf villas or private homes will no longer come to Oro Valley for their golf. Restaurants, hotels, the Oro Valley Marketplace will suffer greatly. People will lose their jobs. Is this what we want to happen?
Winter visitors are not going to come to Oro Valley to walk on linear parks, bicycle trails left to grow as natural vegetation, surrounded by houses. We have sufficient walking trails all through Oro Valley including Catalina State Park.
The golf courses are now producing revenue. Let them continue. Instead of denigrating golf, work to keep the junior golf, First Tee viable for our young people and keep Oro Valley Green.
I sincerely hope the new mayor and council consider the ramifications closure of the golf courses will cause the community.
Edward Cooke
Former president Canada Hills Master Association"
Labels: Community Center, El Conquistador Country Club, Golf
The Watchdog Report: April 2019 Community Center Financials
The Community Center Fund (CCF) ended April 2019 with a positive balance of $698,301. Although a positive balance of this magnitude is a good sign, there are a lot of promised obligations that need to be fulfilled…and they're not being fulfilled.
What happened to ADA compliance?
We have owned this property since May 2015 and it is still not ADA compliant. Why isn't the Town Manager funding an elevator for the Community Center? Does anyone care about our citizens who are disabled and currently have to enter the building through the loading dock? What happened to the funding for ADA and Code Compliance and Life Safety Issues that was shown during the Power Point presentation in December 2014?
ADA and Code Compliance Life Safety Issues
FY 2014/15 $381,000
FY 2016/17 $69,000
TOTAL $1,143,000
Greg Caton (Town Manager in 2014) promised that between FY 2014/15 and FY 2018/19 that the Town would spend $1,143,000 to remedy these issues. Fiscal year 2018/19 ends on June 30th and to-date the Town has spent ZERO on ADA compliance.
What happened to paying back the $1.2 million dollar loan?
In 2015 the Town Council borrowed $1.2M from the General Fund to start the Community Center Fund with a promise to pay back $120,000 per year for 10 years. There has been no transfer of the promised annual $120,000 from the CCF to the General Fund.
Gains and Losses
Troon lost $85,220 in April 2019, bringing their losses to date to $1,267,303.
The Overlook lost $2,232 in April bringing its total losses so far this fiscal year to $89,679. Since the Overlook opened in 2015 it has lost $556,141. Of interest is that four years into this endeavor they are still losing more than what they've budgeted to lose. Budgeted losses YTD were $58,712. Actual losses YTD are $89,679. (Difference of $30,967).
The Town part of the investment (fitness, recreation, swimming) made a little over $125,000 as of April 2019. There is nothing wrong with the Community Center part of the investment; it is golf that continues to be a financial drain on the Town. So far this fiscal year your sales tax revenues dedicated to the Community Center and Golf amount to $2,033,576 (as of April 2019).
I recently submitted a Freedom of Information request asking for the number of employees assigned to maintain the golf courses, including supervisors and mechanics, and the total water usage for 36 holes (either in gallons or acre feet). The Town responded that they did not have the requested documents because these items are not broken down individually. I'm not sure if this is stonewalling or irresponsible management. How can the Town not know how much water is utilized or how many employees are utilized for golf maintenance? I am trying again with a revised submittal.
I am currently working on a plan for an 18-hole, strictly municipal model for golf. Town Manager, Mary Jacobs, seems to be leaning towards the 36-hole model if the adjacent HOA's supplement the Town via increased HOA dues. The recently passed budget still includes the Overlook and the 36-hole model. One wonders what it will take to get the Town Manager to understand that the current model for golf is not working.
Mike Zinkin has a Bachelor's degree in history and government from the University of Arizona and a Master's degree in Social and Philosophical Foundations of Education from California State University, Northridge. He was a commissioned ensign in the United States Navy Reserve. He was an Air Traffic Controller for 30 years. He and his wife moved to Oro Valley in 1998. Mike served on the Oro Valley Development Review Board from 2005-2009 and the Board of Adjustment from 2011-2012. He served on the Town Council from 2012-2016 during which time he was named a Fellow for the National League of Cities University, he was a member of the National League of Cities Steering Committee for Community and Economic Development, and a member of the Arizona League of Cities Budget and Economic Development Committee.
Labels: ADA compliance, Community Center, El Con Golf Courses, Golf, Overlook Restaurant, Troon
More Oro Valley Stores Closing
Store closings are a nationwide problem
LOVE has noted that stores are closing in Oro Valley. Empty storefronts are not just an Oro Valley problem. It's a nationwide problem. There are lots of reasons for it.
Recent Oro Valley retail store closings, like the closing of Platinum Fitness in April, or now the closing of the Alfonso's Olive Oil and Balsamic store, Rigazzi's and a cleaners in the Trader Joe's Mall are gaining attention on Nextdoor.com.
Nextdoor.com readers speculate on the causes
A recent comment that was posted on Nextdoor.com spawned an interesting conversation.
The originator of the posting (see panel) suggested that the council get involved in retaining business. Others responded, citing host of reasons why stores close including:
The seasonal transient nature of some Oro Valley residents
High lease rates (which was the cause of the closing of Platinum Fitness)
Oro Valley's higher than competing communities sales tax rate
The rise of online shopping
Store closings are really the problem of the store owner
It's far too easy to point to outside forces causing a retail business to fail. Our experience in working with retailers for 60 plus years has taught us that there are really six possible causes of a store's failure. Any one or a combination of these can do a store in!
There wasn't a market for the product the retailer sells in first place;
The store is just another "me too" business;
Poor location;
The retailer failed to bring sufficient capital to weather the startup time it takes to get a business established;
The economic formula for making the business a success just wasn't there. For example, if the rent is going to be too much in relation to the business that will be done then the store is simply not financially feasible; and
Store management simply did not know how to operate the store efficiently. For example, they buy too much inventory or too much of the wrong inventory. So, they have to mark down the product to get rid of it or customers walk out because what they want isn't there.
Can the council fix this problem?
Some Nextdoor.com commenters suggested that the town council do something to fix this problem. The only factor that the council controls is the sales tax. Reducing the sales tax is hard to do until the council fixes the hemorrhaging losses of the town owned country club community center. We will learn more about the options and the possible financial impact of them at tomorrow's regular council meeting.
More real Oro Valley jobs paying real wages can pave the way to retail store success
The hope for Oro Valley is that Oro Valley Economic Development Director JJ Johnston's five year comprehensive economic development strategy will work. As we have previously written, it calls for bringing in non retail businesses to bolster real employment in our community. The UA Veterinary School is an example of this. Once the town has more "real jobs that pay real wages" the town will have more people working here full-time who will need and who will visit retail stores.
Labels: Economic Development, JJ Johnston
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Discussion in 'Reviews' started by Pinelogcreek, Jun 15, 2018.
I've been wearing a pair of Altra Lone Peak 3.5's for a couple months now and in the last two weeks have given them a strong workout. I'm usually wear size 10.5 shoes and 11 in hikers. I ordered 11.5 in these bases on reviews and I'm glad that I did. No more toes hitting going downhill. Week one I tramped around SW Virginia putting in miles on rocky trails and farm fields. The grip on rocks was good, they stayed cool as any shoe would hiking. The lateral stability was good also. The second week was visiting Washington DC with my family. Here we averaged 8-10 miles per day on asphalt and concrete. I was prepared for issues in my mind but I was pleasantly surprised that my feet were not sore at night, more importantly my knees and hips did better than in my previous Brooks shoes. I really enjoy the wide toe box that lets the foot spread out naturally. I know shoes are a personal thing but I have been well satisfied with these.
Plus one on these. Great set of shoes. Highly recommend!
I should absolutely point out, and agree that sizing up on these is mandatory. I wear a 10.5 wide and have to wear a 12 in these.