Arecibo IS radar (Qihou Zhou, zhou@naic.edu) and Fabry-Perot (Craig Tepley, craig@naic.edu)

The Arecibo Observatory is operated by Cornell University under cooperative agreement with the National Science Foundation.

Arequipa Fabry-Perot (Manfred Biondi, biondi@vm3.cis.pitt.edu)

The Arequipa Automated Airglow Observatory is operated by the University of Pittsburgh with support from the National Science Foundation. Space and on-site technical support are provided by the National Aeronautics and Space Administration.

Argentia Digisonde (Jim Scali, james_scali@uml.edu)

The Argentia Digisonde is owned and operated by the US Air Force Research Laboratory (AFRL) at Hanscom Air Force Base. The data is analyzed, processed and supplied by the University of Massachusetts Lowell Center for Atmospheric Research under contract with AFRL.

Chatanika IS Radar (John Kelly, kelly@sri.com)

The Chatanika incoherent scatter radar was supported by the National Science Foundation.

EISCAT (Peter Collis, peter@eiscathq.ird.se)

The EISCAT Scientific Association is supported by Centre National de la Recherche Scientifique of France, Suomen Akatemia of Finland, Max-Planck-Gesellschaft of Germany, Norges Almenvitenskapelige Forskningsraringd of Norway, Naturvetenskapliga Forskningsraringsdet of Sweden, National Institute for Polar Research of Japan and the Science and Engineering Research Council of the United Kingdom.

Goose Bay HF Radar (Michael Ruohoniemi, ruohoniemi@jhuapl.edu)

The Goose Bay HF radar is operated by the Applied Physics Laboratory of The Johns Hopkins University with support from the National Science Foundation.

Halley Fabry-Perot (Matthew Paley, mtpa@pcmail.nerc-bas.ac.uk)

The Halley Fabry-Perot Interferometer is operated by the British Antarctic Survey which is part of the United Kingdom's Natural Environment Research Council.

Halley HF Radar (Michael Pinnock, mpi@pcmail.nerc-bas.ac.uk)

The Halley HF radar is jointly supported by the British Antarctic Survey, which is part of the United Kingdom Natural Environment Research Council, and the National Science Foundation Division of Polar Programs.

Hankasalmi HF Radar (Mark Lester, mle@ion.le.ac.uk)

The CUTLASS (Co-operative UK Twin Located Auroral Sounding System) radars form part of the SuperDARN (Dual Auroral Radar Network) HF project and consist of radars at Hankasalmi, Finland and Pykkvibaer, Iceland. They are operated by the Radio and Space Plasma Physics Group at the University of Leicester with support from the Particle Physics and Astronomy Council, and additional support from the Finnish Meteorological Institute and the Swedish Meteorological Institute.

Jicamarca IS Radar(dataMarch 1995: Erhan Kudeki, kudeki@uiuc.edu; Farady data: David Hysell, daveh@vlasov.phys.clemson.edu)

The Jicamarca Radio Observatory is operated by the Geophysical Institute of Peru, Ministry of Education, with support from the National Science Foundation as contracted through Cornell University.

Kapuskasing HF Radar (Michael Ruohoniemi, ruohoniemi@jhuapl.edu)

The Kapuskasing HF radar is operated by the Applied Physics Laboratory of The Johns Hopkins University with support from the National Aeronautics and Space Administration and the National Science Foundation.

Millstone Hill Digisonde (Jim Scali, james_scali@uml.edu)

The Millstone Hill Digisonde is owned and operated by the US Air Force Research Laboratory (AFRL) at Hanscom Air Force Base. The data is analyzed, processed and supplied by the University of Massachusetts Lowell Center for Atmospheric Research under contract with AFRL.

Millstone Hill Fabry-Perot (Dwight Sipler, dps@haystack.mit.edu)

The Millstone Hill Fabry-Perot is supported by the National Science Foundation.

Millstone Hill IS Radar (John Holt, jmh@haystack.mit.edu)

The Millstone Hill IS radar is supported by the National Science Foundation.

Pykkvibaer HF Radar (Mark Lester, mle@ion.le.ac.uk)

The CUTLASS (Co-operative UK Twin Located Auroral Sounding System) radars form part of the SuperDARN (Dual Auroral Radar Network) HF project and consist of radars at Hankasalmi, Finland and Pykkvibaer, Iceland. They are operated by the Radio and Space Plasma Physics Group at the University of Leicester with support from the Particle Physics and Astronomy Council, and additional support from the Finnish Meteorological Institute and the Swedish Meteorological Institute.

Qaanaaq Digisonde (Jim Scali, james_scali@uml.edu)

The Qaanaaq Digisonde is owned and operated by the US Air Force Research Laboratory (AFRL) at Hanscom Air Force Base. The data is analyzed, processed and supplied by the University of Massachusetts Lowell Center for Atmospheric Research under contract with AFRL.

St. Santin IS Radar (Christine Amory-Mazaudier, mazaudier@cetp.ipsl.fr)

The extension of the CNET (Centre National d'Etudes des Télécommunications) incoherent scatter facility at St.-Santin to a quadristatic configuration was supported by the Institut d'Astronomie et de Géophysique and by the Direction des Recherches et Moyens d'Essais. The facility is operated with financial support from the Centre National de la Recherche Scientifique.

Saskatoon HF Radar (George Sofko, sofko@skisas.usask.ca)

The Saskatoon HF radar is operated by the University of Saskatchewan with support from the Natural Sciences and Engineering Research Council of Canada.

Sondre Stromfjord Fabry-Perot (Rick Niciejewski, niciejew@umich.edu)

The Sondre Stromfjord Fabry-Perot is operated by the University of Michigan with support from the National Science Foundation.

Sondrestrom IS Radar (John Kelly, kelly@sri.com)

The Sondrestrom incoherent scatter radar is supported by the National Science Foundation.

Stokkseyri HF Radar (Jean-Paul Villain, jvillain@cnrs-orleans.fr)

The Stokkseyri HF radar is operated by CNRS/LPCE (Centre National de la Recherche Scientifique/ Laboratoire de Physique Chimie de l'Environnement) and CNRS/CETP (Centre d'etudes des Environnements Terrestre et Planetaires) with support from the Institut National des Sciences de l'Univers.

Syowa Station HF Radar (Natsuo Sato, nsato@nipr.ac.jp)

The Syowa Station HF radar is operated by the National Institute of Polar Research in Japan.

Thule Fabry-Perot (Rick Niciejewski, niciejew@umich.edu)

The Thule Fabry-Perot is operated by the University of Michigan with support from the National Science Foundation and from Phillips Laboratory, which is operated by the United States Air Force. Phillips Laboratory was formerly Geophysics Laboratory, which was formerly the Air Force Geophysics Laboratory.

Watson Lake Fabry-Perot (Rick Niciejewski, niciejew@umich.edu)

The Watson Lake Fabry-Perot is operated by the University of Michigan with support from the National Science Foundation and the United States Air Force.

II) Satellite Data

NOAA Electron Precipitation Data (Dave Evans, devans@sec.noaa.gov)

The NOAA electron precipitation data were provided by Dave Evans of the Space Environment Center.

DMSP Electron Precipitation Data (Fred Rich, rich@plh.af.mil; Herb Kroehl, hwk@ngdc.noaa.gov)

The Defense Meteorological Satellite Program electron precipitation data were provided by Fred Rich of the Air Force Research Laboratory or by Herb Kroehl of the National Geophysical Data Center.

DMSP IDM Data (Fred Rich, rich@plh.af.mil; Rod Heelis, heelis@utdallas.edu)

The Defense Meteorological Satellite Program Ion Drift Meter data were provided by Fred Rich of the Air Force Research Laboratory or by Rod Heelis of the University of Texas at Dallas.

DMSP IDM/RPA Data (Rod Heelis, heelis@utdallas.edu; Marc Hairston, hairston@utdallas.edu)

The Defense Meteorological Satellite Program Ion Drift Meter or Retarding Potential Analyzer data were provided by Rod Heelis or Marc Hairston of the University of Texas at Dallas.

DMSP Magnetometer Data (Fred Rich, rich@plh.af.mil)

The Defense Meteorological Satellite Program magnetometer data were provided by Fred Rich of the Air Force Research Laboratory.

UARS MEPS Data (Rudy Frahm, rudy@pemrac.space.swri.edu)

The Upper Atmosphere Research Satellite MEPS electron precipitation data were provided by Rudy Frahm of the Southwest Research Institute.

UARS AXIS Data (Rudy Frahm, rudy@pemrac.space.swri.edu; Dave Chenette, chenette@pemacs.space.lockheed.com)

The Upper Atmosphere Research Satellite AXIS X-ray image data were provided by Rudy Frahm of the Southwest Research Institute or by Dave Chenette from Lockheed/Martin Corporation.

POLAR UV Image Data (Dirk Lummerzheim, lumm@loke.gi.alaska.edu)

The UV imager data from the POLAR satellite were provided by Dirk Lummerzheim of the University of Alaska.

III) Ground Magnetometers

NGCD (http://julius.ngdc.noaa.gov:8080/index.html; Les Morris, lmorris@ngdc.noaa.gov)

The National Geophysical Data Center provided several magnetometers.

CANOPUS chain: CNL RIT EKP FCC BKC FSM FSP RAL GIM DAW FMC ISL PIN (http://www.dan.sp-agency.ca/www/canopus_home.html; Terry Hughes, hughes@dan.sp-agency.ca; Follow CANOPUS Rules of the Road, need article list)

The CANOPUS instrument array was constructed and is maintained and operated by the Canadian Space Agency.

EMR Canadian data: ALE RES MBC CBB BLC YKC FCC PBQ MEA STJ OTT VIC GLN (http://gdcinfo.agg.emr.ca/geomag/; Gerrit Van Beek, vanbeek%mvax4.decnet@geolab.emr.ca)

Energy Mines and Resources Canada provided several magnetometers.

MACCS array: PG, CY, CD, IG, CH, RB (RPB), PB, GH (also use IQA) (Mark Engebretson, engebretson@auggie.span.nasa.gov; Jeff Hughes, hughes@bu.edu)

The MACCS magnetometer array was provided by Mark Engebretson of Augsburg College or by Jeff Hughes of Boston University.

DMI array: west coast: THL SVS KUV UPN UMQ GDH ATU STF SKT GHB FHB NAQ; central: MCG MCN MCW (MAGIC, see below); east coast: NRD DMH DNB SCO AMK; Denmark: BFE (Peter Stauning, pst@dmi.min.dk; need to hear from users)

The Danish Meteorological Institute provided several magnetometers.

MAGIC: MCG MCN MCW (http://www.sprl.umich.edu/MIST; Bob Clauer, clauer@zasu.sprl.umich.edu)

The MAGIC array operated by the University of Michigan provided several magnetometers.

SAMNET: FAR GML YOR NOR KVI OUL NUR (David Milling, dave@aurora.york.ac.uk)

The SAMNET magnetometer array was provided by David Milling of the University of York.

IMAGE: NAL LYR HOR HOP BJN SOR KEV TRO MAS KIL MUO SOD PEL ALT KAU (http://www.geo.fmi.fi/image/; Hermann Luehr, luehr@geophys.nat.tu-bs.de; Ari Viljanen or Lasse Hakkinen, ari.viljanen@fmi.fi or lass.hakkinen@fmi.fi)

The Image magnetometer data were provided by Hermann Luehr of the Technische Universitat of Braunschweig or by Ari Viljanen or Lasse Hakkinen of the Finnish Meterorological Institute(?).

BAS: AIA and HBA (Alan Rodger, u_asr@vc.nbs.ac.uk)

Several magnetometers were provided by Alan Rodger of the British Antarctic Survey.

BGS: ESK HAD LER (Toby Clark, e_tdgc@vaxa.nerc-murchison.ac.uk)

Several magnetometers were provided by Toby Clark of the BGS (British Geological Survey?).

SIBIZMIR: IRT, YAK, MGD, NVS, SVD(ARS), PET, VLA, POD (Vilen Mishen, root@sitmis.irtusk.ru, subject: message for Dr. Vilen Mishen, mostly analog)

Several magnetometers were provided by Vilen Mishen of SIBIZMIR, Irkutsk.

AAR: HIS, DIK, CCS, CWE, MIR (Oleg Troshichev, oleg@omr.izmi.ras.spb.ru)

Several magnetometers were provided by Oleg Troshichev of the Arctic and Antarctic Research Institute in St. Petersburg.

Bell Labs: IQA TKN PTA MCM SPA (Carol Maclennon, cgm@physics.att.com)

Several magnetometers were provided by Carol Maclennon of Bell Labs.

Antarctic Russian array: VOS KOM PIO MIR (http://www.sprl.umich/edu/MIST; Vladimir Papitashvili, papita@zasu.sprl.umich.edu)

Several magnetometers were provided by Vladimir Papitashvili of the University of Michigan (plus Russian acknowledgment?).

Terra Nova Bay (TNB) (A. Meloni or Lili Cafarella, meloni@in8800.ingrm.it or cafarella@in8800.ingrm.it)

The Terra Nova Bay magnetometer data were provided by A. Meloni or Lili Cafarella of ING.

210 chain: MCQ ADL DLB BRV LRM DRW WEP GUA CBI EWA KAG ONW MSR CHD TIK CAN ASA WTK WEW BIK PTN KOR YAP MUT LNP BJN PTK IRT MGC YAK ZYK AGN KOT KTN (http://www.stelab.nagoya-u.ac.jp/omosaic/goin95/geomag.html; K. Yumoto at yumoto@geo.kyushu-u.ac.jp, needs to review acknowledgements)

Acknowledgements for the 210 MM Chain

NOTE: The degree sign should follow all uses of '210'.
Rules: Taken from web site: http://www.stelab.nagoya-u.ac.jp/omosaic/goin95/geomag.html
from the README on anonymous ftp site: 133.47.128.10
from the list of co-investigators on the 210 MM chain
from the reference: Yumoto, K. and the 210 MM Magnetic Observation Group, The STEP 210 magnetic meridian network project, J. Geomag. Geoelec., in press, 1996.

A) Contact PI Dr. K. Yumoto in all cases at yumoto@geo.kyushu-u.ac.jp and let him review the acknowledgments, references, paper, etc.
B) Contact Co-I Dr. K. Shiokawa at shiokawa@stelab.nagoya-u.ac.jp if any data is removed from the web or anonymous ftp site.
[NOTE: All data is labelled XYZ but is in HEZ nT. Z is + upward for all SH stations since Aug 12, 1993 or earlier, so sign is changed to be + downward. All NH stations (including YAP and KOR) have Z + downward. Both CBI and WWK have Y(E) + westward, so this sign must be changed to be + eastward.]

1) When the 210 MM data are essential in the publication and presentation, the user is requested to offer an authorship to the PI and members of the 210 MM team.

2) If no one on the 210 MM team participates as an author, the paper should acknowledge the 210 MM team and STEL for the use of the data base and should refer to the following papers:
a) Yumoto, K., Y. Tanaka, T. Oguti, K. Shiokawa, Y. Yoshimura, A. Isono, B. J. Fraser, F. W. Menk, and the 210 MM Magnetic Observation Group, Globally coordinated magnetic observations along 210 magnetic meridian during STEP period, 1, Preliminary results of low-latitude Pc 3's, J. Geomag. Geoelec., 44, 261-276, 1992.
b) Yumoto, K. and the 210 MM Magnetic Observation Group, Initial results from the 210 magnetic meridian project - Review, J. Geomag. Geoelec., 47, 1197-1213, 1995.
[NOTE: Would probably prefer to reference the in press article on the network project since the data would often be taken from there.]

General acknowledgment:

The authors would like to aknowledge use of the 210 Magnetic Meridian (MM) data. The PI K. Yumoto manages the 210 MM observations project and group. The database is located at the Solar-Terrestrial Environment Laboratory (STEL) at Nagoya University.

Specific acknowledgments for each station used (can be combined for institutions that manage more than 1 station):
[NOTE1: Only Co-I's are named here, and those not associated with a particular station are not named (i.e., Shiokawa, Takahashi, Kokubun, Matsuoka, Osaki, Tanaka, Seto, Sakurai). This may be changed, especially in the cases where Dr. K. Shiokawa has provided the data, since he is one of those who is not specifically named. Also, others named in the 1996 JGG article could be named here.]
[NOTE2: The web acknowledgments did not label ISTP(IRT), IGCAS (BJI), GSARI (KAT), and STEL (MSR,KAG)]
[NOTE3: The 1996 JGG paper had additional institutions: Albatross Hotel, Katanning Research Station, Department of Agriculture (would this be GSARI?)]
[NOTE4: There was no name in the 210 Co-I team list for the following stations: BRV (POB), YAP (UK), IRT (ISTP), BJI (IGCAS), MSR+KAG (STEL)]
[NOTE5: Institutions not named below are: TIT, TKU, and GRL, since no station could be attributed to them from the list of stations.]

1) ADL, Electronics Research Laboratory (DSTO: K. J. W. Lynn), Australia
2) ASA, ??? (Albatross Hotel???)
3) BIK, Biak Aerospace Observatory (LAPAN Biak: Sukmadradjat), Indonesia
4) BJI, IGCAS??
5) BRV, Birdsville Police Station (POB), Australia
6) CAN, IPS Radio and Space Service (IPS: D. Cole), Australia
7) CBI, Kakioka Magnetic Observatory (KMO: S. Tsunomura), Japan
8) CHD, Institute of Cosmophysical Research and Aeronomy (IKFIA: S. I. Solovyev, G. F. Krymsky) and Institute of the Physics of Earth (IFZ: V. A. Pilipenko), Russia
9) DLB, Dalby Agriculture College (DAC) and University of Newcastle (UNC: B. J. Fraser, F. W. Menk), Australia
10) DRW, CSIRO Tropical Exosystems Research Center (TERC) and University of Newcastle (UNC: B. J. Fraser, F. W. Menk), Australia
11) EWA, NOAA/Pacific Tsunami Warning Center (PTWC: M. Blackford), USA
12) GAM (GUA), Guam Magnetic Observatory, (USGS: P. Hattori), Guam
13) IRT, ISTP???
14) KAG, Solar-Terrestrial Environment Laboratory (STEL: ???), Japan
15) KAT, Katanning Research Station (GSARI???) and University of Newcastle (UNC: B. J. Fraser, F. W. Menk), Australia
16) KOR, Koror Observatory of the US National Weather Service and the University of Alaska (UAF: J. V. Olson, S.-I. Akasofu), USA
17) KOT, University of Alaska (UAF: J. V. Olson, S.-I. Akasofu), USA
18) KTN, Institute of Cosmophysical Research and Aeronomy (IKFIA: S. I. Solovyev, G. F. Krymsky), Russia
19) LEM (LRM), Learmonth Solar Observatory (IPS: J. A. Kennewell) and the University of Newcastle (UNC: B. J. Fraser, F. W. Menk), Australia
20) LNP, National Central Univerisity (NCU: J. K. Chao) and Lunping Observatory (LNP: S.-W. Chen), Taiwan, Republic of China
21) MCQ, Australian Antarctic Division (ADD: R. J. Morris), Australia
22) MGD, Institute of Space Research and Radiowaves (IKIR: E. F. Vershinin, V. V. Bogdaroj, A. V. Buzevich)
23) MSR, Solar-Terrestrial Environment Laboratory (STEL: ???), Japan
24) MUT, Coast and Geodetic Survey Department (CGSD: R. B. Feir), Philippines
25) ONW, Tohoku University (THU: T. Takahasi), Japan
26) PTN, IRDC National Institute of Aeronautics and Space (LAPAN: S. L. Manurung, O. Sobari, M. Ruhimat), Indonesia
27) PTK, Institute of Space Research and Radiowaves (IKIR: E. F. Vershinin, V. V. Bogdaroj, A. V. Buzevich)
28) TIX (TIK), Institute of Cosmophysical Research and Aeronomy (IKFIA: S. I. Solovyev, G. F. Krymsky) and Institute of the Physics of Earth (IFZ: V. A. Pilipenko), Russia
29) WEP, Weipa North State School (WNSS) and University of Newcastle (UNC: B. J. Fraser, F. W. Menk), Australia
30) WTK, IRDC National Institute of Aeronautics and Space (LAPAN: S. L. Manurung, O. Sobari, M. Ruhimat), Indonesia
31) WWK, Paradise Wewak Hotel (PWH) and University of Papua New Guinea (UPNG: D. Yeboah-Amankwah)
32) YAK, Institute of Cosmophysical Research and Aeronomy (IKFIA: S. I. Solovyev, G. F. Krymsky), Russia
33) YAP, Kyushu University (UK: ???), Japan
34) ZGN, Institute of Cosmophysical Research and Aeronomy (IKFIA: S. I. Solovyev, G. F. Krymsky), Russia
35) ZYK, Institute of Cosmophysical Research and Aeronomy (IKFIA: S. I. Solovyev, G. F. Krymsky), Russia

NOTE: The stations would probably not be specifically named in the Acknowledgments, but the institutions and names in parentheses would be combined into 1 long sentence depending on what stations were used.