15-17 Sept99 Space Weather Campaign

Participant List

 Name

 Address

 Phone & Email

 Instrumentation/Modeling Support

 Saji Abraham  4 Nottinghill Ct Baltimore, MD 21244USA (301) 794-3018 <sabraham@estar.gsfc.nasa.gov>
  • Ionospheric Faraday rotation and scintillation studies.
 Joe Allen  SCOSTEP  <jha@luna.ngdc.noaa.gov>
  •  SRAMP Campaign coordination
 Mangalathail Ali Abdu    <abdu@dae.inpe.br>
  • Digisonde and optical measurements in the equatorial and low latitude loactions in Brazil.
 Anatoly Belov 142092 IZMIRAN, Troitsk, Moscow region, Russia <abelov@izmiran.troitsk.ru>
 David Boteler    Boteler@Geolab.nrcan.gc.ca
  •  SRAMP campaign coordination
Alan Burns  Space Physics Research Lab, University of Michigan, Ann Arbor, MI 48109-2143  734-763-6246 (tel) 734-763-0437(fax) <aburns@umich.edu>
  • Real-time GCM modeling of the thermosphere and ionosphere 
 Jinbin CAO  Center for Space Science and Applied Research, P.O. Box 8701, Beijing, 100080, P.R. China 86-10-62582644 (tel) 86-10-62576921 (fax) <jbcao@center.cssar.ac.cn>
  • 1.(two)Magnetometers - Purpose: Measure the geomagnetic pulsation. Located at geomagnetic (19.4N, 184.9E ), (28.9N, 186.1E)

Located at geographic (40.0N, 116.2E)

  • GPS Receiver - total Ne
  • Superneutron Monitor - cosmic ray intensity
  • ACK-1 Ionization Chamber -Measure cosmic ray meson intensity

Located at geographic (23.1N, 113.3E)

  • Scintillator multi-directional meson telescop - Measure cosmic ray directional intensity
  • Ion Composition sensor on board chinese meteorological Satellite FY-1C. Measures heavy ion, electron and proton flux. Orbit of FY-1C: Sunsynchronous orbit, h=870km, inclination =99
 J.K. (Jerry) Chao    <jkchao@jupiter.ss.ncu.edu.tw>
  •  SRAMP Campain coordination
David S. Coco   <coco@arlut.utexas.edu>
  • ionospheric tomography measurements from the Caribbean area
Helen E. Coffey NOAA NGDC E/GC2, 325 Broadway, Boulder, CO 80303 (303)497-6223 Work (303)497-6513(Fax) <hcoffey@ngdc.noaa.gov>
 Ashish Dasgupta Institute of Radio Physics and Electronics, University of Calcutta, 92, Acharya Prafulla Chandra Road, Calcutta-700009  Ph:+91-33-350-9115/9116/9413 Fax:+91-33-351-5828 <ashikp@cucc.ernet.in>
  •  Scintillation observations at 244 MHz from FSC, 1.5 GHz from INMARSAT and GPS. Spaced aerial observations at 244 MHz.
  • Useful data for global models, particularly, longitudinal dependence of ESF
Aleksey Dmitriev D.V. Scobeltsyn Institute of Nuclear Physics Moscow State University, Moscow, 119899, Russia Phone: +7 (095) 9394290 Fax:+7(095) 9395034 <dalex@srdlan.npi.msu.su>
 Yosuke Ebihara  Swedish Institute of Space Physics, Box 812, S-981 28 Kiruna, Sweden  <ebihara@irf.se>
  •  Ring current modeling depending on solar wind parameters. We will provide the results of the real-time simulation of the differential flux of ions and the Dst index at http://www.isc.nipr.ac.jp/~ebihara /rt.
 Thomas Farges  CEA, DASE/LDG, BP 12, 91680 Bruyeres le Chatel, FRANCE  <farges@ldg.bruyeres.cea.fr>
  •  1 ionosonde performing 1 ionogram per half of hour
  • 1 CW HF bistatic network with : 1 transmitter (48.6 N, 1.6E) transimitting CW at 4.6 MHz, 3 receptors far from the transmitter of 60 km in 3 directions
John C. Foster Millstone Hill Observatory MIT Haystack Observatory, Westford, MA 01886USA  (781) 981-5621 (tel.) (781)981-5766(fax) <jcf@haystack.mit.edu>
  •  Incoherent scatter radar observations of ionospheric characteristics over 15 deg latitude.
  • Directing ISR WLS World Day Campaign. Radar observations wil be scheduled for an active interval during Space Weather month.
 Nicola Fox  NASA/Goddard SFC  <Nicola.Fox@jhuapl.edu>
  •  ISTP program support
  • Maximized instrument coverage during the campaign interval
 Reiner Friedel  Space & Atmospheric Sciences, NIS-1, Mail Stop D-466, Los Alamos National Lab, Los Alamos, New Mexico, 87545, USA  <friedel@nis.lanl.gov>
  •  LANL geosynchronous satellites MPA & SOPA data
  • POLAR CEPPAD data
  • post-event analysis & modeling
  John M. Goodman  Radio Propagation Services, Inc., 8310 Lilac Lane, Alexandria VA 22308 +1-703-360-7127 (tel) +1-703-360-3954 (fax) <jmgood@erols.com>
  •  oblique-Incidence sounder recordings
  • raw ionograms of paths over US
  • Scaled maximum observable frequencies
Ray Greenwald   Applied Physics Lab (APL), Johns Hopkins University  <GreenRA1@ SPACEMSG.JHUAPL.edu>
  •  SuperDARN radar support
Vladimir I. Guselnikov Novosibirsk State University, Pirogova 2 st, Novosibirsk 630090, Russia 7(3832)397838 (tel.) 7(3832)397807(fax) <vgusel@phys.nsu.ru>
  • Flight data from Russian geostationary spacecraft EXPRESS-11, GALS-12.
  • The MIPE DIERA Patrol System for spacecraft charging investigation are mounted on both S/C.
  • Daily observations from electric field probes.
Marc Hairston  Center for Space Sciences, University of Texas at Dallas, PO Box 830688 FO22, Richardson TX 75083-0688  <hairston@utdallas.edu>
  • thermal plasma data from DMSP-F12 and F-13 spacecraft including in isitu ion flow (3 components), plasma density and composition, electrostatic potential (in the polar ionosphere), cross polar cap potential drop
  • available through http://utd500.utdallas.edu/~hairston /sept99.html
 Gary Heckman  NOAA, Space Environment Center  <gheckman@sec.noaa.gov>
 Mike Henderson  Space & Atmospheric Sciences, NIS-1, Mail Stop D-466, Los Alamos National Lab, Los Alamos, New Mexico, 87545, USA  <mhenderson@lanl.gov>
  • LANL geosynchronous satellites MPA & SOPA data
  • POLAR CEPPAD data
  • post-event analysis & modeling
 Joe Hirman  NOAA, Space Environment Center  <jhirman@sec.noaa.gov>
 Per Hoeg  Danish Meteorological Institute (DMI), Atmosphere Ionosphere Research Division (AIR), Lyngbyvej 100, DK-2100 Copenhagen, DENMARK +45 39 157 486 (tel) +45-39-157-460 (fax) <hoeg@dmi.dk>
  •  Ionosphere electron density profiles, TEC and TEC fluctuations based on GPS limb soundings from the satellite OERSTED. Global TEC measurements above the satellite orbital height (800 km).
  • Digisonde electron density profiles and ionosphere drift velocities from the Greenland Digisonde Chain (in cooperation with AFRL and University of Lowell)
  • Comments: The ORSTED GPS ionosphere measurements will be in 6 hour windows during the whole month of September. The Digisonde observations will be for the whole period with a 15 minutes time interval.
Robert A.Hoffman   NASA/Goddard SFC  <Robert.A.Hoffman.1 @gsfc.nasa.gov>
  • ISTP program support
  • Maximized instrument coverage during the campaign interval)
 Jean-Claude Jodogne    <jean-claude.jodogne@oma.be>
  • Dourbes Digisonde station is running 5 minutes soundings since September 3rd and will continue up to September 30th.
  • Hourly soundings will be manually scaled later but all data will be available in usual SAO-4 format 
  • Dourbes Digisonde data are shown in near-real time on the Web site: http://digisonde.oma.be
 Roberta Johnson  Space Physics Research Lab, University of Michigan, 2455 Hayward, Ann Arbor, MI 48109-2143 rmjohnsn@engin.umich.edu 
  •  SPARC outreach and education for the SRAMP campaign
Kirsti Kauristie  Finnish Meteorological Institute, Geophysical Research, P.O.Box 503, FIN-00101,Helsinki, Finland +358-9-19294637 (tel.) +358-9-19294603 (fax) <kirsti.kauristie@fmi.fi>
  •  Observations of the MIRACLE network, i.e. magnetometer, all-sky camera and ionospheric radar data. For more details, please, check http://www.geo.fmi.fi/ MIRACLE/
Tim Killeen   University of Michigan, Space Physics Res Lab, 2455 Hayward, Ann Arbor,MI 48109-2143  <tkilleen@umich.edu>
  •   Support from the Space Physics Research Collaboratory (SPARC)
 Alex Klimas  Code 692, NASA / Goddard Space Flight Center, Greenbelt, MD 20771  301-286-3682 (tel) <alex.klimas@gsfc.nasa.gov>
 Delores.Knipp Suite 2A25, Fairchild Hall, USAF Academy, CO 80840-6254 719-333-2560(tel) 719-333-3182(fax)  <delores.knipp@usafa.af.mil>
  • AMIE-statstical joule heating and electric potentials distributions binned by IMF
 Peter A. Knoop    <knoop@umich.edu>
  •  SPARC Campaign coordination
 Hannu Koskinen    <Hannu.Koskinen@fmi.fi>
  •  SRAMP campaign coordination
Valery Kozlov Insitute of Cosmophysical Research end Aeronomy., 677891,31 Lenin Ave.Yakutsk.Russia.  (4112)446322, (4112)445551 <v.i.kozlov@sci.yakutia.ru>
  • The early diagnosis method of large-scale IMF disturbances by registration of GCR intensity scintillation (by means of the correlation method of signal receive from the distant high-latitude neutron monitors) has been suggested.
  • It has been established that cosmic ray scintillation are associated with large-scale disturbances in the interplanetary magnetic field ( magnetic corks). The magnetic corks separate the particle trajectories into permitted and prohibited ones that is manifested in the celestial sphere scintillation in cosmic rays.
  • http://teor.ysn.ru/rswi/
  • http://teor.ysn.ru/LTKP/
Janet U. Kozyra  University of Michigan, Space Physics Research Lab, 2455 Hayward,Ann Arbor, MI 48109-2143  <jukozyra@engin.umich.edu>
  •  Modeling of the ring current evolution
William T. Kreiss 1100 W. Hollyvale Street, P.O. Box 296, Azusa, CA 91702-0296  Phone: 626/812-8050, FAX: 626/969-5772 <william.kreiss@aerojet.com>
  •  Short-term predictions for spacecraft applications (particle flux and charging).
MANOHAR LAL  Equatorial Geophysical Research Laboratory, Indian Institute of Geomagnetism, Krishnapuram BO, Maharajanagar PO, Tirunelveli-627011, India 091-0462-579465 (tel) 091-0462-579481 (Attn: Manohar Lal, EGRL) - Fax <lal_manohar@hotmail.com>
  • Magnetic component (H,Z, and D) from Variometer
  • Absolute magnetic field at ground
  • Surface pressure by using Microbarograph. This is being used for the study of generation of gravity waves at ground.
  • Comments: We are continously recording magnetic field variation and surface pressure variation at low latitude (8.7 deg N, 77.8 deg E).
Michael Liemohn   Univ. of Mich., SPRL 2455 Hayward St. Ann Arbor, MI 48109-2143 734-647-4705 (tel.) 734-647-3083(fax) <liemohn@umich.edu>
  •  Thermal and energetic plasma modeling.
Dirk Lummerzheim  University of Alaska, Geophysical Institute, Fairbanks, AK 99775-7320  (907)474-7564 (tel) (907)474-7290(FAX) <lumm@gi.alaska.edu>
 Henrik Lundstedt Swedish Institute of Space Physics, Solar-Terrestrial Physics Division, Scheelev. 17, SE-223 70 Lund, Sweden

+46-46-2862120 (phone) +46-46-129879 (fax) <henrik@irfl.lu.se>

homepage http:://www.irfl.lu.se
  •  Real-time predictions of geomagnetic indices Dst, AE, Kp, based on ACE solar wind data and with the use of neural networks at (http://www.astro.lu.se/~henrik/ spwrealfo.html)
  • Real-time predictions of satellite anomalies using neural networks.
  • Real-time measurements of geomagnetic induced currents (GICs) in Southern Sweden.
  • Preliminary neural network models of GICs.
  • NOTE: Space Weather, GICs and Effects - A Nordic GIC Meeting in Lund September 23-24
 Larry Lyons Department of Atmospheric Sciences, UCLA, Los Angeles, CA 90095-1565 310-206-7876 (tel) 310-206-5219(fax) <larry@atmos.ucla.edu> 
  • Evaluation of types of geomagnetic disturbances and their relation to solar wind inputs
 Kristy McAdams  Space & Atmospheric Sciences, NIS-1, Mail Stop D-466, Los Alamos National Lab, Los Alamos, New Mexico, 87545, USA  <kmcadams@nis.lanl.gov>
  •  LANL geosynchronous satellites MPA & SOPA data
  • post-event analysis & modeling
 David J. McComas  Los Alamos National Labs  <dmccomas@lanl.gov>
  •   ACE SWEPAM observations
  • LANL Geosynchronous particle data
 Mary McCready  SRI International, 333 Ravenswood Ave., Menlo Park CA 94025  650-859-5084 (tel) <mccready@sri.com>
  •  Involved in the WLS campaign
 Alan Manson ISAS, University of Saskatchewan, 116 Science Pl., Saskatoon, S7N 5E2 Canada  1-306-966-6449 (phone) 1-306-966-6428 (fax) <manson@dansas.usask.ca>
  •  MF radar observations of winds and waves 60-110km at Saskatoon 52N Tromso 70N
  • We have interest in response of tides and gravity waves to disturbances in the upper middle atmosphere or MLT
 Katsuhide Marubashi    <kmaru@crl.go.jp>
 Chris Meek  116 Science Place, University of Saskatchewan, Saskatoon, SK S7N 5E2, Canada  Phone: (306) 966-6446 <meek@dansas.usask.ca>
  •  MF radar continuous wind
  • signal strength
  • 60 - 100 km
 Steven Musman  NOAA Geosciences Research Division, National Geodetic Survey, NGS/6 Sta # 9840, 1315 East-West Highway, Silver Spring, MD 20910  (301)-713-2855 (tel) (301)-713-4475(Fax) <stevem@ulf.grdl.noaa.gov>
Torsten Neubert   Danish Meteorological Institute, Lyngbyvej 100, 2100 Copenhagen O,Denmark +4539-15-74-92 (tel) +4539-15-74-60 (fax) <neubert@dmi.dk>
  •  High precision measurements of earth's magnetic field from the Oersted satellite (high-inclination, LEO,launch Feb 23, 1999)
  • Energetic charged particles and GPS ionospheric/atmospheric sounding
Rick Niciejewski  Space Physics Research Lab, University of Michigan, Ann Arbor, MI 48109-2143   (734)647-3445 (tel) (734)763-0437(fax) <niciejew@umich.edu>
  • SPARC coordination 
 Olle Norberg  Swedish Institute of Space Physics, Box 812 SE-981 28 Kiruna, Sweden +46-980-79119 (tel.) +46-980-79050(fax) <Olle.Norberg@irf.se>
  •  We can supply data from the Swedish Astrid-2 satellite. Astrid-2 is in a circular 1000 km altitude, 83 degree inclination orbit, and measures E- and B-fields, electrons, ions, plasma density, and makes spin-scanning UV images.
  • I will be "scientist in charge" for Astrid-2 during September 1999. I will try to operate the satellite in a way that is optimal for the space weather campaign (i.e.,to get as large coverage as possible of all times, instead of shorter duration high-res data).
Takahiro Obara  Chief, STP section CRL, Solar Terrestrial Res. Ctr (Hiraiso), JAPAN  <T.Obara@crl.go.jp>
 Paul O'Brien 6705 Geology, UCLA, 405 Hilgard, Los Angeles, CA 90036 USA  (310) 825-2441 (tel) <tpoiii@igpp.ucla.edu>
Vladimir Odintsov  IZMIRAN, Troitsk, Moscow region, 142092, Russia  Phone: (7-095)3340293 Fax: (7-095)3340124 <vodin@izmiran.rssi.ru>
 Todd Pedersen  Air Force Research Laboratory, Ionospheric Hazards Branch (AFRL/VSBI),29 Randolph Road, Hanscom AFB, MA 01731-3010 781-377-2845 (tel.) (DSN-478) 781-377-3550 (fax) (DSN-478) <pedersen@plh.af.mil>
  •  Measurements from Thule and Qaanaaq, Greenland (central polar cap) during 9-22 Sept 1999:
  • Ionosonde electron density profiles & drifts
  • All-sky optical images at several wavelengths (subject to weather and sun/moon locations)
  • Scintillation at 250 MHz & GPS frequencies
  • GPS position errors
  • TEC.
 Xiaoqing Pi  Jet Propulsion Laboratory, M/S 138-308, 4800 Oak Grove Drive, Pasadena, CA 91109-8099  818-354-4257 (tel) 818-393-5115 (fax) <Xiaoqing.Pi@jpl.nasa.gov>

 With GPS measurements to provide

  • Near real-time (NRT) global ionospheric TEC
  • NRT global ionospheric irregularities
  • Real-time ionospheric TEC in north America
  • Support from SPARC
Risto Pirjola  Finnish Meteorological Institute/Geophysical Research Division, Vuorikatu 15 A, P.O. Box 503, FIN-00101 Helsinki, Finland +358-9-19294652 (tel) +358-9-19294603 (fax) <risto.pirjola@fmi.fi>
  • Measurements of the geomagnetically induced currents (GIC) in pipelines and transmission lines located in the Nordic Countries
  • Modeling of GIC in pipelines and in power systems
Simon P. Plunkett USRA, NASA Goddard Space Flight Center, Mail Code 682.3, Greenbelt, MD 20771 +1-301-286-2941 (tel) +1-301-286-0264 (fax) <plunkett@kreutz. nascom.nasa.gov>
  •  SOHO LASCO and EIT Coronal Imaging Observations
  • Alerts and reports on halo CMEs.
  • Comments: The SOHO spacecraft will be undergoing engineering activities for much of the second half of September. Observations should be largely unaffected. However, the dates most likely to be impacted are around 16-17 September!
 Antti Pulkkinen Finnish Meteorological Institute/Geophysical Research Division, Vuorikatu 15 A, P.O. Box 503, FIN-00101 Helsinki, Finland  +358-9-19294694 (tel) +358-9-19294603 (fax) <antti.pulkkinen@fmi.fi>
  • Measurements of the geomagnetically induced currents (GIC) in pipelines and transmission lines located in the Nordic Countries
  • Modeling of GIC in pipelines and in power systems
 Geoff Reeves Space and Atmospheric Sciences,NIS-1, Mail Stop D-466, Los Alamos National Laboratory, Los Alamos, New Mexico, 87545, USA  505-665-3877 (Phone) 505-665-7395(Fax) <reeves@lanl.gov>
  •  LANL geosynchronous satellites MPA & SOPA data
  • POLAR CEPPAD data
  • post-event analysis & modeling
Bodo W. Reinisch  University of Massachusetts Loewll, Center for Atmospheric Research, Department of Environmental, Earth and Atmospheric Sciences, 600 Suffolk Street, Lowell, MA 01854  1-978-934-4903 (tel) 1-978-459-7915 (fax) <Bodo_Reinisch@uml.edu>
  •  Groundbased ionospheric observations with Digisonde network
  • Ionospheric drift analysis for equatorial and polar regions during campaigns
Aaron J. Ridley  Southwest Research Inc.  ridley@zed.space.swri.edu
  •  Run the assimilative mapping of ionospheric electrodynamics (AMIE) technique for all of September 1999 using ground based magnetometer data collected in real time, ACE IMF and solar wind measurements, NOAA 12 and-14 estimates of hemispheric power, and DMSP measurements of cross track drift velocities. Summary results are available on line at: http://roy.space.swri.edu/amie
  • Global 5 minute maps of electric potential, conductances, Joule heating, horizontal currents, and field aligned currents will be made available soon, or by request.
  • Becuase AMIE can ingest a wide variety of data sets, and it becomes more accurate with more data sets, we are very willing to rerun the model with additional data sets. Please e-mail Aaron Ridley if you would like to include your data set in a run.
Pete Riley   10260 Campus Point Dr, MS W2M, San Diego. CA 92121  <uk2@haven.saic.com>
  •  Coronal and solar wind MHD modeling
O. C. St.Cyr   Computational Physics, Inc., MS 682, NASA-Goddard, Greenbelt, MD 20771 301-286-2575 (tel) 301-286-1617(fax) <cstcyr@cpi.com>
  •  SOHO LASCO and EIT
 Joe Salah  MIT Haystack Observatory, Route 40, Westford, MA 01886 781-981-5400 (tel) 781-981-0590(fax) <jsalah@haystack.mit.edu>
  •  ISR Observations, Millstone Hill, E-region emphasis.
 Ennio R. Sanchez  SRI International, 333 Ravenswood Ave., Menlo Park, CA 94025 <ennio.sanchez@sri.com>
  •  Incoherent scatter radar observations of high-latitude ionospheric parameters
  • Alerts and advisories support
 Rainer Schwenn    <Schwenn@linax1.mpae.gwdg.de>
  •  SRAMP Campaign coordination
Hanumant Shankar Sawan  H.S. Sawant-DAS, Instituto Nacional de Pesquisas Espacias Sci Josidos, Campos,Av.dos Astronautas, 1758 zip 12201-970 SP, Brazil

 00 55 12 345 6816/6819

(Sec. Mrs. Ivone 6794) (tel.)

00 55 12 345 6811/6810 (fax)

 <sawant@das.inpe.br>
  •  Modeling by using techniques of solar tomography.
Kristian Schlegel  Max-Planck-Institut fuer Aeronomie Max-Planck-Str. 2 D-37191 Katlenburg-Lindau,Germany  +49-5556-979-468 (tel.) +49-5556-979-240 (fax) <schlegel@linmpi.mpg.de>
  • Incoherent scatter obsevations with EISCAT and the EISCAT SValbard radar
  • Evaluation in terms of currents, fields, correlation with solar wind (SOHO) data.
 Howard Singer    <HSinger@sec.noaa.gov>
  •  SRAMP campaign coordination
 Jim Spann  NASA/MSFC, Hunstville, AL 256-544-5339 (tel) 256-544-5344(fax) <jim.spann@msfc.nasa.gov>
  • Provide Global images of the aurora in the Ultraviolet wavelenghts
  • UVI images on 10 minute resolution at http://uvisun.msfc.nasa.gov/data/ 1999/brwse.html .
  • Browse images updated as full 24 hr files become available. Currently, data through 9/6/99 is online.
  • The gif files show the raw UVI data with continental outlines overlain and an MLT plot of the data above 50 degree magnetic lattitude.
  • near-realtime images, telemetered during contacts with the spacecraft, are available at http://uvisun.msfc.nasa.gov/data/ 1999/nrt.html
 Peter Stauning  Danish Meteorological Institute, Lyngbyvej 100, DK-2100 Lyngby, Denmark +45-3915-7473 (tel) +45-3915-7460(fax) <pst@dmi.dk>
  •  Observatons:  High latitude imaging riometer data
  • Modeling: (i) dayside high-latitude field-aligned current systems (cusp & above), (ii) nightside field-aligned currents at substorm activity, (iii) energetic particle radiation and field-aligned currents at high-latitude, and small-scale disturbances
  • My investigations will primarily be concentrated to fields where geophysical observations from Greenland and precision magnetic field & high-energy particle data from the Danish Oersted satellite are of primary importance.
Nataly Stepanian Crimean Astrophysical Observatory, p. Nauchny, Crimea, 98409, Ukraine

380-655471107

380-655440704 <nataly@crao.crimea.ua>
 Takahashi Tanaka    <Tanaka@crl.go.jp>
  •  SRAMP Campaign coordination
 Jeffrey P. Thayer  SRI International, 333 Ravenswood Ave., Menlo Park, CA 94025  <thayer@sri.com>
  •  Incoherent scatter radar observations of high-latitude ionospheric parameters
 Michelle Thomsen  Los Alamos National Lab, Los Alamos, New Mexico, 87545, USA  <mthomsen@lanl.gov>
  • LANL geosynchronous satellites MPA data
  • post-event analysis & modeling
 Richard Thompson IPS Radio and Space Services, PO Box 1386, Haymarket, NSW 1240, Australia  +61-2-92138061 (fax) +61-2-92138033 (tel) <richard@ips.gov.au>
Alan W P Thomson   British Geological Survey, West Mains Road, Edinburgh EH9 3LA Scotland,UK

+44-131 650 0257 (tel.) +44-131-668-4368 (fax)

<a.thomson@bgs.ac.uk>
  • Ground-based vector magnetometers in UK (3), Ascension Island (Equatorial Atlantic), Falkan Islands (South Atlantic), Sable Island (North Atlantic)
  • Near-real-time data in UK, Sable I., Models of geomagnetic main-field, aa indices in near-real-time, magnetic index prediction, geophysical intertratation of magnetic activity for drilling operations and power companies,etc.

Happy to collaborate in any aspect! 

Tony van Eyken EISCAT Scientific Association, Box 432, N-9171 Longyearbyen, Norway <Tony.van.Eyken@eiscat.uit.no>
  •  Incoherent Scatter Radars
 Oleg Troshichev    <OlegTro@geophys.spb.su>
  •  SRAMP Campaign coordination
 Juan A. Valdivia  Code 692, NASA/Goddard Space Flight Center, Greenbelt, MD 20771  (301) 286-3545 (tel) <alejo@roselott.gsfc.nasa.gov>
  • near-real-time prediction of the spatial structure of the high latitude magnetic perturbations (HLMP) at http://lepgst.gsfc.nasa.gov/ nrt_predictions.html
  • This nonlinear model runs from ACE data, that we obtain in near-real-time, to predict the evolution of the HLMP. The evolution model is based on a mixture of phase space reconstruction and fuzzy logic pattern recognition. The ACE data has been balistically propagated to the subsolar point.
 Dimitris Vassiliadis  Goddard Space Flight Center  <vassi@lepgst.gsfc.nasa.gov>
Ari Viljanen Finnish Meteorological Institute/Geophysical Research Division, Vuorikatu 15 A, P.O. Box 503, FIN-00101 Helsinki, Finland +358-9-19294668 (tel) +358-9-19294603 (fax) <ari.viljanen@fmi.fi>
  •  Measurements of the geomagnetically induced currents (GIC) in pipelines and transmission lines located in the Nordic Countries
  • Modeling of GIC in pipelines and in power systems
 Rupa Vuthaluru Department of Physics and Mathematical Physics, University of Adelaide, Adelaide, South Australia, Australis - 5005 <rvuthalu@physics. adelaide.edu.au>
  •  Ionospheric D-region MF radar observations Empirical Modeling
 Huaning Wang Beijing Astronomical Observatory, Datun Rd. A20, Chaoyang District, Beijing 100012, China  86-10-64888716 (fax) <whn@solar48.bao.ac.cn> <zgq@public.east.cn.net>
  •  We observe vector magnetic fields on the solar photospheric surface and H_beta images everyday.
  • There were no strong solar acitivities in the solar atmosphere from September 1st to 12th.
Wenbin Wang   Space Physics Research Lab, University of Michigan, Ann Arbor, MI 48109-2143   <wenbin@umich.edu>
  •  Real time GCM modeling of the thermosphere & ionosphere
Jurgen Watermann   Solar-Terrestrial Physics Division, Danish Meteorological Institute, Lyngbyvej 100, DK-2100 Copenhagen, Denmark  <jfw@dmi.dk>
  •  Magnetic variations from the DMI Greenland chain of ground-based magnetometers
  • Data analysis and interpretation in terms of ionospheric current flow
  • participate in studies utilizing simultaneous multi-instrument data sets if they include the Greenland magnetometer data
 James A. Whalen Air Force Research Laboratory, VSBP, 29 Randolph Road, Hanscom AFB, MA 01784-3010 781-377-4766 (tel) 781-377-3550(fax) <whalen@plh.af.mil>
  •  Polar Cap Ionosphere
Phil Wilkinson   IPS Radio and Space Services, P O Box 1386, Haymarket, NSW 1240, AUSTRALIA.  +61 2 9213 8003 (tel) +61-2-9213 8060 (fax) <phil@ips.gov.au>
 Jian-Guo Wu  Solar-Terrestrial Physics Division, Danish Meteorological Institute, Lyngbyvej 100, DK-2100 Copenhage, Denmark +45-39-15-74-59 (tel) +45-39-15-74-60 (fax) <jgw@dmi.dk>
 Martin Wuest  Space Science Dept., Southwest Research Institute, POB 28510, San Antonio, TX 78228  <MWuest@swri.edu>
  •  POLAR/TIDE/TIMAS Observations
  • Would like to collaborate
Alexander N. Zaitzev  IZMIRAN, Troitsk near Moscow, 142092, RUSSIA  <zaitzev@izmiran.rssi.ru>
Ma Zhen-Guo  Datun Rd.#20A, Chaoyang District, Beijin, 100012, China 010-64877278 (tel.) 010-64888731 (fax) <mazg@159.226.63.2>
  •  Radio Telescope

Note: This list is used to construct an email group for announcementsand alerts prior to and during the campaign inerval. It is also providedto facilitate collaborations among participants. The main focus of the campaignis the post-event analysis of the data sets compiled during 15-17 Sept 99.Sign-ups are welcome before, during and after the core campaign interval.