Global Change Master Directorygsfc-gcmduso@mail.nasa.gov502013-05-23T08:37:11ZGCMD Search: [Parameters: Topic='SUN-EARTH INTERACTIONS', Term='IONOSPHERE/MAGNETOSPHERE DYNAMICS', Variable_Level_1='MAGNETIC FIELDS/MAGNETIC CURRENTS']http://mddemo.gsfc.nasa.gov/KeywordSearch/OpenSearch.do 52 0 http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]NSF-ANT10-43621A Comparison of Conjugate Auroral Electojet Indices-180.0,-79.5,180.0,-54.52011-06-01T00:00:00Z2013-05-31T00:00:00Z2013-04-18T04:00:00ZThe auroral electrojet index (AE) is used as an indicator of geomagnetic activity at high latitudes representing the strength of auroral electrojet currents in the Northern polar ionosphere. A similar ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]ucar.scd.vets.vg.smeSolar Magnetic Eruption Disturbances2012-07-10T04:00:00ZSolar Magnetic Eruptions (SME), such as Coronal Mass Ejections and Solar
Flares, and their impact on Earth's space environment are the target of this
Space Weather research.Solar Magnetic Eruptions ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]K069_1989_2012_NZ_1Monitoring Magnetosphere - Ionosphere Coupling, Arrival heights, Scott Base, Antarctica166.7625,-77.9175,166.7625,-77.91751990-01-01T00:00:00ZT00:00:00Z2012-06-15T04:00:00ZA magnetometer and data recording system was installed and began recording hydromagnetic and ion cyclotron waves (geomagnetic pulsations) propagating into the high latitude cusp and polar cap regions ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]NICT_AURORAL_RADARRadio Aurora Records at Syowa Station40.0,-69.0,40.0,-69.01966-03-13T00:00:00ZT00:00:00Z2012-04-16T04:00:00ZRadio auroral echoe observed with auroral radar at Syowa Station.http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]JCADM_US_MAG_AGOSearch coil magnetometer data from BAS AGOs in Antarctica-20.4,-80.7,-20.4,-80.73.0,-81.5,3.0,-81.5-23.9,-84.4,-23.9,-84.41997-01-01T00:00:00Z2003-12-07T00:00:00Z1996-01-01T00:00:00Z2003-12-07T00:00:00Z1999-01-01T00:00:00Z2003-12-07T00:00:00Z2011-07-28T04:00:00ZSearch coil magnetometer data are primarily used to study waves and
transient variations in Earth's magnetic field in the ULF
(Ultra-Low-Frequency) range, from ~0.001 Hz to ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]HMO-PSWS_PPM_SNAOVH1HMO-PSWS PPM Total Magnetic Field Studies at SANAE IV, Antarctica-2.83058,-71.67443,-2.83058,-71.674432008-01-08T00:00:00ZT00:00:00Z2011-07-22T04:00:00ZAbsolute magnetic field studies at SANAE IV, Antarctica, are conducted with a GSM-19W high sensitivity proton magnetometer sensor, using the Overhauser effect to detect the absolute magnetic field. ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]HMO-PSWSS_NADSFS1HMO-PSWS Vector Magnetic Field Studies at SANAE IV, Antarctica-2.82993,-71.67464,-2.82993,-71.674642008-01-17T00:00:00ZT00:00:00Z2011-07-22T04:00:00ZVector magnetic field studies at SANAE IV, Antarctica, are conducted with a FGE suspended magnetometer, manufactured by the Danish Meteorological Institute. It is a In Situ land based application ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]WIND_WAVESRadio and Plasma Wave Investigation (WAVES) on WIND1994-11-01T00:00:00ZT00:00:00Z2011-03-11T05:00:00ZThe main purpose of the Wind spacecraft is to measure the incoming
solar wind, magnetic fields and particles, although early on it will
also observe the Earth's foreshock region. Wind, together with ...http://gcmd.gsfc.nasa.gov/getdif.htm?[NOAA-NMMR]gov.noaa.ngdc.G00582Satellite Environment-180.0,-90.0,180.0,90.01967-01-01T00:00:00ZT00:00:00Z2011-03-02T05:00:00ZABSTRACT: Satellites monitor in situ the effect of the Sun on the near-Earth environment. The GOES and SOLRAD satellites orbited at geostationary levels, about 22,000 miles above the Earth's surface. ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]IMP8_MAGInterplanetary Monitoring Platform (IMP-8) Magnetometer Experiment Data1973-10-30T00:00:00ZT00:00:00Z2011-03-01T05:00:00ZIMP-8 (IMP-J) was launched by NASA on October 26, 1973 to measure the
magnetic fields, plasmas, and energetic charged particles (e.g.,
cosmic rays) of the Earth's magnetotail and ...http://gcmd.gsfc.nasa.gov/getdif.htm?[NOAA-NMMR]gov.noaa.ngdc.G00038GOES Space Environment Monitor, Magnetometer-180.0,-90.0,180.0,90.01974-07-01T00:00:00ZT00:00:00Z2011-02-28T05:00:00ZABSTRACT: Three orthogonal flux-gate magnetometer elements, (spinning twin fluxgate magnetometer prior to GOES-8) provide magnetic field measurements in three mutually perpendicular components: HP, ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]INCOHERENT_SCATTER_RADARCEDAR Incoherent Scatter Radar Data Base from NCAR/HAO-76.0,-12.0,-76.0,-11.0-67.0,18.0,-66.0,19.0137.0,34.0,136.0,35.0-72.0,42.0,-71.0,43.00.0,44.0,3.0,48.0-148.0,65.0,-147.0,66.020.0,67.0,21.0,68.0-27.0,67.0,-26.0,68.0-51.0,67.0,-51.0,67.01966-01-01T00:00:00ZT00:00:00Z2011-01-31T05:00:00ZThe Coupling, Energetics, and Dynamics of Atmospheric Regions (CEDAR)
at the National Center for Atmospheric Research/High Altitude
Observatory (NCAR/HAO) incoherent-radar data base was established ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]CEDAR_NCAR_HAOCoupling, Energetics, and Dynamics of Atmospheric Regions (CEDAR) Database at NCAR/HAO-180.0,-90.0,180.0,90.01966-01-01T00:00:00ZT00:00:00Z2010-09-22T04:00:00ZThe Coupling, Energetics, and Dynamics of Atmospheric regions (CEDAR) is a
program sponsored by the National Science Foundation (NSF) designed to enhance
the capability of ground-based instruments ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]CEDAR_GEO_INDICESGeophysical Indices from the CEDAR Data Base at NCAR/HAO-180.0,-90.0,180.0,90.01966-01-01T00:00:00ZT00:00:00Z2010-09-22T04:00:00ZThe Coupling, Energetics, and Dynamics of Atmospheric Regions (CEDAR)
Data Base has some files of geophysical indices. These include Dst,
Kp, ap, AP, solar 10.7 cm flux, sunspot number, AE indices, ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]NSF-ANT08-40398PENGUIn - A High-Latitude Window to Geospace Dynamics-180.0,-90.0,180.0,-75.02009-09-01T00:00:00Z2011-08-31T00:00:00Z2010-08-12T04:00:00ZThis award is funded under the American Recovery and Reinvestment Act of 2009 (Public Law 111-5). The PENGUIn team will continue investigating in depth a multi-scale electrodynamic system that comprises ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]PENGUIn_AGO_Search_CoilCollaborative Research: PENGUIn AGO Search Coil- A High-Latitude Window to Geospace Dynamics 129.61,-83.86,129.61,-83.86-46.38,-85.67,-46.38,-85.6728.59,-82.75,28.59,-82.7596.76,-82.01,96.76,-82.01123.52,-77.24,123.52,-77.24130.03,-69.51,130.03,-69.511994-01-11T00:00:00ZT00:00:00Z1993-12-22T00:00:00ZT00:00:00Z1995-01-26T00:00:00ZT00:00:00Z1994-01-27T00:00:00Z2001-01-21T00:00:00Z1996-01-17T00:00:00ZT00:00:00Z1997-05-15T00:00:00Z2001-11-15T00:00:00Z2010-08-10T04:00:00ZThis award is funded under the American Recovery and Reinvestment Act of 2009 (Public Law 111-5).
The PENGUIn team will continue investigating in depth a multi-scale electrodynamic system that comprises ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]NSF-ANT08-39858Polar Experimantal Network for Geospace Upper-atmosphere Investigations (PENGUIn): Interhemispheric Investigations along the 40 Degree Magnetic Meridian-1.0,-85.0,103.0,-77.02009-09-01T00:00:00Z2013-08-31T00:00:00Z2010-07-29T04:00:00Z'This award is funded under the American Recovery and Reinvestment Act of 2009 (Public Law 111-5).' The solar wind - magnetosphere - ionosphere system and the space weather phenomena it controls ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]US_JCADM_MAG_SPSearch coil Magnetometer Data from Halley, South Pole and McMurdo, Antarctica and Two Sites Conjugate to the South Pole-16.3,-75.6,-16.3,-75.6-180.0,-90.0,-180.0,-90.0166.7,-77.9,166.7,-77.9-50.7,67.0,-50.7,67.0-68.6,63.8,-68.6,63.82005-01-01T00:00:00ZT00:00:00Z1982-01-01T00:00:00ZT00:00:00Z1985-01-01T00:00:00ZT00:00:00Z1984-01-01T00:00:00ZT00:00:00Z1993-01-01T00:00:00ZT00:00:00Z2010-07-28T04:00:00ZSearch coil magnetometer data are primarily used to study waves and transient variations in Earth's magnetic field in the ULF (Ultra-Low-Frequency) range, from ~0.001 Hz to 5 Hz. Naturally-observed ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]IPST_UMD_ANTARCTIC_IONOSUpper Atmospheric and Ionospheric Data-0.0,-90.0,-0.0,-90.0166.67,-77.85,166.67,-77.851986-01-01T00:00:00Z2001-01-01T00:00:00Z2010-07-07T04:00:00ZThe projects that operate from instrumentation at South Pole Station,
and at the Arrival Heights Laboratory at McMurdo Station, examine
natural phenomena occurring in the earth's atmosphere, ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]SIENA_ANTARCTIC_IONOSUpper Atmospheric and Ionospheric Data-0.0,-90.0,-0.0,-90.0166.67,-77.85,166.67,-77.851986-01-01T00:00:00Z2001-01-01T00:00:00Z2010-07-07T04:00:00ZThe projects that operate from instrumentation at South Pole Station,
and at the Arrival Heights Laboratory at McMurdo Station, examine
natural phenomena occurring in the earth's atmosphere, ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]SAMBA-dataSAMBA magnetometer data, 2002 - present2002-04-01T00:00:00ZT00:00:00Z2010-07-02T04:00:00ZGround magnetometer data from the 12 stations of the South American Meridional B-field Array (SAMBA) covering magnetic latitudes from near equatorial to mid-latitudes and with one auroral
station. ...http://gcmd.gsfc.nasa.gov/getdif.htm?[BAS_AEDC]GB-NERC-BAS-AEDC-00263Magnetometer data from 2001 - LPM network-68.1167,-88.025,95.9756,-64.81672001-12-01T00:00:00ZT00:00:00Z2010-04-27T04:00:00ZThe British Antarctic Survey holds magnetic data measuring the plasmaspheric mass loading on magnetic field lines in Antarctica. The network of Low Power Magnetometer instruments consists of permanent ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]SPDS-GeneralSpace Physics, Solar Physics and Astronomy Data from Space Physics Data System-180.0,-90.0,180.0,90.02009-08-28T04:00:00ZThe Space Physics Data System (SPDS) ( http://spdf.gsfc.nasa.gov/ )
serves the four science disciplines encompassed within the programs
of the NASA Space Physics Division, namely: ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]GES_DISC_UARPE2VMAGAC_V001UARS PEM L2 VMAG AC V001 UARPE2VMAGAC at GES DISC-180.0,-57.15,180.0,57.151991-09-26T00:00:00Z2005-08-23T00:00:00Z2009-08-21T04:00:00ZThe Particle Environment Monitor (PEM) on NASA's Upper Atmosphere
Research Satellite (UARS) measures the type, amount, energy, and
distribution ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]GES_DISC_UARPE2VMAGDC_V001UARS PEM L2 VMAG DC V001 UARPE2VMAGDC at GES DISC-180.0,-57.15,180.0,57.151991-09-15T00:00:00Z2005-08-23T00:00:00Z2009-08-21T04:00:00ZThe Particle Environment Monitor (PEM) on NASA's Upper Atmosphere
Research Satellite (UARS) measures the type, amount, energy, and
distribution ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]GES_DISC_UARPE3AT_V001UARS Particle Environment Monitor (PEM) Level 3AT V001 (UARPE3AT) at GES DISC-180.0,-80.0,180.0,80.01991-10-01T00:00:00ZT00:00:00Z2009-08-21T04:00:00ZThe Particle Environment Monitor (PEM) on NASA's Upper Atmosphere
Research Satellite (UARS) measures the type, amount, energy, and
distribution of charged particles injected ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]GES_DISC_UARPE3TP_V001UARS Particle Environment Monitor (PEM) Level 3TP V001 (UARPE3TP) at GES DISC-180.0,-80.0,180.0,80.01991-10-01T00:00:00ZT00:00:00Z2009-08-21T04:00:00ZThe Particle Environment Monitor (PEM) on NASA's Upper Atmosphere
Research Satellite (UARS) measures the type, amount, energy, and
distribution of charged particles injected ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]K002_1969_1970_NZ_2Measurement of ionosphere activity from the Beacon satellite launched in 1964166.75,-77.85,166.75,-77.852009-06-30T04:00:00ZThe Polar Ionosphere Beacon Satellite Program, S-66, was for the purpose of ionospheric research. The S-66 program aimed to make possible a synoptic study of the ionosphere as it varies in time and ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]SEL-01NOAA Space Environment Laboratory On-Line Solar and Geophysical Data-180.0,-90.0,180.0,90.01990-01-01T00:00:00ZT00:00:00Z2009-06-11T04:00:00ZThe NOAA Space Environment Laboratory collects, evaluates, and
distributes data relating to space plasma events, solar activity,
and cosmic ray particle activity on a nearly real-time basis.
Space ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]K069_1989_2008_NZ_1Induction magnetometer data, Arrival heights, Scott Base, Antarctica 166.7625,-77.9175,166.7625,-77.91751990-01-01T00:00:00ZT00:00:00Z2009-05-11T04:00:00ZA magnetometer and data recording system was installed and began recording hydromagnetic and ion cyclotron waves (geomagnetic pulsations) propagating into the high latitude cusp and polar cap regions ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]EQUATOR-SEQUATOR-S: Earth's Equatorial Magnetosphere Data1997-12-02T00:00:00ZT00:00:00Z2009-04-14T04:00:00ZEQUATOR-S is a low-cost mission designed to study the Earth's equatorial
magnetosphere out to distances of 67000 km and it forms an element of the
closely-coordinated ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]ACE_MAG_LEVEL2Advanced Composition Explorer (ACE) Magnetic Field Experiment (MAG) Level 2 Data1997-08-25T00:00:00ZT00:00:00Z2009-03-30T04:00:00ZThe Magnetic Field Experiment (MAG) consists of twin vector fluxgate
magnetometers controlled by a common CPU. The sensors are mounted on
booms extending 4.19 meters from the center of ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]ACE_RTSWAdvanced Composition Explorer (ACE) Real-Time Solar Wind Data from NOAA/SEC1997-08-25T00:00:00ZT00:00:00Z2009-03-30T04:00:00ZAdvanced Composition Explorer (ACE) Real-Time Solar Wind (RTSW) Data from
NOAA's Space Environment Center (SEC) provides up to an hour's advance warning
of unusual solar activity, such ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]SPA-MAGSouth Pole Magnetometer Data1980-01-01T00:00:00Z2008-09-26T00:00:00Z2008-10-01T04:00:00ZSlow variations of the terrestrial magnetic field are measured with the fluxgate magnetometer (DC to the Nyquist frequency of 0.5 Hz, at 1-Hz sampling rate); the sensor itself comprises three small ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]ENVIRONETGeoscientific and Engineering Models at NASA's National Space Science Data Center (NSSDC)-180.0,-90.0,180.0,90.02008-05-29T04:00:00ZThe National Space Science Data Center (NSSDC) at NASA/Goddard
Space Flight Center has many space physics and space weather
models available on:
- Gavitation and Geopotential Models
- Atmospheric ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]IMAGEImager for Magnetopause-to-Aurora Global Exploration (IMAGE) Data Archive at NASA/NSSDC and SWRI2000-03-25T00:00:00ZT00:00:00Z2008-05-27T04:00:00ZThe Imager for Magnetosphere-to-Aurora Global Exploration (IMAGE)
mission produced the first comprehensive global images of the plasma
populations in the inner magnetosphere.
IMAGE data are archived ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]NASA_POLARPolar Sun-Earth Connection Mission Data Archive at NASA/GSFC1996-02-24T00:00:00ZT00:00:00Z2008-05-09T04:00:00ZThe Polar spacecraft was launched on February 24, 1996, to obtain data from
both high- and low-altitude perspectives of this active region of geospace.
High above the poles the particles of the solar ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]WILCOX_SOLAR_ATLASWilcox Solar Observatory Solar Data and Solar Magnetic Field Atlas1985-03-01T00:00:00ZT00:00:00Z2008-04-25T04:00:00ZThe Wilcox Solar Observatory began daily observations of the Sun's
global magnetic field in May 1975, with the goal of understanding
changes in the Sun and how those changes affect the Earth; this ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]CNNADC_S2000_S_DPS4_ZSDigisonde Portable Sounder 4 Data at Zhongshan Station, Antarctica, Year 200076.6,-69.6,76.6,-69.62001-03-05T00:00:00Z2002-01-01T00:00:00Z2007-08-21T04:00:00ZThe DPS-4, developed by the University of Masachusetts at Lowell Center for Atmospheric Research (ULCAR), is a pulse HF Doppler radar controlled by a computer. It can measure the amplitude, phase, ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]CEDAR_MODELSTheoretical and Empirical Models in the CEDAR Data Base at NCAR/HAO-180.0,-90.0,180.0,90.02006-10-13T04:00:00ZThe Coupling, Energetics, and Dynamics of Atmospheric Regions (CEDAR)
Data Base at NCAR/HAO holds information on theoretical models and
source code for several empirical models.
Theoretical models ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]USGS_OFR_2006_1136Aeromagnetic Survey of Dillingham Area in Southwest Alaska, A Website for the Preliminary Distribution of Data-159.19,58.3,-155.45,60.062005-09-01T00:00:00Z2005-10-22T00:00:00Z2006-06-15T04:00:00ZThis is a USGS Open-File-Report for the preliminary release of aeromagnetic
data collected in the Dillingham Area of Southwest Alaska and associated
contractor reports.
An airborne high-resolution ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]FASTFast Auroral SnapshoT Explorer (FAST) Data Archive1996-08-21T00:00:00ZT00:00:00Z2005-10-31T05:00:00ZThe Fast Auroral SnapshoT (FAST), the second mission in NASA's Small Explorer
Satellite Program (SMEX), is a satellite designed to study Earth's aurora. This
highly successful spacecraft has helped ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]Ionospheric_vertical_soundingIonospheric vertical sounding164.1,-74.7,164.1,-74.71993-11-01T00:00:00Z2002-01-01T00:00:00Z2005-08-01T04:00:00ZIonospheric observations, using radio techniques, are an important part of the
aeronomic studies that may be carried out in polar zones where the peculiarity
of the physical phenomena, due to the ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]WIND_MFIMagnetic Field Investigation (MFI) on WIND1994-11-01T00:00:00ZT00:00:00Z2005-08-01T04:00:00ZThe main purpose of the Wind spacecraft is to measure the incoming
solar wind, magnetic fields and particles, although early on it will
also observe the Earth's foreshock region. Wind, together with ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]WIND_SWESolar Wind Experiment (SWE) on WIND1994-11-01T00:00:00ZT00:00:00Z2005-08-01T04:00:00ZThe main purpose of the Wind spacecraft is to measure the incoming
solar wind, magnetic fields and particles, although early on it will
also observe the Earth's foreshock region. Wind, together with ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]CNDA-ESP_ANT95-0094-CO3Vulcanism, Seismicity, Magnetism and Geodynamics of the South Shetland Island: Magnetic station at Spanish Antarctic station (Livingston); Geomagnetic and Ionospheric studies.-61.0,-63.0,-61.0,-63.01996-01-01T00:00:00ZT00:00:00Z2005-08-01T04:00:00ZIn English:
The main scientific objectives of the campaign were:
To create a data base indispensable to the reduction of geomagnetic surveys. To
determine the geologic structures these surveys require ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]CLUSTER-IICLUSTER-II Solar-Terrestrial Data2000-07-16T00:00:00ZT00:00:00Z2005-07-29T04:00:00ZCluster II is part of an international collaboration to investigate the
physical connection between the Sun and Earth. Flying in a tetrahedral
(triangular pyramid) formation, the four spacecraft collect ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]CRRESCombined Release and Radiation Effects Satellite Data at NASA/NSSDC1990-07-25T00:00:00Z1991-10-12T00:00:00Z2005-07-29T04:00:00ZThe Combined Release and Radiation Effects Satellite (CRRES) was launched into
a geosynchronous transfer orbit (GTO) for a nominal three-year mission to
investigate fields, plasmas, and energetic ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]NASA_GEOTAILGeotail Data Archive at NASA/GSFC1992-07-24T00:00:00ZT00:00:00Z2005-07-29T04:00:00ZThe GEOTAIL mission is a collaborative project undertaken by the Institute of
Space and Astronautical Science (ISAS) and the National Aeronautics and Space
Administration (NASA). Its primary objective ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]IMP8_MITInterplanetary Monitoring Platform (IMP-8) Solar Plasma Faraday Cup Data1973-10-30T00:00:00ZT00:00:00Z2005-07-29T04:00:00ZIMP-8 (IMP-J) was launched by NASA on October 26, 1973 to measure the
magnetic fields, plasmas, and energetic charged particles (e.g.,
cosmic rays) of the Earth's magnetotail and magnetosheath and ...