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1. Provisional magnetic data recorded at Macquarie (MCQ) and Davis (DVS) MAGDAS (MAGnetic Data Acquisition System) stations [AAS_4020]
SERC, Kyushu University, have deployed MAGDAS magnetometers at 57 stations along the 210- and 96-degree magnetic meridians (MM) and the magnetic Dip equator, and three FM-CW radars along the 210o ...


2. Solar Geophysical Data (SGD) Reports (1955-2009) [gov.noaa.ngdc.stp.solar.solar_geophysical_data]
Solar-Geophysical Data (SGD) reports were a comprehensive compilation of many different kinds of observational data of the sun's activity and its effects on the Earth. Data from the worldwide network ...


3. GOES Space Environment Monitor, Magnetometer [gov.noaa.ngdc.sem.goes_mag_g00038]
Three orthogonal flux-gate magnetometer elements, (spinning twin fluxgate magnetometer prior to GOES-8) provide magnetic field measurements in three mutually perpendicular components: HP, HE and HN. ...


4. A Comparison of Conjugate Auroral Electojet Indices [NSF-ANT10-43621]
The 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 ...


5. Solar Magnetic Eruption Disturbances [ucar.scd.vets.vg.sme]
Solar 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 ...


6. Monitoring Magnetosphere - Ionosphere Coupling, Arrival heights, Scott Base, Antarctica [K069_1989_2012_NZ_1]
A 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 ...


7. Radio Aurora Records at Syowa Station [NICT_AURORAL_RADAR]
Radio auroral echoe observed with auroral radar at Syowa Station.


8. Search coil magnetometer data from BAS AGOs in Antarctica [JCADM_US_MAG_AGO]
Search 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 ...


9. HMO-PSWS PPM Total Magnetic Field Studies at SANAE IV, Antarctica [HMO-PSWS_PPM_SNAOVH1]
Absolute 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. ...


10. HMO-PSWS Vector Magnetic Field Studies at SANAE IV, Antarctica [HMO-PSWSS_NADSFS1]
Vector 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 ...


11. Radio and Plasma Wave Investigation (WAVES) on WIND [WIND_WAVES]
The 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 ...


12. Interplanetary Monitoring Platform (IMP-8) Magnetometer Experiment Data [IMP8_MAG]
IMP-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 ...


13. CEDAR Incoherent Scatter Radar Data Base from NCAR/HAO [INCOHERENT_SCATTER_RADAR]   PARENT DIF
The 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 ...


14. Coupling, Energetics, and Dynamics of Atmospheric Regions (CEDAR) Database at NCAR/HAO [CEDAR_NCAR_HAO]   CHILD DIFs
The 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 ...


15. Geophysical Indices from the CEDAR Data Base at NCAR/HAO [CEDAR_GEO_INDICES]   PARENT DIF
The 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, ...


16. PENGUIn - A High-Latitude Window to Geospace Dynamics [NSF-ANT08-40398]
This 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 ...


17. Collaborative Research: PENGUIn AGO Search Coil- A High-Latitude Window to Geospace Dynamics [PENGUIn_AGO_Search_Coil]
This 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 ...


18. Polar Experimantal Network for Geospace Upper-atmosphere Investigations (PENGUIn): Interhemispheric Investigations along the 40 Degree Magnetic Meridian [NSF-ANT08-39858]
'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 ...


19. Search coil Magnetometer Data from Halley, South Pole and McMurdo, Antarctica and Two Sites Conjugate to the South Pole [US_JCADM_MAG_SP]
Search 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 ...


20. Upper Atmospheric and Ionospheric Data [IPST_UMD_ANTARCTIC_IONOS]
The 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, ...


21. Upper Atmospheric and Ionospheric Data [SIENA_ANTARCTIC_IONOS]
The 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, ...


22. SAMBA magnetometer data, 2002 - present [SAMBA-data]
Ground 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. ...


23. Magnetometer data from 2001 - LPM network [GB-NERC-BAS-AEDC-00263]
The 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 ...


24. Space Physics, Solar Physics and Astronomy Data from Space Physics Data System [SPDS-General]
The 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: ...


25. UARS PEM L2 VMAG AC V001 UARPE2VMAGAC at GES DISC [GES_DISC_UARPE2VMAGAC_V001]
The Particle Environment Monitor (PEM) on NASA's Upper Atmosphere Research Satellite (UARS) measures the type, amount, energy, and distribution ...


26. UARS PEM L2 VMAG DC V001 UARPE2VMAGDC at GES DISC [GES_DISC_UARPE2VMAGDC_V001]
The Particle Environment Monitor (PEM) on NASA's Upper Atmosphere Research Satellite (UARS) measures the type, amount, energy, and distribution ...


27. UARS Particle Environment Monitor (PEM) Level 3AT V001 (UARPE3AT) at GES DISC [GES_DISC_UARPE3AT_V001]
The Particle Environment Monitor (PEM) on NASA's Upper Atmosphere Research Satellite (UARS) measures the type, amount, energy, and distribution of charged particles injected ...


28. UARS Particle Environment Monitor (PEM) Level 3TP V001 (UARPE3TP) at GES DISC [GES_DISC_UARPE3TP_V001]
The Particle Environment Monitor (PEM) on NASA's Upper Atmosphere Research Satellite (UARS) measures the type, amount, energy, and distribution of charged particles injected ...


29. Measurement of ionosphere activity from the Beacon satellite launched in 1964 [K002_1969_1970_NZ_2]
The 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 ...


30. NOAA Space Environment Laboratory On-Line Solar and Geophysical Data [SEL-01]
The 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 ...


31. Induction magnetometer data, Arrival heights, Scott Base, Antarctica [K069_1989_2008_NZ_1]
A 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 ...


32. EQUATOR-S: Earth's Equatorial Magnetosphere Data [EQUATOR-S]
EQUATOR-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 ...


33. Advanced Composition Explorer (ACE) Magnetic Field Experiment (MAG) Level 2 Data [ACE_MAG_LEVEL2]
The 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 ...


34. Advanced Composition Explorer (ACE) Real-Time Solar Wind Data from NOAA/SEC [ACE_RTSW]
Advanced 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 ...


35. South Pole Magnetometer Data [SPA-MAG]
Slow 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 ...


36. Geoscientific and Engineering Models at NASA's National Space Science Data Center (NSSDC) [ENVIRONET]
The 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 ...


37. Imager for Magnetopause-to-Aurora Global Exploration (IMAGE) Data Archive at NASA/NSSDC and SWRI [IMAGE]
The 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 ...


38. Polar Sun-Earth Connection Mission Data Archive at NASA/GSFC [NASA_POLAR]
The 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 ...


39. Wilcox Solar Observatory Solar Data and Solar Magnetic Field Atlas [WILCOX_SOLAR_ATLAS]
The 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 ...


40. Digisonde Portable Sounder 4 Data at Zhongshan Station, Antarctica, Year 2000 [CNNADC_S2000_S_DPS4_ZS]
The 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, ...


41. Theoretical and Empirical Models in the CEDAR Data Base at NCAR/HAO [CEDAR_MODELS]   PARENT DIF
The 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 ...


42. Aeromagnetic Survey of Dillingham Area in Southwest Alaska, A Website for the Preliminary Distribution of Data [USGS_OFR_2006_1136]
This 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 ...


43. Fast Auroral SnapshoT Explorer (FAST) Data Archive [FAST]
The 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 ...


44. Ionospheric vertical sounding [Ionospheric_vertical_sounding]
Ionospheric 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 ...


45. Magnetic Field Investigation (MFI) on WIND [WIND_MFI]
The 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 ...


46. Solar Wind Experiment (SWE) on WIND [WIND_SWE]
The 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 ...


47. Vulcanism, Seismicity, Magnetism and Geodynamics of the South Shetland Island: Magnetic station at Spanish Antarctic station (Livingston); Geomagnetic and Ionospheric studies. [CNDA-ESP_ANT95-0094-CO3]   PARENT DIF
In 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 ...


48. CLUSTER-II Solar-Terrestrial Data [CLUSTER-II]
Cluster 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 ...


49. Combined Release and Radiation Effects Satellite Data at NASA/NSSDC [CRRES]
The 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 ...


50. Geotail Data Archive at NASA/GSFC [NASA_GEOTAIL]
The 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 ...


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