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51. 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 ...


52. 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 ...


53. Solar Features - Solar Flares - SIDS [gov.noaa.ngdc.stp.solar.solar-features_solar-flares_sids]
A Sudden Ionospheric Disturbance (SID) is any of several radio propagation anomalies due to ionospheric changes resulting from solar or geophysical events.


54. 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 ...


55. 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 ...


56. 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 ...


57. 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 ...


58. Space Environment Modeling [gov.noaa.ngdc.stp.swx.space_environment_modeling]
Collection includes presentation materials and outputs from operational space environment models produced by the NOAA Space Weather Prediction Center (SWPC) and other related model datasets. Included ...


59. 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: ...


60. Stanford University ELF/VLF Data [STANFORD_VLF]
The Stanford VLF Group collects data from ground stations located across the globe. There are two principle types of data collected, broadband and narrowband. Broadband data is full waveform data ...


61. Sudden Impulses of Solar Wind Dynamic Pressure studied by means of SuperDARN radars [SD-Coco]
The Super Dual Auroral Radar Network (SuperDARN) has been developed in the last 10 years for the study of the high latitude ionosphere in the framework of Solar-Terrestrial ...


62. SuperDARN HF-radar Observation at Syowa Station [NIPR_UAP_HFRADAR_SYO]
SuperDARN (Super Dual Auroral Radar Network) radar observes the two-dimensional distribution of the plasma drift in the ionospheric F region in a broad area (3600 km range and 53º azimuth) by using ...


63. The SWICS/MASS/STICS (SMS) Instrument Package on WIND [WIND_SMS]
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 ...


64. The Student Nitric Oxide Explorer (SNOE) Data Archive at LASP and NSSDC [SNOE]
The Student Nitric Oxide Explorer (SNOE or "snowy") is a small scientific satellite that measured the effects of energy from the sun and from the magnetosphere on the density of nitric oxide in the ...


65. Theoretical and Empirical Models in the CEDAR Data Base at NCAR/HAO [CEDAR_MODELS]   PARENT METADATA
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 ...


66. Transient Gamma-Ray Spectrometer (TGRS) on WIND [WIND_TGRS]
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 ...


67. U.S. Geomagnetic Observatory Data [GEOMAG]
Magnetometer data from the USGS observatories are available in two forms, 'preliminary' and 'definitive'. Preliminary data are available in near-real time, but they are unprocessed, they have not ...


68. ULF induction magnetometer data from Australian Antarctic and subantarctic stations [AAS_4172]
Space weather is a significant hazard to modern technology. It results from energization of the Earth's radiation belts and subsequent transport of relativistic particles to low altitudes. Plasma ...


69. US-Total Electron Content Product (USTEC) [gov.noaa.ngdc.stp.ionosphere.G10009]
The US Total Electron Content (US-TEC) product is designed to specify TEC over the Continental US (CONUS) in near real-time. The product uses a Kalman Filter data assimilation model, described in ...


70. Ulysses Heliospheric Data [ULYSSES]
The primary mission of the Ulysses spacecraft was to characterize the heliosphere as a function of solar latitude. The periods of primary scientific interest is when Ulysses was at or higher than ...


71. Unmanned magnetometer network observation data [NIPR_UAP_LPM]
Unmanned magnetometer network observation data


72. Upper Atmosphere Data including the Fabry-Perot Interferometer, Mesosphere/Stratosphere Radar, and Ionospheric Models from NCAR [NCAR_UPA]
These data sets including model data correspond mostly to the upper atmosphere between 80 and 1000 km and is archived at the National Center for Atmospheric Research (NCAR). A detailed catalog of ...


73. Upper Atmosphere Physics Monitoring Observation at Syowa Station [NIPR_UAP_UAPM_SYO]
Upper Atmosphere Physics Monitoring Observation at Syowa Station


74. Upper Atmosphere Physics observation at Zhongshan Station [NIPR_UAP_ZHONGSHAN]
Upper Atmosphere Physics observation at Zhongshan Station


75. 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, ...


76. Upper Atmospheric and Ionospheric Data - IPST_UMD_ANTARCTIC_IONOS [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, ...


77. VETS Visualizations: Compressible Convection in an Ionizing Fluid [ucar.scd.vets.vg.ccif]
The Sun rings like a bell. By looking at the frequencies of this ringing we can tell what the bell is made of. In the case of the Sun we can tell the sound speed (temperature) ...


78. Values for the 15-minute Index of Geomagnetic Activity at High Latitude Stations (Geomagnetic Latitude 58 Degrees) [gov.noaa.ngdc.stp.indices.G00592]
The NOAA National Centers for Environmental Information (formerly National Geophysical Data Center) receives, on a monthly basis, Q indices from Sodankyla. These data are available from July 1957 ...


79. Values of Kp Indices, Ap Indices, Cp Indices, C9 Indices, Sunspot Number, and 10.7 cm Flux [gov.noaa.ngdc.stp.indices.G00191]
This data file consists of Kp indices, Ap indices, Cp indices, C9 indices, sunspot number, and 10.7 cm flux. The most often requested parameter of this file are the Kp indices. These planetary indices ...


80. Values of the Earth's Magnetic Field Components X, Y, and Z Recorded in Finland [gov.noaa.ngdc.stp.geomag.G00414]
This data set was generated by the Finish Academy of Science from magnetic data collected during the International Magnetospheric Study, 1976-1978. The data were collected by an array of digital magnetometers ...


81. Vertical Electric Field data from Concordia Station - 2009 - 2012 [ASAC_974_Concordia]
Vertical Electric field measurements captured at Concordia Station. The files are stored in XML format, and contain detailed headings describing the data layout and format. The data are collected ...


82. Vertical electric field - Vostok from 2006-2011 [ASAC_974_2]
These data are collected under a collaborative arrangement between the Australian Antarctic Division (Principal Investigator: Gary Burns) and the Russian Antarctic Expeditions (Most-recent contact: ...


83. Vertical electric field - Vostok from 2006-2011; processed 20-minute averages [AAS_974_Vostok_2006to2011_20min]
These data are collected under a collaborative arrangement between the Australian Antarctic Division (Principal Investigator: Gary Burns) and the Russian Antarctic Expeditions (Most-recent contact: ...


84. Very low frequency subionospheric communication transmitter observations [K069_2008_2009_NZ_1]
The AARDDVARK/WWLLN Very Low Frequency (VLF) Radio Sensor was installed at Arrival Heights from 10-15 December 2008 by Dr Craig J. Rodger and Dr. James Brundell as part of Antarctica New Zealand Event ...


85. Very low frequency subionospheric communication transmitter observations (WWLLN) [K060_2008_2012_NZ_1]
The AARDDVARK/WWLLN Very Low Frequency (VLF) Radio Sensor was installed at Arrival Heights from 10-15 December 2008 by Dr Craig J. Rodger and Dr. James Brundell as part of Antarctica New Zealand Event ...


86. 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 METADATA
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 ...


87. 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 ...


88. Worldwide Hourly Values of Ionospheric Characteristics: foF2, M(3000)F2, hF2,FoF1, M(3000)F1, hF, FoE, hE, foE2, hE2, foEs, fbEs, fmI, and FxI [gov.noaa.ngdc.stp.ionosonde.G00004]
The ionosphere is that part of the Earth's atmosphere that results mainly from the ionizing effect of Solar electromagnetic radiation. For poleware latitudes, the ionizing effect of incident energetic ...


89. Worldwide Instantaneous Values of Geomagnetic Components D, H, and Z or X, Y, and Z at 2.5-minute Intervals from 1964 to 1974 [gov.noaa.ngdc.stp.geomag.G00001]
This data file is comprised of instantaneous values of the geomagnetic components D, H, and Z or X, Y, and Z at 2.5-minute intervals. These values were derived from analog recordings (magnetograms) ...


90. 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 ...


91. AFI 01/08 - Imaging the plasmasphere from Antarctica - VLF Doppler (Doppler Radio Receiver) at Rothera 2001-2002 [GB-NERC-BAS-AEDC-00284]
New instrumentation was deployed in the Antarctic Peninsula region to monitor conditions occurring in the region of near-space surrounding the Earth. The opportunity was taken to link into a NASA ...


92. ALIS, Auroral Large Imaging System [SMHI_IPY_ALIS]
ALIS consists of unmanned imaging stations located in Northern Scandinavia in a grid of about 50×50 km. Each station is equipped with an imager having a high-resolution monochrome 1024×1024 pixel ...


93. Advanced Composition Explorer (ACE) CRIS Level 2 Data [ACE_LEVEL2]
The Cosmic Ray Isotope Spectrometer (CRIS) on the Advanced Composition Explorer (ACE) spacecraft is intended to be a major step in ascertaining the isotopic composition of the Galactic ...


94. Advanced Composition Explorer (ACE) Electron, Proton, and Alpha Monitor (EPAM) Level 2 Data [ACE_EPAM_LEVEL2]
The Electron, Proton, and Alpha Monitor (EPAM) is composed of five telescope apertures of three different types. Two Low Energy Foil Spectrometers (LEFS) measure the flux and direction ...


95. 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 ...


96. Advanced Composition Explorer (ACE) Particle Composition and Flux Browse Data [ACE_PARTCLE_FLUXES]
The Advanced Composition Explorer (ACE) is an Explorer mission that is being managed by the Office of Space Science Mission and Payload Development Division of the National Aeronautics ...


97. 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 ...


98. Advanced Composition Explorer (ACE) Solar Wind Electron, Proton, and Alpha Monitor (SWEPAM) Level 2 Data [ACE_SWEPAM_LEVEL2]
The Solar Wind Electron, Proton, and Alpha Monitor (SWEPAM) measures the solar wind plasma electron and ion fluxes (rates of particle flow) as functions of direction and energy. These ...


99. Advanced Composition Explorer (ACE) Solar Wind Ion Composition Spectrometer (SWICS) and Solar Wind Ion Mass Spectrometer (SWIMS) Level 2 Data [ACE_SWICS_SWIMS_LEVEL2]
The Solar Wind Ion Composition Spectrometer (SWICS) and the Solar Wind Ion Mass Spectrometer (SWIMS) on ACE are instruments optimized for measurements of the chemical and isotopic composition ...


100. Advanced Composition Explorer (ACE) Ultra Low Energy Isotope Spectrometer (ULEIS) Level 2 Data [ACE_ULEIS_LEVEL2]
The Ultra Low Energy Isotope Spectrometer (ULEIS) measures ion fluxes over the charge range from H through Ni from about 20 keV/nucleon to 10 MeV/nucleon, thus covering both suprathermal ...


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