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51. 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 ...


52. 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, ...


53. 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, ...


54. Ottawa/Penticton 2800 MHz Solar Radio Flux [FE00216]
Solar radio flux is measured from the undisturbed solar surface, developing active regions on the sun and from short-lived enhancements above the daily level. Radio ...


55. ELF/VLF Observations of Lightning Discharges, Whistler-mode waves and Electron Precipitation at Palmer Station, Antarctica [NSF-ANT05-38627]
This proposal is focused on experimental studies of the thunderstorms electrodynamic coupling to the Earth's radiation belts through the upward lightning flashes that lead to ionospheric parameters ...


56. 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: ...


57. Interplanetary Monitoring Platform (IMP-8) Energetic Particle Experiment (EPE) Data [IMP8_JHUEPE]
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 magnetosheath and ...


58. Interplanetary Monitoring Platform (IMP-8) Solar Plasma Electrostatic Analyzer Data [IMP8_LANL]
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 ...


59. UARS SOLSTICE Level 3BS Solar UV Irradiance Spectra V001 (UARSO3BS) at GES DISC [GES_DISC_UARSO3BS_V001]
The Solar-Stellar Irradiance Comparison Experiment (SOLSTICE) on NASA's Upper Atmosphere Research Satellite (UARS) measured the energy input to the upper atmosphere by observing ...


60. UARS SUSIM Level 3BS Solar UV Irradiance Spectra V001 (UARSU3BS) at GES DISC [GES_DISC_UARSU3BS_V001]
The SUSIM home page on the WWW is http://www.nrl.navy.mil/content.php?P=SUSIM . The Solar Ultraviolet Spectral Irradiance Monitor (SUSIM) on NASA's ...


61. NASA STEREO (Solar TErrestrial RElations Observatory) Data Products [NASA_STEREO_DATA_PLACEHOLDER]
[Source: NASA/GSFC Solar TErrestrial RElations Observatory (STEREO) home page, http://stereo.gsfc.nasa.gov/ ] STEREO (Solar ...


62. Microbially Mediated Alteration of Volcanic Glass using McMurdo Extreme Environments as Natural Laboratories [NSF-ANT07-39712]
This project studies the microbial processes that alter volcanic glass, which is critical to understanding the earliest life on earth. To understand the environmental controls on these processes, ...


63. 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 ...


64. 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 ...


65. 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 ...


66. 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 ...


67. 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 ...


68. 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 ...


69. Advanced Composition Explorer (ACE) Solar Energetic Particle Charge Analyser (SEPICA) Level 2 Data [ACE_SEPICA_LEVEL2]
The Solar Energetic Particle Charge Analyser (SEPICA) is used to determine the charge state distribution of energetic particle distributions. ...


70. 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 ...


71. 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 ...


72. 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 ...


73. Solar Ground-Based Data from the Base de donnees Solaire Sol (BASS) 2000 Project [SOLAR_BASS2000]
BASS 2000 has been initiated by the Institut National des Sciences de l'Univers together with the Midi-Pyrenees Observatory, the research group "solar and stellar magnetodynamic", the ...


74. SOHO/Solar Ultraviolet Measurements of Emitted Radiation (SUMER) Data Archive [SOHO_SUMER]
The Solar Ultraviolet Measurements of Emitted Radiation (SUMER) is a UV telescope and spectrometer that was designed and built at the Max-Planck-Institut fur Aeronomie (MPAe) with international ...


75. 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) ...


76. Pumping of Magnetic Fields by PTCC [ucar.scd.vets.vg.pumping]
This research explores the transport of magnetic fields on the Solar surface by Penetrative Turbulent Compressible Convection (PTCC).This research attempts to better understand the process ...


77. Solar Magnetic Flux Tubes [ucar.scd.vets.vg.mft]
Solar Magnetic Flux Tubes are magnetic field concentrations near the surface of the sun. Because of their close relation to their much larger cousins, sun spots, they are of great interest ...


78. 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 ...


79. Interplanetary Monitoring Platform (IMP-8) Electrostatic Energy-Charge Analyzer (EECA) Data [IMP8_UMD]
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 magnetosheath ...


80. SOHO/Comprehensive Suprathermal and Energetic Particle Analyzer (COSTEP) Data Archive [SOHO_COSTEP]
COSTEP addresses scientific objectives related to the following phenomena: * Steady state processes in the solar atmosphere * Energy release and particle acceleration in the solar atmosphere ...


81. General Access to GRO/BATSE Solar Database Maintained at NASA/GSFC [GRO_BATSE_SOLAR_DB]
For the use of the solar physics and astronomy communities, a system that is available on-line for quick-look access to the solar flare data from the Gamma-Ray Observatory (GRO) has been established. ...


82. MAGSAT Magnetic Field Data, Anomaly Plots, Plus Analysis Software at NSSDC [MAGSAT-GEN]
The Magsat project was a joint NASA/USGS effort to measure near-earth magnetic fields on a global basis. Objectives included obtaining an accurate description of the earth's magnetic field, obtaining ...


83. 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 ...


84. 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 ...


85. RHESSI Solar Flare Data: Light Curves, Spectra, and Images [RHESSI]
The primary mission of the Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI) is to explore the basic physics of particle acceleration and energy release in solar flares. RHESSI consists ...


86. SOHO/Charge, Element, and Isotope Analysis System (CELIAS) Data Archive [SOHO_CELIAS]
The CELIAS instrument is designed to study the composition of the solar wind (SW) and of solar and interplanetary energetic particles on SOHO. SOHO is a project of international cooperation between ...


87. SOHO/Michelson Doppler Imager (MDI) and Solar Oscillations Investigation (SOI) Data Archive [SOHO_MDI_SOI]
MDI is a project of the Stanford-Lockheed Institute for Space Research and is a joint effort of the Solar Oscillations Investigation (SOI) in the W.W. Hansen Experimental Physics Laboratory of Stanford ...


88. SOHO/Solar Wind Anisotropies (SWAN) Data Archive [SOHO_SWAN]
The SWAN (Solar Wind ANisotropies) instrument is one of twelve instruments onboard SOHO (SOlar Heliospheric Observatory) satellite. It is a collaboration between Finnish Meteorological Institute and ...


89. SOHO/Energetic and Relativistic Nuclei and Electron (ERNE) Data Archive [SOHO_ERNE]
The Energetic and Relativistic Nuclei and Electron (ERNE) Sensor Unit (ESU) has two energetic particle sensors: LED and HED. ERNE will investigate the solar atmosphere by detecting charged particles ...


90. SOHO/Global Oscillations at Low Frequencies (GOLF) Data Archive [SOHO_GOLF]
The GOLF experiment on the SOHO mission aims to study the internal structure of the sun by measuring the spectrum of global oscillations in the frequency range 10**-7 to 10**-2 Hz. Both p and g mode ...


91. SOHO/Large Angle and Spectrometric Coronagraph Experiment (LASCO) Data Archive [SOHO_LASCO]
The Large Angle and Spectrometric COronagraph (LASCO) instrument is one of 11 instruments included on the joint NASA/ESA SOHO (Solar and Heliospheric Observatory) spacecraft. The LASCO instrument ...


92. SOHO/UltraViolet Coronograph Spectrometer (UVCS) Data Archive [SOHO_UVCS]
The purpose of the UltraViolet Coronograph Spectrometer (UVCS) on the Solar and Heliospheric Observatory (SOHO) is to provide a detailed description of the extended solar corona that can be used to ...


93. 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 ...


94. Solar Chromospheric Variability from the National Solar Observatory (NSO) [NSO_CA2]
Observations of the disk-integrated solar Ca II K-line are made using the Evans Coronal Facility at The National Solar Observatory/ Sacramento Peak. A coelostat is used to feed the horizontal Littrow ...


95. Solar Ultraviolet Observations from the Solar Maximum Mission/ Ultraviolet Spectrometer and Polarimeter (SMM/UVSP) [SMM-06]
Data from the Ultraviolet Spectrometer and Polarimeter (UVSP) consist of photon counts at selected UV wavelengths in the 1170 - 3500 A band from detectors which are used in a variety of modes to build ...


96. Solar Global Oscillation Network Group (GONG) [GONG]
The Global Oscillation Network Group ( GONG ) is a community-based project to conduct a detailed study of solar internal structure and dynamics using helioseismology. In order to exploit this new ...


97. Images in H-alpha, 80, 160, and 327 MHz, and dynamic spectrograph data from Culgoora Observatory, Australia [CULGOORA]
The Culgoora Solar Observatory is located 25 km west of the town of Narrabri, in north-west New South Wales. The observatory conducts continuous optical and radio observations of the sun every day ...


98. Active Region UV Atlas [HRTS-II_ATLAS]
An ultraviolet spectral Atlas of a sunspot with high spectral and spatial resolution in the wavelength region 1190 - 1730 A is presented. The sunspot was observed with the High Resolution Telescope ...


99. On-line Solar Imaging Data Available from Big Bear Observatory [BBSO_ON_LINE]
Daily Big Bear Solar Observatory (BBSO) images are available from http://www.bbso.njit.edu/. Data available include: High-resolution H-alpha filtergram (usually center line) Dopplergram (usually ...


100. Server of Early Ground Magnetometer Data [BRUNET_GROUND]
Magnetic data from chains of ground stations are currently available at UCLA for 1977 through 1987. They are available at one minute resolution in either HDZ or XYZ coordinates. Data from the following ...


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