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1. Hourly scaled ionospheric characteristics for Macquarie Island, Mawson and Casey. [IPS_IONOSONDE]
Routine high latitude observations made in Antarctica form a climatological baseline of the ionosphere extending back to 1958 at Mawson and Casey, and for almost two decades at Davis and Macquarie ...


2. Cosmic Ray Observations in McMurdo [NSF-ANT07-39620]
This proposal seeks funding to continue the neutron monitor observations at McMurdo for at least 4 years of operation - through the next solar activity maximum predicted in 2011-12. The neutron monitor ...


3. 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 ...


4. Ionospheric Vertical Sounding [NICT_IONOSONDE_OBS]
Virtual height profile of ionospheric electron density at Syowa Station, East Antarctica


5. NASA Solar Dynamics Observatory (SDO) Science Data Products [SDO_DIF_PLACEHOLDER]
[Text Source: The Solar Dynamics Observatory (SDO) Project Home page, http://sdo.gsfc.nasa.gov/mission/about.php ] SDO: The Solar Dynamics Observatory is the first ...


6. Investigations of Space Weather and the Mesosphere using the TIGER Radar [ASAC_1246]
The Tasman International Geospace Environment Radar (TIGER) is an over-the-horizon radar that locates ionospheric structures in the region between Tasmania and Antarctica, measuring their velocities. ...


7. Observatory Operations - Riometer and Magnetometer Data from the Australian Antarctic Territory and Riometer Data from Macquarie Island [ASAC_527]
An analogue data acquisition system (ADAS), designed to collect time-stamped, time series data from any analogue signal is currently used to log data from the riometer, magnetic pulsations and fluxgate ...


8. Energetic Particles: Acceleration, Composition and Transport (EPACT) Investigation on WIND [WIND_EPACT]
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 ...


9. Measurement of Cosmic Ray Response Functions for an Ice Cherenkov Detector [NSF-ANT08-38838]
We determined a set of cosmic ray response functions for the ice Cherenkov detector used by the surface air shower IceTop, part of the IceCube Neutrino Observatory at the South Pole. At the same time ...


10. NOAA CLASS archive: Continuously Operating Reference Stations (CORS) [gov.noaa.class.CORS]
ABSTRACT: The National Geodetic Survey (NGS), an office of NOAA's National Ocean Service (NOS), coordinates a network of geodetic-quality CORS stations that provide Global Positioning System (GPS) ...


11. HMO-PSWS GPS Ionospheric Scintillation and Total Electron Content Monitoring on Marion Island, Gough Island, and at SANAE IV, Antarctica [HMO-PSWS_GISTM_MAR_GOG_SNA]
Ionospheric Scintillation observations at GPS (L-band) frequencies, as measured with the Novatel GSV4004B GPS Ionospheric and Total Electron Content Monitor (GISTM). The data format is proprietary ...


12. Ionospheric Digital Database [gov.noaa.ngdc.G01257]
ABSTRACT: The ionosphere is that part of the Earth's atmosphere that results mainly from the photo ionization of the upper atmosphere. Traditionally, the following ionospheric regions and their approximate ...


13. DMSP OLS - Operational Linescan System [gov.noaa.ngdc.G01119]
ABSTRACT: Visible and infrared imagery from DMSP Operational Linescan System (OLS) instruments are used to monitor the global distribution of clouds and cloud top temperatures twice each day. The ...


14. DMSP SSIES - Ion Electron Scintillation Monitor [gov.noaa.ngdc.G01127]
ABSTRACT: The SSIES measures the ambient electron density and temperatures, ambient ion density, the average ion temperature and molecular weight, the plasma drift and scintillation at the DMSP orbital ...


15. Airglow Data [gov.noaa.ngdc.G00603]
ABSTRACT: Airglow is a faint luminescence of the earth's upper atmosphere. The emitted electromagnetic radiation results mainly from photo-chemical reactions of upper atmospheric constituents. Although ...


16. Measurement of the Low-Energy Portion of the Primary Cosmic Ray Spectrum [gov.noaa.ngdc.G00599]
ABSTRACT: Most cosmic rays come from the galaxy, though some are produced by eruptive events on the Sun's surface. These high energy cosmic ray particles can affect satellites, causing single event ...


17. Energetic Solar Protons and Electrons - Data from GOES Satellites [gov.noaa.ngdc.G00543]
ABSTRACT: The Space Environment Monitor (SEM) instrument package on-board all GOES satellites has provided magnetometer, energetic particle, and soft X-ray data continuously since July 1974. Usually ...


18. Ionospheric Oblique Incidence Soundings by Satellites [gov.noaa.ngdc.G00563]
ABSTRACT: The oblique incidence sweep-frequency ionospheric sounding technique uses the same principle of operation as the vertical incidence sounder. The primary difference is that the transmitter ...


19. Ionospheric Values (Daily Work Sheets), F-Plots, Tabulations, Booklets, Catalogs, and Log Books [gov.noaa.ngdc.G00556]
ABSTRACT: These ionospheric data consist of scaling notes, equipment usage logs, and ionospheric values in the form of daily work sheets, F-Plots, tabulations, and booklets. The station notes list ...


20. Measurements of the Absorptive Properties of the Ionosphere [gov.noaa.ngdc.G00569]
ABSTRACT: Absorption of radio waves occurs when electrons responding to the wave fields collide with and transfer energy to the neutral particles. A study of ionospheric absorption yields information ...


21. Photographic Records Showing the Variations of the Virtual Height of Reflection as a Function of the Radio Frequency [gov.noaa.ngdc.G00551]
ABSTRACT: The standard (analog) ionosonde produces photographic records known as ionograms, which show the variations of the virtual height of reflection as a function of the radio frequency. The ...


22. Aurorae Data [gov.noaa.ngdc.G00594]
ABSTRACT: An aurora involves emitted electromagnetic radiation that results primarily from the interaction of energetic, extra-atmospheric particles with the neutral gases of the upper atmosphere. ...


23. Electron Density Profile Data Contains Virtual Height/Frequency Pairs from a Profile or Profiles (Composite Months) of Ionograms [gov.noaa.ngdc.G00146]
ABSTRACT: The Electron Density Profile, N(h), data set contains both individual profiles and composite months. The data consist of virtual height/frequency pairs from a profile or profiles (composite ...


24. Measurement of Incoherent Scatter [gov.noaa.ngdc.G00145]
ABSTRACT: For radio waves transmitted through the ionosphere with frequencies much larger (50 to 1300MHz) than the plasma frequency (up to 15MHz), very small-scale fluctuations of electron density ...


25. POES Space Environment Monitor, Energetic Particles [gov.noaa.ngdc.G00188]
ABSTRACT: The TIROS/NOAA satellite series, also known as POES, is designed to meet the National Oceanic and Atmospheric Administration's need for operational, remote sensing products for numerical ...


26. 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 ...


27. SHIRE Imaging Riometer, Davis, Antarctica [Riometer_SHIRE]
Mapping 38.2 MHz cosmic noise/particle precipitation in [2].7 x 7 beams 12.8 deg, ~200 x 200km at 90km altitude. A Southern Hemisphere Imaging Riometer Experiment. A joint project of the Australian ...


28. 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 ...


29. 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 ...


30. O(1S) Effective Lifetimes [ASAC_43]
Metadata record for data from ASAC Project 43 See the link below for public details on this project. From the abstract of the referenced paper: Intensity time-series ...


31. 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, ...


32. 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, ...


33. NOAA archive: Continuously Operating Reference Stations (CORS) [gov.noaa.ngdc.G10019]
The National Geophysical Data Center (NGDC) is the designated archive of the Continuously Operating Reference Stations (CORS) data set from the National Geodetic Survey (NGS). This record is for the ...


34. NASA THEMIS Mission Level 1 and 2 CDF Data [THEMIS_L1_L2_DATA]
[Source: THEMIS Mission Home page at Space Sciences Laboratory, University of California, Berkeley, CA, http://themis.ssl.berkeley.edu/overview.shtml ] THEMIS answers longstanding fundamental questions ...


35. 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: ...


36. 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 ...


37. 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 ...


38. 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 ...


39. Ionospheric dynamics in the polar cap [ASAC_949]
The aim is to measure structure and drift in polar-cap ionospheric layers in order to test current theories and models, identify unexplained behaviour and develop theoretical explanations. The polar ...


40. 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 ...


41. Geostationary Earth Radiation Budget experiment and data [GERB_OMA_BE]
The Institut Royal Meteorologique de Belgique ( RMIB ) and its On Line Short-term Service ( ROLSS ) provides near real-time Level 2.0 (radiances and fluxes) data from the GERB instruments. This ...


42. 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 ...


43. 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 ...


44. 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 ...


45. 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 ...


46. 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. ...


47. Advanced Composition Explorer (ACE) Solar Isotope Spectrometer (SIS) Level 2 Data [ACE_SIS_LEVEL2]
The Solar Isotope Spectrometer (SIS) is designed to provide high resolution measurements of the isotopic composition of energetic nuclei from He to Ni (Z=2 to 28) over the energy range ...


48. 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 ...


49. 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 ...


50. 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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