Global Change Master Directorygsfc-gcmduso@mail.nasa.gov502013-05-25T02:19:39ZGCMD Search: Parameters|SUN-EARTH INTERACTIONS|SOLAR ACTIVITY|SOLAR RADIO WAVE EMISSIONShttp://mddemo.gsfc.nasa.gov/KeywordSearch/OpenSearch.do 22 0 http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]NCAR_DS834.0NGDC Sunspots and 10.7cm Flux, 1749-1992Jun1749-01-01T00:00:00Z1993-12-31T00:00:00Z2013-05-23T04:00:00ZThis dataset contains daily and monthly sunspot numbers for various periods
between 1749 and 1992 and daily and monthly solar flux from 1947.
The most current data should be available from the National ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]G02201International Polar Year Historical Data and Literature-180.0,-90.0,180.0,90.01882-01-01T00:00:00Z2007-12-31T00:00:00Z2012-05-13T04:00:00ZThe International Polar Year Historical Data and Literature collection (formerly known as the Discovery and Access of Historic Literature from the IPYs (DAHLI) project) is an online data collection ...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]SDO_DIF_PLACEHOLDERNASA Solar Dynamics Observatory (SDO) Science Data Products2012-02-01T05:00:00Z[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 ...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.G00581Sudden Ionospheric Disturbances (SID)-180.0,-90.0,180.0,90.01958-01-01T00:00:00ZT00:00:00Z2011-03-07T05:00:00ZABSTRACT: Sudden ionospheric disturbances (SID) are caused by solar flare enhanced X-rays in the 1 to 10 angstrom range. Solar flares can produce large increases of ionization in the D-region of the ...http://gcmd.gsfc.nasa.gov/getdif.htm?[NOAA-NMMR]gov.noaa.ngdc.G00546Radio Emissions from Jupiter-180.0,-90.0,180.0,90.01966-07-01T00:00:00Z1979-08-01T00:00:00Z2011-03-02T05:00:00ZABSTRACT: The National Geophysical Data Center holds a published series of observations of Jovian Dekametric Emission bursts recorded on the University of Colorado's Boulder radio spectrograph. Between ...http://gcmd.gsfc.nasa.gov/getdif.htm?[NOAA-NMMR]gov.noaa.ngdc.G00216Solar Radio Data-180.0,-90.0,180.0,90.01947-02-14T00:00:00ZT00:00:00Z2011-03-01T05:00:00ZABSTRACT: Scientists monitor the structure of the solar corona, the outer most regions of the Sun's atmosphere, using radio waves. The surface of the Sun is 6,000 degrees Kelvin, while the high corona ...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?[CANADA-CGDI]FE00216Ottawa/Penticton 2800 MHz Solar Radio Flux1947-02-14T00:00:00ZT00:00:00Z2010-03-08T05:00:00ZSolar 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 ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]NASA_STEREO_DATA_PLACEHOLDERNASA STEREO (Solar TErrestrial RElations Observatory) Data Products2006-10-26T00:00:00ZT00:00:00Z2009-08-03T04:00:00Z[Source: NASA/GSFC Solar TErrestrial RElations Observatory (STEREO) home page, http://stereo.gsfc.nasa.gov/ ]
STEREO (Solar ...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]SOLAR_BASS2000Solar Ground-Based Data from the Base de donnees Solaire Sol (BASS) 2000 Project1995-10-01T00:00:00ZT00:00:00Z2009-03-30T04:00:00ZBASS 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 ...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]CULGOORAImages in H-alpha, 80, 160, and 327 MHz, and dynamic spectrograph data from Culgoora Observatory, Australia1950-01-01T00:00:00ZT00:00:00Z2005-11-04T05:00:00ZThe 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 ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]DCB2_SA-001Global Solar Activity Data Catalog at World Data Center B2, Moscow, USSR-180.0,-90.0,180.0,90.01957-07-01T00:00:00ZT00:00:00Z2005-08-01T04:00:00ZThe catalog contains solar data received by World Data Center-B2 from
1957-1986. The geographic coordinates of stations are given in the
stations-list. The observing instruments are described in the ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]ULYSSESUlysses Heliospheric Data1990-10-06T00:00:00ZT00:00:00Z2005-07-29T04:00:00ZThe 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 ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]JCADM_CDA_DNA_IONOSPHYSICSIonosphere Physics Data from Belgrano and San Martin Bases, Antarctica-67.103,-68.13,-67.103,-68.13-36.917,-77.967,-36.917,-77.967-34.627,-77.875,-34.627,-77.8751963-01-01T00:00:00Z1979-12-31T00:00:00Z1980-01-01T00:00:00ZT00:00:00Z1991-01-01T00:00:00ZT00:00:00Z2005-07-28T04:00:00ZVertical incidence ionosoundings are being performed at the Belgrano
and San Martmn stations. Ionospheric cosmic noise absorption is
continuously recorded at the same stations, at a frequency of ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]BIMASolar Flare Data from the Berkeley-Illinois-Maryland Array1989-01-01T00:00:00ZT00:00:00Z2005-07-28T04:00:00ZThe BIMA array is a 3-element radio interferometer. Flare
observations at 86 GHz with high spatial resolution were obtained
during the Flares 22/MAX'91 campaign of December 1991/Jnauary 1992.
Times ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]SRO-01Solar Radio Observations from Space1962-09-29T00:00:00Z1977-04-26T00:00:00Z2005-07-28T04:00:00ZMany spacecraft were launched from 1962 thru 1973 to record solar and
cosmic radio bursts. The spacecraft carried receivers for various
frequency ranges, and collected data intermittently over those ...http://gcmd.gsfc.nasa.gov/getdif.htm?[GCMD]CDA_AR_ATMO_VLF_SIGNALSVLF Signals-36.92,-77.97,-36.92,-77.971974-01-01T00:00:00Z1990-12-31T00:00:00Z2002-04-03T05:00:00ZVLF (Very Low Frequency) signals in the range of 10-34 kHz are
continuously recorded during the polar night.