2.0.1 spase://VSPO/DisplayData/STEREO-B/SWAVES/Spectrograms STEREO-B SWAVES Daily spectrograms 2009-07-08T00:00:00 Daily Summary spectrograms for STEREO-A and -B, 2.6 kHz - 16 MHz. Data for both spacecraft are on common plots. Electric field minute-averaged intensities above background are displayed. See Bougeret et al, Space Sci. Rev., 136, 2008, 487-528. Please acknowledge the SWAVES PI, J.L. Bougeret, and the SWAVES team. spase://SMWG/Person/Jean-Louis.Henry.Bougeret PrincipalInvestigator spase://SMWG/Person/Robert.J.MacDowall GeneralContact Space Sci. Rev. paper http://www.springerlink.com/content/205j176733432726/fulltext.pdf spase://SMWG/Repository/NASA/GSFC/STEREO_SC Online Open SWAVES site at GSFC http://swaves.gsfc.nasa.gov/cgi-bin/wimp.pl Common query specification and results display page JPEG spase://SMWG/Instrument/STEREO-B/SWAVES ElectricField Waves.Passive Spectrum 2006-10-27T00:00:00 P1D Spectra are current to within about 1 day. RadioFrequency Sun.Corona Heliosphere.Inner Heliosphere.Remote1AU spase://SMWG/Observatory/STEREO-B STEREO B STEREO Behind STEREO West Solar Terrestrial Relations Observatory B 2009-05-20T20:00:12Z The Solar-Terrestrial Relations Observatory (STEREO) mission includes two spacecraft respectively lagging (STEREO A) and leading (STEREO B) the Earth in heliocentric orbit around the Sun for remote 3-D imaging and radio observations of coronal mass ejections (CMEs). These events are responsible for large solar energetic particle events in interplanetary space and are the primary cause of major geomagnetic storms at Earth. The two spacecraft are launched to drift slowly away from the Earth in opposite directions at about 10 degrees per year for the lagging spacecraft and 20 degrees per year for the leading one. Optimal longitudinal separation of about sixty degrees is achieved after two years. Afterwards the separation gradually increases beyond the design lifetime of two years with the possibility of extended mission observations at larger angles. Science instruments selected for STEREO include the Sun Earth Connection Coronal and Heliospheric Investigation (SECCHI) for extreme ultraviolet (EUV), white-light coronographic, and heliospheric imaging, the STEREO/WAVES (SWAVES) interplanetary radio burst tracker, the In situ Measurements of Particles and CME Transients (IMPACT) investigation for in-situ sampling the 3-D distribution and plasma characteristics of solar energetic particles and the interplanetary magnetic field, and the PLAsma and SupraThermal Ion and Composition (PLASTIC) experiment to measure elemental and charge composition of ambient and CME plasma ions. STEREO data recorded and stored onboard each spacecraft will be downlinked through the NASA Deep Space Network on a daily schedule. Real-time space weather data will be continuously transmitted through a separate beacon system to NASA and non-NASA receiving stations. spase://SMWG/Person/Michael.L.Kaiser ProjectScientist STEREO Project Page http://stereo.gsfc.nasa.gov/ Project home page NSSDC's Master Catalog http://nssdc.gsfc.nasa.gov/database/MasterCatalog?sc=2006-047B Information about the STEREO B mission spase://vspo/observatory/140 STEREO Heliosphere.Remote1AU spase://SMWG/Instrument/STEREO-B/SWAVES Stereo/Waves (Swaves) Swaves 2009-05-20T21:10:12Z This experiment is designed to measure remotely and in situ: Type II radio bursts associated with electrons accelerated by CME-driven shocks; Type III radio bursts associated with impulsively accelerated electrons streaming out from the sun; in situ plasma waves and waveforms. Two radio receivers measure wave intensity, source direction and angular size in the frequency range 16 MHz to 40 kHz, corresponding to heliocentric source distances of about 1 Rs to 1 AU. One 10-40 kHz receiver measures radio and plasma waves near the 1 AU electron plasma frequency. One receiver makes high time resolution measurements at 50 MHz. Time Domain Samplers make simultaneous wideband waveform measurements on three electric components. Antenna systems include three mutually orthogonal 6-meter monopoles. spase://SMWG/Person/Jean-Louis.Henry.Bougeret PrincipalInvestigator NSSDC's Master Catalog http://nssdc.gsfc.nasa.gov/database/MasterCatalog?sc=2006-047B&ex=2 Information about the Stereo/Waves (Swaves) experiment on the STEREO B mission. Unspecified Stereo/Waves (Swaves) on STEREO B spase://SMWG/Observatory/STEREO-B spase://SMWG/Repository/NASA/GSFC/STEREO_SC STEREO Science Center SSC 2008-08-26T21:02:30Z STEREO Science Center, NASA/Goddard spase://SMWG/Person/Michael.L.Kaiser GeneralContact STEREO Science Center http://stereo-ssc.nascom.nasa.gov/ spase://SMWG/Repository/STEREO_SC spase://SMWG/Person/Michael.L.Kaiser Mr. Michael L. Kaiser GSFC-Code 695 spase://SMWG/Person/Robert.J.MacDowall Dr. Robert J. MacDowall GSFC-Code 695 spase://SMWG/Person/Jean-Louis.Henry.Bougeret Dr. Jean-Louis Henry Bougeret Observatoire de Paris-Meudon