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- a0abb2f4-579b-4dfe-a35e-5074b57dfe63 definition "The Solar Wind Experiment (SWE) on WIND will measure ions and electrons in the solar wind and the foreshock regions (particles whose energies are in the kiloelectronvolt range). From these measurements, the solar wind velocity, density, temperature and heat flux can be deduced. Electron and ion velocity distributions should reveal properties of the following plasmas and their pivotal role in the transfer of mass, momentum, and energy from the Sun to the Earth. Measurements made in the foreshock region will contribute to understanding the structure of the bow shock. The SWE instrument consists of five integrated sensor/electronics boxes and a data processing unit (DPU). The sensor units are mounted on the top and bottom shelves of the spacecraft, extending through the top and bottom surfaces. 3D velocity distribution measurements of the ion component in the solar wind are made by a pair of Faraday Cup analyzers, which provide a wide field-of-view and the capability for flow characterization within one spin revolution (3 seconds). 3D velocity distribution measurements of ions and electrons in plasmas having Mach numbers. For more information, see: http://web.mit.edu/afs/athena/org/s/space/www/wind.html Group: Instrument_Details Entry_ID: SWE Group: Instrument_Identification Instrument_Category: Solar/Space Observing Instruments Instrument_Class: Particle Detectors Short_Name: SWE Long_Name: Solar Wind Experiment (WIND) End_Group Group: Associated_Platforms Short_Name: WIND End_Group Group: Spectral_Frequency_Information Wavelength_Keyword: Gamma Ray Number_Channels: 5 Spectral_Frequency_Coverage_Range: 5 eV - 22 KeV End_Group Online_Resource: http://web.mit.edu/afs/athena/org/s/space/www/wind.html Sample_Image: http://web.mit.edu/space/www/wind/wind_figures/wind-3.339x269.gif Group: Instrument_Logistics Instrument_Start_Date: 1994-11-01 Instrument_Owner: NASA Instrument_Owner: MIT Instrument_Owner: University of New Hampshire End_Group End_Group" @default.
- a0abb2f4-579b-4dfe-a35e-5074b57dfe63 id "1655208" @default.
- a0abb2f4-579b-4dfe-a35e-5074b57dfe63 path_id 02c354fd-8e2d-4825-b786-aa4b0782d1d6 @default.
- a0abb2f4-579b-4dfe-a35e-5074b57dfe63 path_id 5f5e4f2c-61b7-4694-8680-3fc5799f6171 @default.
- a0abb2f4-579b-4dfe-a35e-5074b57dfe63 path_id b2140059-b3ca-415c-b0a7-3e142783ffe8 @default.
- a0abb2f4-579b-4dfe-a35e-5074b57dfe63 path_label "Instruments" @default.
- a0abb2f4-579b-4dfe-a35e-5074b57dfe63 path_label "Particle Detectors" @default.
- a0abb2f4-579b-4dfe-a35e-5074b57dfe63 path_label "Solar/Space Observing Instruments" @default.
- a0abb2f4-579b-4dfe-a35e-5074b57dfe63 prefLabel "SWE" @default.
- a0abb2f4-579b-4dfe-a35e-5074b57dfe63 reference "" @default.
- a0abb2f4-579b-4dfe-a35e-5074b57dfe63 tag "Instruments" @default.
%20on%20WIND%20will%20measure%20ions%20and%20electrons%20in%20the%0Asolar%20wind%20and%20the%20foreshock%20regions%20(particles%20whose%20energies%20are%20in%20the%0Akiloelectronvolt%20range).%20From%20these%20measurements%2C%20the%20solar%20wind%20velocity%2C%0Adensity%2C%20temperature%20and%20heat%20flux%20can%20be%20deduced.%20Electron%20and%20ion%20velocity%0Adistributions%20should%20reveal%20properties%20of%20the%20following%20plasmas%20and%20their%0Apivotal%20role%20in%20the%20transfer%20of%20mass%2C%20momentum%2C%20and%20energy%20from%20the%20Sun%20to%20the%0AEarth.%20Measurements%20made%20in%20the%20foreshock%20region%20will%20contribute%20to%0Aunderstanding%20the%20structure%20of%20the%20bow%20shock.%0AThe%20SWE%20instrument%20consists%20of%20five%20integrated%20sensor%2Felectronics%20boxes%20and%20a%0Adata%20processing%20unit%20(DPU).%20The%20sensor%20units%20are%20mounted%20on%20the%20top%20and%20bottom%0Ashelves%20of%20the%20spacecraft%2C%20extending%20through%20the%20top%20and%20bottom%20surfaces.%0A3D%20velocity%20distribution%20measurements%20of%20the%20ion%20component%20in%20the%20solar%20wind%0Aare%20made%20by%20a%20pair%20of%20Faraday%20Cup%20analyzers%2C%20which%20provide%20a%20wide%20field-of-view%0Aand%20the%20capability%20for%20flow%20characterization%20within%20one%20spin%20revolution%20(3%0Aseconds).%203D%20velocity%20distribution%20measurements%20of%20ions%20and%20electrons%20in%0Aplasmas%20having%20Mach%20numbers.%0AFor%20more%20information%2C%20see%3A%0Ahttp%3A%2F%2Fweb.mit.edu%2Fafs%2Fathena%2Forg%2Fs%2Fspace%2Fwww%2Fwind.html%0A%0A%0AGroup%3A%20Instrument_Details%0A%20%20%20Entry_ID%3A%20SWE%0A%20%20%20Group%3A%20Instrument_Identification%0A%20%20%20%20%20%20Instrument_Category%3A%20Solar%2FSpace%20Observing%20Instruments%0A%20%20%20%20%20%20Instrument_Class%3A%20Particle%20Detectors%0A%20%20%20%20%20%20Short_Name%3A%20SWE%0A%20%20%20%20%20%20Long_Name%3A%20Solar%20Wind%20Experiment%20(WIND)%0A%20%20%20End_Group%0A%20%20%20Group%3A%20Associated_Platforms%0A%20%20%20%20%20%20Short_Name%3A%20WIND%0A%20%20%20End_Group%0A%20%20%20Group%3A%20Spectral_Frequency_Information%0A%20%20%20%20%20%20Wavelength_Keyword%3A%20Gamma%20Ray%0A%20%20%20%20%20%20Number_Channels%3A%205%0A%20%20%20%20%20%20Spectral_Frequency_Coverage_Range%3A%205%20eV%20-%2022%20KeV%0A%20%20%20End_Group%0A%20%20%20Online_Resource%3A%20http%3A%2F%2Fweb.mit.edu%2Fafs%2Fathena%2Forg%2Fs%2Fspace%2Fwww%2Fwind.html%0A%20%20%20Sample_Image%3A%20http%3A%2F%2Fweb.mit.edu%2Fspace%2Fwww%2Fwind%2Fwind_figures%2Fwind-3.339x269.gif%0A%20%20%20Group%3A%20Instrument_Logistics%0A%20%20%20%20%20%20Instrument_Start_Date%3A%201994-11-01%0A%20%20%20%20%20%20Instrument_Owner%3A%20NASA%0A%20%20%20%20%20%20Instrument_Owner%3A%20MIT%0A%20%20%20%20%20%20Instrument_Owner%3A%20University%20of%20New%20Hampshire%0A%20%20%20End_Group%0AEnd_Group%22){kind=link}