Polar-efi

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  • POLAR-EFI
definition
  • The Electric Field Instrument (EFI) on the Polar spacecraft measures the three components of the ambient vector electric field and the thermal electron density. The electric field and plasma density measurements are made over a frequency range of DC to above 20 kHz. The dynamic range of the electric field measurement is 0.02 to 1000 mV/m, while the plasma density will be measured at least over the range of 0.1 to 100 particles per cubic centimeter. A by-product of the experiment is measurement of the floating potential of the spacecraft over the range of about +1 to +90 volts. An important component of the Electric Field Instrument is a two megabyte burst memory that allows storage of high time resolution field and plasma density measurements, allowing study of rapid variations of non-linear spatial structures and waves. The EFI sensors are arranged as three orthogonal sphere pairs whose potential differences and Langmuir probe characteristics are measured. Two of these sphere pairs are in the satellite spin plane on the ends of wire booms that provide tip to tip sphere separations of 100 and 130 meters respectively, while the third pair is aligned along the spacecraft spin axis with a 14 meter tip to tip separation that is provided by rigid stacer booms. The electric field preamplifiers have frequency responses to above one mHz to accommodate their use by the Plasma Wave Instrument. In addition, the Electric Field Instrument interfaces on the spacecraft with the Magnetic Field Expirement (which provides information for deciding when to trigger bursts of data collection), the Hydra plasma experiment (in order that both instruments collect high time resolution data simultaneously), and the low energy plasma experiment, Tide, (which wants to know when the Electric Field Instrument is collecting data in the burst mode). The heritage for the Electric Field Instrument encompasses instruments previously flown on the S3-3, GEOS, ISEE-1, Viking, and CRRES satellites, as well as experiments being built for the Freja, FAST, and Cluster satellites. Harvey, P., F. S. Mozer, D. Pankow, J. Wygant, N. C. Maynard, H. Singer, W. Sullivan, P. B. Anderson, R. Pfaff, T. Aggson, A. Pedersen, C. G. Falthammar, and P. Tanskannen, THE ELECTRIC FIELD INSTRUMENT ON THE POLAR SATELLITE, Space Science Reviews 71: 583-596, 1995. http://ssed.gsfc.nasa.gov/PolarEFI/Instrument/instrument.html For more information, see: http://ssed.gsfc.nasa.gov/PolarEFI/ and http://pwg.gsfc.nasa.gov/polar/polar_inst.shtml Group: Instrument_Details Entry_ID: EFI Group: Instrument_Identification Instrument_Category: Solar/Space Observing Instruments Instrument_Class: Magnetic Field/Electric Field Instruments Short_Name: EFI Long_Name: Electric Fields Investigation End_Group Group: Associated_Platforms Short_Name: POLAR End_Group Online_Resource: http://ssed.gsfc.nasa.gov/PolarEFI/index.html Online_Resource: http://ssed.gsfc.nasa.gov/PolarEFI/Instrument/instrument.html Group: Instrument_Logistics Instrument_Start_Date: 1996-02-24 Instrument_Owner: NASA End_Group End_Group
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  • Polar Electric Fields Instrument
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