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: http://smdc.sinp.msu.ru/index.py?nav=meteor_m
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Meteor-M no.1
PurposeGlobal observation of the Earth's atmosphere and surface, allowing to systematically obtain hydrometeorological and heliogeophysical information at planetary scale. Among other instruments Meteor-M no.1 carries the heliogeophysical hardware package GGAK-M, which brings six a wide range of emission detection instruments to a single platform. These include SGMTD, MIP, DAS-4 and DAS-1 (2 differently directed instruments each). This creates a powerful system for detecting proton and electron fluxes in the near-Earth space. 1. The MSGI-MKA spectrometer is used to measure the following parameters:
MSGI-MKA is built as a single block comprised of two identical units. At any moment only one unit is operating, while the second one is in cold stanby mode. 2. SKL-MKA is used to measure the following parameters:
SKL-MKA is built as a single block comprised of two identical units. At any moment only one unit is operating, while the second one is in cold stanby mode. Z axis is directed from the center of the Earth to the satellite, X axis is directed as tangential velocity vector Parameters measured
Nominal geometric factor for SKL and MSGI instruments is 0.1, i.e., counts/sec * 10 = flux in units of protons/cm2/sec/ster. Charged particle fluxes measurement |