Äîêóìåíò âçÿò èç êýøà ïîèñêîâîé ìàøèíû. Àäðåñ
îðèãèíàëüíîãî äîêóìåíòà
: http://smdc.sinp.msu.ru/index.py?nav=meteor_m
Äàòà èçìåíåíèÿ: Unknown Äàòà èíäåêñèðîâàíèÿ: Sat Apr 9 22:47:39 2016 Êîäèðîâêà: Windows-1251 Ïîèñêîâûå ñëîâà: ð ð ð ð ð ð ð ð ð ð ð ð ð ð ð ð ð ð ð ð ð ð ð ð ð ð ð ð ð ð ð ð ð ð ð ð ð ð ð ð ð ð ð ð ð ð ð ð ð ð ð ð |
|
|||||||||||||||||||||||||||||||||||||||||||||||||||||||
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
| |||||||||||||||||||||||||||||||||||||||||||||||||||||||
| |||||||||||||||||||||||||||||||||||||||||||||||||||||||
Developed in 2007. Copyright ¿ 2007 - 2016 Skobeltsyn Institute of Nuclear Physics Moscow State University Feedback |