October 7, 2009 during flight testing of the spacecraft Meteor-M "№ 1 carried out switching on the GGAK-M heliogeophysical complex by NTs OMZ

All instrument of GGAK-M complex operates reliably
1.Multichanel geoactive corpuscular radiation spectrometer MSGI-ICA.
2.Solar cosmic rays spektrometr SKL-M.
3.Galactic cosmic rays detektor GALS-M.
4.Radiofrequency mass spectrometer Rims-M.
5.Shortwave radiation gauge ICOR-M.

In the Research Center for Earth Operative Monitoring and other organizations-developers of the components of the complex, the Institute of Applied Geophysics. Academician EK Fedorova, Roshydromet, the Research Institute of Nuclear Physics of Moscow State University. MV University, the Research Institute of Natural Sciences of SSU them. IG Chernyshevskogo in the Special Design Office of Space Instrumentation IKI receives the service information and information about heliogeophysical the following parameters:

— Differential energy spectra of low-energy electrons in the energy range 0.05 … 20.0 keV;

— Flux density of electrons with the detuning from the background of protons in the energy intervals 0,03-0,1-0,7-2,0-4,0-6,0 and  6,0 MeV;

— Flux density of protons with the detuning from the background electrons in the energy intervals 0,5-3,0-10,0-30,0-50,0-100,0-300,0;  300,0;  600,0 MeV ;

— Pitch-angle distribution of electron fluxes with energies 0,1-1,0 MeV proton events with energies 3,0-30,0 MeV;

— Ionic composition of the upper atmosphere in the range of 1.4 amu (including ions of hydrogen and helium);

— Ionic composition of the upper atmosphere in the range 5-20 amu (including atomic ions of nitrogen and oxygen);

— Short-wave reflected solar radiation in the spectral range 0,2 … 4,0 m