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METEOR 2.0
our successful space weather solution

meteor 2.0
Our successful space weather solution

meteor 2.0
Our successful space weather solution
mission
  • Measurement of fluxes, energy spectrums, time variations, angular distributions of ERP particles, SCR particles from solar flares
  • Obtaining heliogeophysical data at the height of the orbit in order to control and predict the radiation situation in near-Earth space, the state of the geomagnetic field and solar activity
why IT'S important?
Global continuous monitoring of radiation fields in the NES is required in order to protect electronic equipment from damage when interacting with energetic charges. Interaction with these particles can also cause failures in navigation systems, reduce the accuracy of global navigation and positioning systems
Our Solution
Measures:
  • differential energy spectrums of low-energy electrons and protons in the energy range from 0.05 to 20.0 keV
  • electron flux density with detuning from the background of protons in six energy intervals in the range from 0.15 to 10.0 MeV
  • proton flux density with detuning from the electron background in 8 energy intervals in the range from 2.0 to more than 160.0 MeV
  • integral fluxes of electrons with energy from 50 keV and integral fluxes of protons with energy from 800 keV
device sRS-He
CRS-HE
CRS-HE/H
ERS
Energetic Radiation Spectrometer
Corpuscular Radiation Spectrometer-Highly Elliptical/Horizontal
ESA
Electrostatic Analyzers
Corpuscular Radiation Spectrometer-Highly Elliptical
DETECTORS:
Telescope of three semiconductor and one scintillation detector
Electronic modules:
  • Amplifiers-shapers
  • Amplitude discrimination device
  • Logical device
  • Power supply
SGMTD-E
SGMTD-P
Segmentoid Analyzer -Electrons
MEASURES:
Electrons: 1-10 MeV
Protons: 1-300 MeV
Segmentoid Analyzer -Protons
ANALYZERS:
Segmentoid type electrostatic analyzers
MEASURES:
Electrons (spectrums):
0.05 - 20 keV
DETECTORS:
Secondary electron multiplier
ANALYZERS:
Segmentoid type electrostatic analyzers
MEASURES:
Protons (spectrums):
0.05 - 20 keV
DETECTORS:
Secondary electron multiplier
IFM
Integrated Flow Modules
CRS-HE/V
Corpuscular Radiation Spectrometer-Highly Elliptical/Vertical
Electronic modules:
  • Amplifier
  • Interface module
  • Signal splitter
ELECTRONIC
modules
Electronic modules:
  • Amplifier
  • Interface module
  • Signal splitter
MEASURES:
Electrons: over 40 keV
Protons: over 0.8 MeV
DETECTOR:
Highly directional end-face Geiger sensor
Omnidirectional Geiger sensors
DETECTOR:
MEASURES:
Electrons: over 1.7 MeV
Protons: over 50 MeV
Electronic modules:
  • Sensor signal amplifier
  • Interface module
  • Signal splitter
  • Power supply
  • High voltage power supply
  • Spectrometer protection module
  • Command board
  • Thermal sensors
Module CRS-HE/V is identical to CRS-HE/H. The difference is due the orientation relative to space craft
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