Official name KORONAS-FOTON
Alternative name Koronas-Foton
Cospar ID 2009-003A
Norad ID 33504
Launch date 2009-01-30
Launch site PKMTR
Launch vehicle Tsiklon-3
Country/Organization Russia
Type application Science, solar
RCS size LARGE
Decay date ON ORBIT
Period (min) 94.39
Inclination (deg) 82.44
Perigee (km) 478
Apogee (km) 500
Eccentricity 0.0224948875255624
Mean motion (revs. per day) 15.2558533742981
Semi-Major axis (km) 6867.135
Raan (deg) 241.4488
Arg of perigee (deg) 20.667
Shape Cyl + 2 Pan
Mass (kg) 2250
Diameter (m) 2.4
Height (m) 6.5
Span (m^2) 12.7
Lifetime 3 years (planned); 1 year (achieved)
Contractors NPP VNIIEM
Configuration Meteor-M bus
Power 2 deployable solar arrays, batteries

CORONAS (Complex ORbital Observations Near-Earth of Activity of the Sun) is a Russian program for study of the Sun and solar-terrestrial connections physics by series of spacecraft, which provides launching of three solar-oriented satellites onto the near-Earth orbit.

CORONAS-PHOTON (or Koronas-Foton) is the third satellite in this series. Two previous missions of the project are CORONAS-I (launched on 2 March 1994) and CORONAS-F (launched on 31 July 2001). Launching date of “CORONAS-PHOTON” spacecraft is 2009.

CORONAS-PHOTON is a part of International Living With a Star Program (ILWS).

The main goal of the project is the investigation of energy accumulation and its transformation into energy of accelerated particles processes during solar flares; the study of the acceleration mechanisms, propagation and interaction of fast particles in the solar atmosphere; the study of the solar activity correlation with physical-chemical processes in the Earth upper atmosphere.

Objectives of the mission:

Physics of the Sun

  • Determination of distribution functions of accelerated electrons, protons and nuclei and their dynamics with a high time resolution;
  • Research of difference in acceleration dynamics of electrons and protons (nuclei);
  • Research of distribution function variations for high energy particles (up to a few  GeV);
  • Research of interacting particle angular anisotropy by statistical analysis of radiation spectra and linear polarization parameters of hard X-rays;
  • Study of directional effects in the region of high energy gamma radiation;
  • Determination of mechanisms and requirements of electrons and protons acceleration in different flare phases, and parameters of propagation region of accelerated particles;
  • Determination of elemental abundance in the region of gamma-ray production by gamma spectroscopy and capture of low energy neutrons in the solar atmosphere;
  • Determination of radiation generation altitudes by observation of deuteron line weakening from limb flares;
  • Determination of energy spectra view of accelerated protons and nuclei and dynamics of these spectra according to nuclear gamma-line ratio;
  • Study of light elements generation (D, 3He, Li, Be) during flares;

Solar-terrestrial connections physics

  • Research of chemical and isotopic compositions of nuclei accelerated in flare on the Earth orbit, and also energy and temporal parameters of flare electrons and protons;
  • Monitoring of the Earth upper atmosphere by absorption of extreme ultraviolet of the quiet Sun;

Astrophysics

  • Study of hard X-ray and gamma radiation from gamma-ray bursts;
  • Study of X-ray radiation from the bright local sources along Ecliptic plane.

The powersystem of Koronas-Foton failed in mid January 2010, ending the mission after only one year in orbit.

Satellite COSPAR Date LS Launch Vehicle Remarks
KORONAS-FOTON 2009-003A 2009-01-30 PKMTR Tsiklon-3