Russian cooperative investigation of solar, heliospheric and magnetospheric processes during October-November 2003

Physics

Scientific paper

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2118 Energetic Particles, Solar, 2139 Interplanetary Shocks, 2736 Magnetosphere/Ionosphere Interactions, 2784 Solar Wind/Magnetosphere Interactions

Scientific paper

The review of the Joint Russian Cooperation of Solar Extreme Events of October-November, 2003(JRC -SEE) efforts will be presented in the multidisciplinary analysis of the data obtained on ground based geophysical and astronomical observatories as well as spacecrafts.Strong solar, heliospheric and magnetic storms are well documented and placed in the context of current studies and retrospective knowledge. Data from CORONAS-F satellite substantially contribute to the better understanding of the solar flare and coronal mass ejection dynamics in the EUV, X-ray, gamma-ray and neutron emissions. In situ measurements of charged energetic particles characteristics in broad spectral ranges are performed onboard CORONAS-F, METEOR, ISS, and several geo-stationary satellites in the near the Earth space. This allows to make important conclusions about the radiation conditions, acceleration and propagation processes of energetic ions and electrons. ODYSSEY/HEND instrument on the orbit around the Mars also brings the valuable information from the different vantage point during this period of time. Observed electromagnetic emissions in the broad range from radio to gamma rays, plasma waves and motions, energetic particle and cosmic ray characteristics, neutrons give some clues to the physics of the solar and heliospheric releases as well as solar-terrestrial relations during this highly perturbed period of time. New features in this respect will be presented and discussed.

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