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Wolf – Rayet stars and relativistic objects

of the flare to the CME arrival at the Earth. The shock wave effectively accelerated electrons. The middle panel of Fig. 15 displays the time dependences of the electron fluxes with energy from 0.3 to 12MeV, which have not been measured by other satellites in this time outside the geomagnetosphere. The upper panel of Fig. 15 shows the electron energy powerlaw index variations. The electron energy spectrum did not vary significantly as the CME approached the Earth. The electron spectra became softer, and the electron, as well as proton and ion, fluxes started decreasing as the CME receded from the Earth. The CORONAS-F satellite also measured the ion fluxes with energy from 2 to 40 MeV per nucleon. The time variations of ions from C to Si were similar to proton and electron variations. The chemical composition of ion fluxes over the entire duration of the high-energy particle outburst practically did not change. Table 3 shows the percentage abundance of different elements relative to oxygen for the flare of November 4 ± 7, 2001.