Solar cosmic rays in a source according to data of observations of energetic particles, hard X radiation and radioemission

Results of observations of splashes of hard x radiation and solar cosmic rays (SCR) are discussed. Measurement data of electron fluxes are presented for the 0.025-1.6 MeV energy range, protons with the energy of E approximately 1-60 MeV, and X-ray quanta with E=0.05-0.75 MeV. Differential distribution of a number of SCR flares in maximum electron flux. Jsub(e) with E>0.07 MeV, accompanied by splashes of hard and thermal x radiation is presented along with distribution of SCR events in Jsub(e), when splashes of hard x radiation were not recorded. Electron differential spectra factors γsub(e) are presented as a function of Jsub(e) within the 0.025-0.2 MeV energy range. It is shown that events in SCR accompanied with hard x radiation are different from those not accompanied with hard x radiation by a slope of electron spectrum and γsub(e)(Jsub(e)) dependence