Book of Proceedings: Ninth Workshop, Sunny Beach, Bulgaria, May 30 - June 3, 2017

Abstract

E Ed di it to or rs s: Katya Georgieva, Boian Kirov, Dimitar DanovProceedings of Ninth Workshop "Solar Influences on the Magnetosphere, Ionosphere and Atmosphere" Sunny Beach, Bulgaria, May 30 ÷ June 3, 2017 C C O O N N T T E E N N T T Sun and Solar Activity Podgorny I.M., Podgorny A.I. Diagnostics of Solar Flares by Analyzing the SpectralLine Emission of Highly Ionized Iron 01 Kalinichenko N., Olyak M., Konovalenko A., Brazhenko A., Ivantishin O., Lytvynenko O., Bubnov I., Yerin S., Kuhai N., Romanchuk O. A method for reconstructing the solar-wind stream structure beyond Earths orbit 07 Melnik V., Brazhenko A., Dorovskyy V., Rucker H., Panchenko M., Frantsuzenko A., Shevchuk M.. Decameter type IV burst associated with behind-limb CME observed on November 7, 2013 13 Miteva R., Samwel S.W., Krupar V. Solar radio burst emission from protonproducing flares and coronal mass ejections 19 Veselovsky I., Kaportseva K., Lukashenko A. Eight types of the solar wind and their origins 24 Stanislavsky A.A., Konovalenko A.A., Koval A.A., Volvach Ya.S.. An upgrade of the UTR-2 radio telescope to a multifrequency radio heliograph I., Gromov S.V., Kleimenova N.G., Dremukhina L.A.. Role of the IMF |Bz|/|By| in the appearance of the daytime high-latitude magnetic bays 103Proceedings of Ninth Workshop "Solar Influences on the Magnetosphere, Ionosphere and Atmosphere" Sunny Beach, Bulgaria, May 30 ÷ June 3, 2017 IV C C O O N N T T E E N N T T Solar Influences on the Lower Atmosphere and Climate Author index 133Proceedings of Ninth Workshop "Solar Influences on the Magnetosphere, Ionosphere and Atmosphere" Sunny Beach, Bulgaria, May 30 -June 3, 2017 Topic: Sun and Solar Activity Abstract.The photos of the pre-flare development observed in the spectral lines of highly ionized iron (SDO AIA apparatus) indicate the energy accumulation for a flare in the corona in the pre-flare local (about 1010 cm) high temperature structure. The pre-flare structures in the corona are observed in UV spectral lines of ions FeXXIV, FeXXIII, FeXVIII several hours before big solar flares. During a flare the emission of the UV spectral lines in the corona are increased explosively. These phenomena can be used for prediction of solar cosmic rays. Information obtained from the worldwide neutron monitor network and measurements on GOES spacecraft demonstrates unambiguously that solar cosmic rays are generated in solar flares. These phenomena are well described by the solar flare electrodynamical model, created on the basis of the observational data and the numerical magnetohydrodynamic simulation using the initial and boundary conditions, taken from the active regions observation before the flare. It is impossible to exclude that the similar mechanism of particle acceleration is responsible for galactic cosmic rays generation. Now all published mechanisms of cosmic ray generation are based on unproven assumptions. These assumptions are not confirmed by longterm observations. With the modern concept of cosmic rays, a fundamentally important qu...