Coronal mass ejections in July 2005 and an unusual heliospheric event
| Autor: | A. V. Belov, M. A. Livshits, A. I. Shakhovskaya, A. R. Osokin, E. A. Eroshenko, L. K. Kashapova |
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| Rok vydání: | 2013 |
| Předmět: |
Physics
Solar flare Coronal cloud Aerospace Engineering Astronomy Astronomy and Astrophysics Coronal loop Nanoflares Solar wind Earth's magnetic field Space and Planetary Science Physics::Space Physics Coronal mass ejection Astrophysics::Solar and Stellar Astrophysics Astrophysics::Earth and Planetary Astrophysics Magnetic cloud |
| Zdroj: | Cosmic Research. 51:326-334 |
| ISSN: | 1608-3075 0010-9525 |
| DOI: | 10.1134/s0010952513040072 |
| Popis: | Using the events in July 2005 as an example, the causes and peculiarities of Forbush effects produced by solar sources remote from the central zone are discussed. The event in question differs from other effects observed at the periphery of interplanetary disturbances by strong variations in cosmic rays on the background of weak disturbances in the solar wind and magnetic field of the Earth. The cloud of magnetized plasma ejected from the Sun was large and fast, but it passed to the west from the Sun-Earth line. According to performed estimates, the mass of the ejected substance was close to the upper boundary of mass for coronal mass ejections (CMEs). Anomalous parameters and high modulation capability of the formed solar wind disturbance are explained, in particular, by the fact that it combined several CMEs and that the last fast disturbance was prepared by a series of impulsive events in the active region of the Sun. Usually, such a great mass is ejected directly after the main energy release in strong solar flares. In the given case, a powerful MHD disturbance occurred approximately half an hour after a maximum of hard X-ray burst under the conditions when gas pressure in the flare loops became close to magnetic pressure, which was just a premise of the largescale ejection. |
| Databáze: | OpenAIRE |
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