... Shibata Energy-frequency distribution of solarflares Large flares are less frequent ... energy: 1024 ~ 1032 ergs Frequency of solarflares with energy >1032 ergs: unknown ...
[
Текст
]
Ссылки http://www.stsci.edu/institute/conference/iausps13/presentations/Maehara.pdf -- 1529.0 Кб -- 05.02.2013 Похожие документы
... behavior of temperature and emission measure appear to follow similar trends as those seen in well-studied solarflares ... dynamical lo op mo dels developed from studies of solarflares reveals compact lo ops reminiscent of solar coronal behavior ...
... of the radiated energy during solar and stellar flares is emitted as white-light ... models using a solar-type flare heating mechanism (nonthermal electrons with a flux ...
... solar phenomena are extremely comp lex, including dynamos, coronal heating ... 4 keV, a common signature seen during solarflares but only rarely se en in stellar ... produced by magnetic reconnection flares near the solar surface (Meyer-Vernet 2007 ...
... 2.2 Solar Particle Radiation Solar particle events consist of solarflares and coronal mass ejections. ... Solarflares occur at a rate of 1000 per year and last a few hours. ...
[
Текст
]
Ссылки http://www.stsci.edu/jwst/doc-archive/technical-reports/JWST-STScI-000385.pdf -- 237.8 Кб -- 05.02.2013 Похожие документы
... Flares are yet another manifestation of magnetic activity, occurring in association with sunspot groups or ``active regions ... M dwarf flares emitting several orders of magnitude more energy than the largest solarflares have been observed. ...