... maximal during solar minimum years due to the presence of the polar coronalholes ... the latitude of the source regions, but also by the presence of coronalholes nearby ...
[
Текст
]
Ссылки http://solarwind.cosmos.ru/txt/2011/presentations/Sun/Ishkov/apj_691_2_1222.pdf -- 1208.5 Кб -- 15.04.2011 Похожие документы
... propagation of high-speed streams of the solar wind from the coronalholes ... longitude structure of active regions and coronalholes, though this issue was not ... 428 (http://alpha.sinp.msu.ru/apev). regions, coronalholes, and active complexes ...
... one high-speed stream of the solar wind caused by a coronalhole into another stream ... solar wind from one (the most extended) coronalhole continued for several days and ...
... Relationship between the Parameters of CoronalHoles and High-Speed Solar Wind Streams over an Activity Cycle (Solar Phys, in press) Badalyan O.G. "Two Types of Differential Rotation of the Solar Corona" New Astronomy, 2010, v. 15, pp. ...
... V. N. Obridko, B. D. Shelting, I. M. Livshits and A. B. Asgarov, Contrast of CoronalHoles and Parameters of Associated Solar Wind Streams, 2009, Solar Physics. ...
... In addition to compact dimmings near ARs 10696, 10695, and 10693, a diffuse extensive dimming was formed north of AR 10696 in place of brightening previously observed in the initial images at the boundary of a low-latitude coronalhole. ...