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Titlebook: Coronal Magnetic Energy Releases; Proceedings of the C Arnold O. Benz,Albrecht Krüger Conference proceedings 1995 Springer-Verlag Berlin He

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樓主: Washington
11#
發(fā)表于 2025-3-23 10:54:52 | 只看該作者
Wavelet Theory and Its Applicationsting process of active, rapidly rotating stars. However, the required cadence of flares has not (yet) been found. The link between stellar coronal heating and magnetic energy release is not clear as long as the various flare-like phenomena in the solar corona are not better understood.
12#
發(fā)表于 2025-3-23 17:31:54 | 只看該作者
Gender Segregation in the Workplaceal images, a much faster operation. Ordering the archive by its content, which facilitates searching and comparing tasks, is investigated using self-organizing maps. Such a map conserves the topological order of the input space. This property may be used to automatically distinguish dissimilar emission types.
13#
發(fā)表于 2025-3-23 18:16:10 | 只看該作者
Gender Segregation in the Workplaceedium has been carried out at Cambridge since March 1990. The method will be described and some typical disturbances observed during this period will be shown. The results provide new insights into the nature of coronal magnetic energy releases responsible for the most powerful interplanetary shocks.
14#
發(fā)表于 2025-3-24 00:47:22 | 只看該作者
A. Lempicki,A. J. Wojtowicz,C. Brecher temperature range from 10.to 2 × 10... SUMER will be flown on the ESA/NASA spacecraft Solar and Heliospheric Observatory (SOHO) to be launched in September 1995. SOHO will be positioned near the first Lagrangean point (L1) of the Sun-Earth system.
15#
發(fā)表于 2025-3-24 03:06:06 | 只看該作者
Flares and coronal heating in the sun and stars,ting process of active, rapidly rotating stars. However, the required cadence of flares has not (yet) been found. The link between stellar coronal heating and magnetic energy release is not clear as long as the various flare-like phenomena in the solar corona are not better understood.
16#
發(fā)表于 2025-3-24 10:25:58 | 只看該作者
17#
發(fā)表于 2025-3-24 12:53:38 | 只看該作者
Interplanetary scintillation imaging of disturbances in the solar wind,edium has been carried out at Cambridge since March 1990. The method will be described and some typical disturbances observed during this period will be shown. The results provide new insights into the nature of coronal magnetic energy releases responsible for the most powerful interplanetary shocks.
18#
發(fā)表于 2025-3-24 15:31:26 | 只看該作者
,SUMER — Solar Ultraviolet Measurements of Emitted Radiation, temperature range from 10.to 2 × 10... SUMER will be flown on the ESA/NASA spacecraft Solar and Heliospheric Observatory (SOHO) to be launched in September 1995. SOHO will be positioned near the first Lagrangean point (L1) of the Sun-Earth system.
19#
發(fā)表于 2025-3-24 20:04:13 | 只看該作者
20#
發(fā)表于 2025-3-25 01:45:48 | 只看該作者
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