miniature
发表于 2025-3-28 17:06:03
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废除
发表于 2025-3-28 18:46:57
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Disk199
发表于 2025-3-29 02:29:26
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indoctrinate
发表于 2025-3-29 06:04:15
Observing the Solar Magnetic Field,powerful for low-resolution magnetic diagnostics based on analysis of Hanle effect in prominences and the emission line corona. Employment of a new generation large-aperture reflecting coronagraph allows to expect advances in high-resolution magnetic observations of prominence and coronal structures.
animated
发表于 2025-3-29 10:18:40
Solar Activity,activity indices and activity mapping, the 11-, 22- and 100-year solar activity cycles, and their effect on the quiet sun, with solar variability. We finish with a few comments on the solar-stellar relation.
NADIR
发表于 2025-3-29 11:48:57
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赦免
发表于 2025-3-29 18:09:06
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GRAZE
发表于 2025-3-29 22:52:06
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Lacunar-Stroke
发表于 2025-3-30 00:55:02
Wenan Tan,Zhejun Liang,Jin Liu,Kai Dingd in the last twenty years, which permits to probe directly the solar interior by means of acoustic waves, and this had a tremendous impact on solar physics because it provides tight observational constraints on our models. We shall illustrate this here by a few examples of recent advances in modeling the Sun.
intention
发表于 2025-3-30 06:24:49
Heliospheric Extent of the Coronal Phenomena,na is watched both from ground and from space. The solar space missions Yohkoh and SOHO are registering coronal phenomena in the X and UV radiations in the ecliptic plane, while Ulysses is crossing over the polar solar region (at an angle of about 87° with the ecliptic plan).