行为
发表于 2025-3-26 22:40:13
The Solar Corona,e surface or photosphere (6000 K) to where it freely expands into the solar system as the solar wind. The exact reasons for its high temperature are still being debated despite more than 50 years of research, but magnetic fields are believed to be responsible for this heating. This article reviews s
RAFF
发表于 2025-3-27 01:57:24
The Solar Wind, of the Sun. The topic is split into two parts on the basis of two types of solar wind flows, (i) quasi-stationary winds and (ii) transient flows. The first part covers the basic ideas of the coronal heating and acceleration of the quasi-stationary wind. It also reviews the large-scale properties an
deviate
发表于 2025-3-27 09:22:02
https://doi.org/10.1007/3-540-36963-5Chromosphere; Corona; Solar wind; astrophysics; helioseismology; solar; solar physics; space science
infringe
发表于 2025-3-27 09:45:47
978-3-642-05686-4Springer-Verlag Berlin Heidelberg 2003
eulogize
发表于 2025-3-27 15:58:14
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TEM
发表于 2025-3-27 19:04:00
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脱落
发表于 2025-3-28 01:01:10
Lecture Notes in Physicshttp://image.papertrans.cn/l/image/583600.jpg
capillaries
发表于 2025-3-28 03:39:51
Magnetic Flux Tubes and Activity on the Sun,fundamental aspects of magnetic activity: (a) the generation, storage and emergence of magnetic fields from the solar interior; (b) the nature of the surface magnetic fields, especially in the form of small-scale flux tubes; and (c) dynamical processes in flux tubes and heating of the magnetic chromosphere.
现代
发表于 2025-3-28 06:23:42
Book 2003sciences. All contributions are self-contained and do not require prior in-depth knowledge of solar physics. The result is a unique textbook that fulfills the needs of those wishing to have a pedagogic exposition of solar physics bringing them up-to-date in a field full of vitality and with exciting research. .
Irrigate
发表于 2025-3-28 11:14:34
Solar Magnetic Fields, rudiments of such a dynamo mechanism are discussed. Some recent issues arising out of new theoretical and observational developments are mentioned. The importance of magnetic topology for various solar phenomena is highlighted. Finally, a few methods of measuring solar magnetic fields are described.