GEM
发表于 2025-3-30 11:22:00
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爱得痛了
发表于 2025-3-30 15:00:19
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睨视
发表于 2025-3-30 16:57:39
Spicules and Their Surroundingsge about spicules both from limb and disk observations, also because it does not seem feasible to discuss the problem of . between spicules and their surroundings without starting by what is known about spicules themselves.
Somber
发表于 2025-3-30 22:21:28
Radiation Pressure in Stellar Atmospheres with Application to Solar Spiculestmosphere. In particular, it is suggested that spicules ejected from the upper solar chromosphere as well as other fine structural features of the chromosphere may very likely be a result of radiation pressure from Ly-.. Numerical computation of the radial radiation pressure due to Ly-. in the chrom
photopsia
发表于 2025-3-31 01:16:31
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DIKE
发表于 2025-3-31 07:35:17
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使迷惑
发表于 2025-3-31 10:07:36
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网络添麻烦
发表于 2025-3-31 16:03:33
Why the Chromosphere has Its Discrete Fine Structuree will first deal with this flux concentration by the convection and its constraints. Then we will discuss the chromospheric network and its main constituent, the spicules. Following that we will look at the inside of the network, i.e. the fibrils.
废墟
发表于 2025-3-31 17:50:09
Properties of the Solar Filigree StructureH. line (eg H. ± 7/8 Å). Dunn and Zirker observed these bright structures with the highest possible resolution using the Sacramento Peak vacuum solar telescope. They find that these bright regions exhibit a very intricate fine structure which can be followed out much further into the H. line wing (e
粘连
发表于 2025-3-31 23:00:31
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