Titlebook: Chromospheric Fine Structure; R. Grant Athay Book 1974 International Astronomical Union 1974 Chromosphere.Corona.LOPES.Sunspot.solar.sun

GEM

愛得痛了

睨視

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

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

DIKE

使迷惑

網(wǎng)絡(luò)添麻煩

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.

廢墟

Properties of the Solar Filigree StructureH. line (eg H. ± 7/8 ?). 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

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