不可接触
发表于 2025-3-23 10:20:22
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FRAUD
发表于 2025-3-23 15:11:08
Magnetic fields on K and M dwarfs,Of seven late K and early M dwarfs, six were observed to have magnetic fields. No relationship was seen between effective temperature and either field strength or filling factor. Magnetic flux was observed not to be constant over this range of effective temperature.
干旱
发表于 2025-3-23 21:47:23
Empirical relations between magnetic fluxes and atmospheric radiative losses for cool dwarf stars,We derive and discuss relations between magnetic, X-ray, and Ca II H+K flux densities for a sample of G, K, and M dwarfs.
子女
发表于 2025-3-23 23:08:43
Broadband linear polarization and chromospheric CA II H and K emission in late-type main sequence sWe discuss correlations between broadband linear polarization, intrinsic stellar parameters, and Ca 11 H+K emission in G and K dwarfs.
显微镜
发表于 2025-3-24 06:21:53
Measurements of stellar magnetic fields: Empirical constraints on stellar dynamo and rotational evoWe explore the implications of empirical stellar magnetic parameters for dynamo theories, stellar activity theories, and models of the evolution of stellar angular momentum.
抛射物
发表于 2025-3-24 10:18:37
Design of Observer-based Controllers,ve been employed, producing a considerable body of data on the mean magnetic field strength in stellar active regions (B) and the fraction (filling factor = f) of the stellar surface covered by these fields (f) for G, K, and M dwarfs. I focus on some of the recent results of observational programs a
Gudgeon
发表于 2025-3-24 12:44:54
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懒鬼才会衰弱
发表于 2025-3-24 16:07:56
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讽刺滑稽戏剧
发表于 2025-3-24 21:46:19
Control Objectives and Strategies,gnetic fields in a wide class of stars has been greatly improved. Calculations of large scale (global) magnetic fields will be presented that utilize sequences of models of a rotating star (the Sun) that take into account differential rotation and meridional circulation. The influence of various mag
antedate
发表于 2025-3-25 00:04:32
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