Titlebook: Cool Stars, Stellar Systems, and the Sun; Proceedings of the F Jeffrey L. Linsky,Robert E. Stencel Conference proceedings 1987 Springer-Ver

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FRAUD

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

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

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.

顯微鏡

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.

拋射物

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

懶鬼才會衰弱

諷刺滑稽戲劇

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

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