Titlebook: Solar Magnetic Fields; Polarized Radiation Jan Olof Stenflo Book 1994 Springer Science+Business Media B.V. 1994 collision.field theory.qua

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Book 1994ocesses be explored in detail. While severalexcellent textbooks have established a diagnostic foundation forexploring the physics of unmagnetized stellar atmospheres throughspectral analysis, no corresponding treatise for magnetized stellaratmospheres has been available. The present monograph fills

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,Solar Magnetism — An Overview,g processes. These interactions manifest themselves in various signatures of stellar activity, like dark spots, bright faculae, flare eruptions, X-ray emissions, coronal transients, wind streams, etc. On a global scale they form a complex pattern that has a cyclic evolution. The sun serves as a prototype for stellar activity.

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Multi-Level Radiative Transfer with Coherence Effects,TE theory of polarized radiative transfer. This theory should be able to account for any coherences that may occur between the atomic levels. The formulations developed in Chapters 3–6 may be retrieved as special cases, and parameters that were previously introduced heuristically can be derived.

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