fulmination
发表于 2025-3-27 00:52:58
https://doi.org/10.1007/978-3-662-44625-6astrophysical diffuse media; astrophysical magnetic fields; interstellar medium properties; magnetic tu
Servile
发表于 2025-3-27 03:18:09
0067-0057 medium and for star formation. Written by a group of leading experts the book represents an excellent overview of the field. Nonspecialists will find sufficient background to enter the field and be able to appreciate the state of the art.978-3-662-50722-3978-3-662-44625-6Series ISSN 0067-0057 Series E-ISSN 2214-7985
inscribe
发表于 2025-3-27 06:57:02
Interstellar Grain Alignment: Observational Statusas having been empirically confirmed, the first two have failed some critical observational tests, whereas the latter has recently been given specific observational support and must now be viewed as the leading candidate.
冥想后
发表于 2025-3-27 11:54:52
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GUISE
发表于 2025-3-27 13:51:26
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完成才会征服
发表于 2025-3-27 20:02:07
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Irremediable
发表于 2025-3-28 00:10:18
Synchrotron Radiation and Faraday Rotationtudy of Faraday rotation in particular, rapid development is taking place in techniques to confidently recover the physical conditions of the magnetoionized medium in the Milky Way and extragalactic objects.
STRIA
发表于 2025-3-28 05:44:48
Kinetic Turbulenceence. Key questions about the nature of kinetic turbulence that drive current research efforts are identified. A comprehensive model of the kinetic turbulent cascade is presented, with a detailed discussion of each component of the model and a review of supporting and conflicting theoretical, numerical, and observational evidence.
2否定
发表于 2025-3-28 08:34:16
Interstellar Polarization and Magnetic Turbulencence in the magnetic field is necessarily an indirect process. In this chapter we explore several techniques and results for using polarimetry to explore the turbulent component of the magnetic field in the Galaxy.
Laconic
发表于 2025-3-28 11:51:11
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