脾气好
发表于 2025-3-21 19:10:18
书目名称Solar Magnetic Fields影响因子(影响力)<br> http://figure.impactfactor.cn/if/?ISSN=BK0871398<br><br> <br><br>书目名称Solar Magnetic Fields影响因子(影响力)学科排名<br> http://figure.impactfactor.cn/ifr/?ISSN=BK0871398<br><br> <br><br>书目名称Solar Magnetic Fields网络公开度<br> http://figure.impactfactor.cn/at/?ISSN=BK0871398<br><br> <br><br>书目名称Solar Magnetic Fields网络公开度学科排名<br> http://figure.impactfactor.cn/atr/?ISSN=BK0871398<br><br> <br><br>书目名称Solar Magnetic Fields被引频次<br> http://figure.impactfactor.cn/tc/?ISSN=BK0871398<br><br> <br><br>书目名称Solar Magnetic Fields被引频次学科排名<br> http://figure.impactfactor.cn/tcr/?ISSN=BK0871398<br><br> <br><br>书目名称Solar Magnetic Fields年度引用<br> http://figure.impactfactor.cn/ii/?ISSN=BK0871398<br><br> <br><br>书目名称Solar Magnetic Fields年度引用学科排名<br> http://figure.impactfactor.cn/iir/?ISSN=BK0871398<br><br> <br><br>书目名称Solar Magnetic Fields读者反馈<br> http://figure.impactfactor.cn/5y/?ISSN=BK0871398<br><br> <br><br>书目名称Solar Magnetic Fields读者反馈学科排名<br> http://figure.impactfactor.cn/5yr/?ISSN=BK0871398<br><br> <br><br>
小故事
发表于 2025-3-21 21:01:22
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enmesh
发表于 2025-3-22 01:09:55
Collisions, Partial Redistribution, and Turbulent Magnetic Fields,In the preceding chapters we have developed the foundations for treating general problems involving radiative scattering in a magnetic field. The theory however needs to be completed by including the effects of collisions and partial redistribution before it is ready for general use on the sun.
DALLY
发表于 2025-3-22 06:24:17
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SHOCK
发表于 2025-3-22 11:58:13
Introduction to Quantum Field Theory of Polarized Radiative Transfer,ubject. The framework of quantum field theory with a quantization of the electromagnetic field should however be used for a consistent treatment and a logical development of the theory of polarized radiative transfer in a magnetic field from first principles.
induct
发表于 2025-3-22 16:43:17
Instrumentation for Solar Polarimetry,racy, spectral, spatial, and time resolution, and spectral and spatial coverage. As it is not possible to optimize all these parameters simultaneously, various combinations of trade-offs are needed. The type of trade-off that one selects depends on the scientific objective of the observations.
类人猿
发表于 2025-3-22 20:03:05
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扫兴
发表于 2025-3-22 22:27:57
https://doi.org/10.1007/978-94-015-8246-9collision; field theory; quantum field theory; scattering; solar; spectra; universe
含铁
发表于 2025-3-23 03:23:50
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Gingivitis
发表于 2025-3-23 08:15:53
,Solar Magnetism — An Overview, sun we know that stellar atmospheres are highly structured, governed by an intricate interplay between magnetic forces, turbulent motions, and heating processes. These interactions manifest themselves in various signatures of stellar activity, like dark spots, bright faculae, flare eruptions, X-ray