从未沮丧
发表于 2025-3-21 18:41:46
书目名称Astronomical Polarisation from the Infrared to Gamma Rays影响因子(影响力)<br> http://figure.impactfactor.cn/if/?ISSN=BK0163603<br><br> <br><br>书目名称Astronomical Polarisation from the Infrared to Gamma Rays影响因子(影响力)学科排名<br> http://figure.impactfactor.cn/ifr/?ISSN=BK0163603<br><br> <br><br>书目名称Astronomical Polarisation from the Infrared to Gamma Rays网络公开度<br> http://figure.impactfactor.cn/at/?ISSN=BK0163603<br><br> <br><br>书目名称Astronomical Polarisation from the Infrared to Gamma Rays网络公开度学科排名<br> http://figure.impactfactor.cn/atr/?ISSN=BK0163603<br><br> <br><br>书目名称Astronomical Polarisation from the Infrared to Gamma Rays被引频次<br> http://figure.impactfactor.cn/tc/?ISSN=BK0163603<br><br> <br><br>书目名称Astronomical Polarisation from the Infrared to Gamma Rays被引频次学科排名<br> http://figure.impactfactor.cn/tcr/?ISSN=BK0163603<br><br> <br><br>书目名称Astronomical Polarisation from the Infrared to Gamma Rays年度引用<br> http://figure.impactfactor.cn/ii/?ISSN=BK0163603<br><br> <br><br>书目名称Astronomical Polarisation from the Infrared to Gamma Rays年度引用学科排名<br> http://figure.impactfactor.cn/iir/?ISSN=BK0163603<br><br> <br><br>书目名称Astronomical Polarisation from the Infrared to Gamma Rays读者反馈<br> http://figure.impactfactor.cn/5y/?ISSN=BK0163603<br><br> <br><br>书目名称Astronomical Polarisation from the Infrared to Gamma Rays读者反馈学科排名<br> http://figure.impactfactor.cn/5yr/?ISSN=BK0163603<br><br> <br><br>
MUT
发表于 2025-3-21 20:31:39
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Lacunar-Stroke
发表于 2025-3-22 04:22:54
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种子
发表于 2025-3-22 07:58:00
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浅滩
发表于 2025-3-22 12:15:30
Gamma-Ray Polarimetry,c nuclei, gamma-ray bursts, black hole binaries, pulsars, etc. The linear polarisation information of gamma-ray sources is measured usingCompton scattering up to a few MeV and the conversion of high-energy photons to electron–positron pairs at higher energies. Thanks to the development of gamma-ray
cinder
发表于 2025-3-22 15:35:55
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机密
发表于 2025-3-22 18:50:38
Spectropolarimetry of Stars Across the H-R Diagram,o understand the origin, evolution, and structure of stellar magnetic fields in stars of different mass at different evolutionary stages. In this chapter we discuss recent measurements together with the underlying assumptions in the interpretation of data and the requirements, both observational and
侵略主义
发表于 2025-3-23 00:33:50
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pineal-gland
发表于 2025-3-23 02:28:10
Polarimetry of Binary Systems: Polars, Magnetic CVs, XRBs,rvation. Indeed, radiation processes such as scattering by free electrons in the hot plasma above accretion discs, cyclotron emission by mildly relativistic electrons in the accretion shocks on the surface of highly magnetic white dwarfs and the optically thin synchrotron emission from jets can be o
Indent
发表于 2025-3-23 05:51:36
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