deliberate
发表于 2025-3-21 17:13:36
书目名称Diffuse Radio Foregrounds影响因子(影响力)<br> http://figure.impactfactor.cn/if/?ISSN=BK0278999<br><br> <br><br>书目名称Diffuse Radio Foregrounds影响因子(影响力)学科排名<br> http://figure.impactfactor.cn/ifr/?ISSN=BK0278999<br><br> <br><br>书目名称Diffuse Radio Foregrounds网络公开度<br> http://figure.impactfactor.cn/at/?ISSN=BK0278999<br><br> <br><br>书目名称Diffuse Radio Foregrounds网络公开度学科排名<br> http://figure.impactfactor.cn/atr/?ISSN=BK0278999<br><br> <br><br>书目名称Diffuse Radio Foregrounds被引频次<br> http://figure.impactfactor.cn/tc/?ISSN=BK0278999<br><br> <br><br>书目名称Diffuse Radio Foregrounds被引频次学科排名<br> http://figure.impactfactor.cn/tcr/?ISSN=BK0278999<br><br> <br><br>书目名称Diffuse Radio Foregrounds年度引用<br> http://figure.impactfactor.cn/ii/?ISSN=BK0278999<br><br> <br><br>书目名称Diffuse Radio Foregrounds年度引用学科排名<br> http://figure.impactfactor.cn/iir/?ISSN=BK0278999<br><br> <br><br>书目名称Diffuse Radio Foregrounds读者反馈<br> http://figure.impactfactor.cn/5y/?ISSN=BK0278999<br><br> <br><br>书目名称Diffuse Radio Foregrounds读者反馈学科排名<br> http://figure.impactfactor.cn/5yr/?ISSN=BK0278999<br><br> <br><br>
COM
发表于 2025-3-21 21:09:50
https://doi.org/10.1007/978-94-009-6726-7In this chapter we describe the processing of the .data and other full sky maps for the polarisation analysis.
水土
发表于 2025-3-22 02:43:27
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pellagra
发表于 2025-3-22 07:45:08
Red Cell Metabolism and FunctionIn this chapter we study the AME in the Lynds Dark Nebula (LDN) 1780. Here, we have detected AME using interferometric observations at 31 GHz with 6. angular resolution (Vidal et al. .).
Emmenagogue
发表于 2025-3-22 11:47:05
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Incisor
发表于 2025-3-22 15:28:12
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Incisor
发表于 2025-3-22 18:10:39
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Paradox
发表于 2025-3-23 00:36:01
,, Polarised Filaments,At frequencies up to a few GHz, the total radio sky brightness is dominated by the diffuse Galactic synchrotron radiation, where cosmic rays (CR) electrons and positrons spiralling
STYX
发表于 2025-3-23 01:45:22
,AME in LDN 1780,In this chapter we study the AME in the Lynds Dark Nebula (LDN) 1780. Here, we have detected AME using interferometric observations at 31 GHz with 6. angular resolution (Vidal et al. .).
transplantation
发表于 2025-3-23 08:49:57
Conclusions and Future Work,In this thesis we have studied the Galactic emission in the 23–43 GHz frequency range, focusing on the diffuse polarised emission and on the anomalous microwave emission.