gratuity
发表于 2025-3-21 17:06:02
书目名称Ionospheric Modeling影响因子(影响力)<br> http://impactfactor.cn/2024/if/?ISSN=BK0475240<br><br> <br><br>书目名称Ionospheric Modeling影响因子(影响力)学科排名<br> http://impactfactor.cn/2024/ifr/?ISSN=BK0475240<br><br> <br><br>书目名称Ionospheric Modeling网络公开度<br> http://impactfactor.cn/2024/at/?ISSN=BK0475240<br><br> <br><br>书目名称Ionospheric Modeling网络公开度学科排名<br> http://impactfactor.cn/2024/atr/?ISSN=BK0475240<br><br> <br><br>书目名称Ionospheric Modeling被引频次<br> http://impactfactor.cn/2024/tc/?ISSN=BK0475240<br><br> <br><br>书目名称Ionospheric Modeling被引频次学科排名<br> http://impactfactor.cn/2024/tcr/?ISSN=BK0475240<br><br> <br><br>书目名称Ionospheric Modeling年度引用<br> http://impactfactor.cn/2024/ii/?ISSN=BK0475240<br><br> <br><br>书目名称Ionospheric Modeling年度引用学科排名<br> http://impactfactor.cn/2024/iir/?ISSN=BK0475240<br><br> <br><br>书目名称Ionospheric Modeling读者反馈<br> http://impactfactor.cn/2024/5y/?ISSN=BK0475240<br><br> <br><br>书目名称Ionospheric Modeling读者反馈学科排名<br> http://impactfactor.cn/2024/5yr/?ISSN=BK0475240<br><br> <br><br>
极肥胖
发表于 2025-3-21 21:50:26
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EXCEL
发表于 2025-3-22 04:03:02
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Biguanides
发表于 2025-3-22 08:39:09
The Role of Vibrationally Excited Nitrogen in the Ionosphere,ere and an aurora are presented. The connection between the excited species and the 4.26-.m radiation intensities is considered. The models for the rate coefficient of the reaction of O. with N. and the electron density decrease resulting from N. in the F region are discussed.
adjacent
发表于 2025-3-22 09:16:09
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Inscrutable
发表于 2025-3-22 15:51:34
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坦白
发表于 2025-3-22 19:51:30
,Modelling of Neutral-Gas Releases into the Earth’s Ionosphere,phere-plasmasphere coupling, in which the transfer equations for charged components are integrated along geomagnetic field lines. The purpose of the model is to calculate the electron density and temperature, ion composition and emission of a disturbed region in the 6300 Å line at ionospheric and plasmaspheric heights.
Anthology
发表于 2025-3-22 22:14:41
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Aggressive
发表于 2025-3-23 04:47:16
,Quasilinear Heating of Electrons in the Earth’s Plasmasphere,crease, and this must lead to an increase in electron temperature in lower-lying plasmaspheric regions and in the subauroral ionosphere. A quantitative estimation of the electron temperature for the ‘hot zone’, made in this paper, is consistent with available experimental data.
Chandelier
发表于 2025-3-23 05:37:18
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