Denial
发表于 2025-3-21 19:17:29
书目名称Solar Eclipses and the Ionosphere影响因子(影响力)<br> http://figure.impactfactor.cn/if/?ISSN=BK0871358<br><br> <br><br>书目名称Solar Eclipses and the Ionosphere影响因子(影响力)学科排名<br> http://figure.impactfactor.cn/ifr/?ISSN=BK0871358<br><br> <br><br>书目名称Solar Eclipses and the Ionosphere网络公开度<br> http://figure.impactfactor.cn/at/?ISSN=BK0871358<br><br> <br><br>书目名称Solar Eclipses and the Ionosphere网络公开度学科排名<br> http://figure.impactfactor.cn/atr/?ISSN=BK0871358<br><br> <br><br>书目名称Solar Eclipses and the Ionosphere被引频次<br> http://figure.impactfactor.cn/tc/?ISSN=BK0871358<br><br> <br><br>书目名称Solar Eclipses and the Ionosphere被引频次学科排名<br> http://figure.impactfactor.cn/tcr/?ISSN=BK0871358<br><br> <br><br>书目名称Solar Eclipses and the Ionosphere年度引用<br> http://figure.impactfactor.cn/ii/?ISSN=BK0871358<br><br> <br><br>书目名称Solar Eclipses and the Ionosphere年度引用学科排名<br> http://figure.impactfactor.cn/iir/?ISSN=BK0871358<br><br> <br><br>书目名称Solar Eclipses and the Ionosphere读者反馈<br> http://figure.impactfactor.cn/5y/?ISSN=BK0871358<br><br> <br><br>书目名称Solar Eclipses and the Ionosphere读者反馈学科排名<br> http://figure.impactfactor.cn/5yr/?ISSN=BK0871358<br><br> <br><br>
Osteons
发表于 2025-3-21 22:35:56
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ALB
发表于 2025-3-22 02:52:01
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Parabola
发表于 2025-3-22 07:50:32
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自负的人
发表于 2025-3-22 08:50:04
Direct Rocket Measurements of the Ionosphere during the Solar Eclipse of November 12,1966 site in southern Brazil. Previously reported results indicate unexpectedly large decreases in the electron density at eclipse totality in the vicinity of 80 km. altitude. Also, measurements with the blunt probe technique showed an unexpectedly large decrease in positive ion density during the cours
CORD
发表于 2025-3-22 13:40:21
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勋章
发表于 2025-3-22 17:43:38
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轻浮思想
发表于 2025-3-23 00:12:12
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食草
发表于 2025-3-23 02:44:44
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极大的痛苦
发表于 2025-3-23 07:05:30
Distribution of X-Ray Emission from the Sun Deduced from Measurements of Ionospheric Absorptionere made from several points along the central line of the path of the eclipse. Solar flux was measured at various frequencies in the cm and mm bands.All the data obtained during the eclipse showed characteristic variations in flux related to local active sources on the solar disk.Fig. 1 shows the d