STRI
发表于 2025-3-21 19:50:27
书目名称Advances in Solar Research at Eclipses from Ground and from Space影响因子(影响力)<br> http://figure.impactfactor.cn/if/?ISSN=BK0149802<br><br> <br><br>书目名称Advances in Solar Research at Eclipses from Ground and from Space影响因子(影响力)学科排名<br> http://figure.impactfactor.cn/ifr/?ISSN=BK0149802<br><br> <br><br>书目名称Advances in Solar Research at Eclipses from Ground and from Space网络公开度<br> http://figure.impactfactor.cn/at/?ISSN=BK0149802<br><br> <br><br>书目名称Advances in Solar Research at Eclipses from Ground and from Space网络公开度学科排名<br> http://figure.impactfactor.cn/atr/?ISSN=BK0149802<br><br> <br><br>书目名称Advances in Solar Research at Eclipses from Ground and from Space被引频次<br> http://figure.impactfactor.cn/tc/?ISSN=BK0149802<br><br> <br><br>书目名称Advances in Solar Research at Eclipses from Ground and from Space被引频次学科排名<br> http://figure.impactfactor.cn/tcr/?ISSN=BK0149802<br><br> <br><br>书目名称Advances in Solar Research at Eclipses from Ground and from Space年度引用<br> http://figure.impactfactor.cn/ii/?ISSN=BK0149802<br><br> <br><br>书目名称Advances in Solar Research at Eclipses from Ground and from Space年度引用学科排名<br> http://figure.impactfactor.cn/iir/?ISSN=BK0149802<br><br> <br><br>书目名称Advances in Solar Research at Eclipses from Ground and from Space读者反馈<br> http://figure.impactfactor.cn/5y/?ISSN=BK0149802<br><br> <br><br>书目名称Advances in Solar Research at Eclipses from Ground and from Space读者反馈学科排名<br> http://figure.impactfactor.cn/5yr/?ISSN=BK0149802<br><br> <br><br>
最高峰
发表于 2025-3-21 23:50:42
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notification
发表于 2025-3-22 04:07:30
The Solar Corona: White Light Polarization and Modelling of the Large Scale Electron Density Distri loops and of streamers, extending up to several solar radii. The corona is separated from the chromosphere by a narrow transition region with very high temperature gradients. In this very thin layer, the temperature increases from about 10 000 K in the chromosphere up to millions K in the corona. T
CLEAR
发表于 2025-3-22 07:15:04
Observing the Solar Magnetic Field, than the line width. This corresponds to magnetic observations of chromosphere, prominences and the corona requiring more advanced technique as compared with the photosphere. Direct and indirect methods of magnetic researches in the upper solar atmosphere are briefly reviewed. The “signal-to-noise”
煞费苦心
发表于 2025-3-22 12:13:22
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paragon
发表于 2025-3-22 14:13:08
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古代
发表于 2025-3-22 19:26:21
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resilience
发表于 2025-3-22 23:23:04
Non-LTE Radiation Processes: Application to the Solar Corona,ocal thermodynamical equilibrium (NLTE), without appealing to any previous knowledge except a few basics of physics and spectroscopy. After recalling elementary notions of radiation transfer, the chapter is focussed on the computation of the level populations, the source function, the ionization sta
remission
发表于 2025-3-23 04:35:20
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主讲人
发表于 2025-3-23 08:11:53
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