ODDS
发表于 2025-3-21 19:35:52
书目名称Energy Storage and Release through the Solar Activity Cycle影响因子(影响力)<br> http://impactfactor.cn/if/?ISSN=BK0310424<br><br> <br><br>书目名称Energy Storage and Release through the Solar Activity Cycle影响因子(影响力)学科排名<br> http://impactfactor.cn/ifr/?ISSN=BK0310424<br><br> <br><br>书目名称Energy Storage and Release through the Solar Activity Cycle网络公开度<br> http://impactfactor.cn/at/?ISSN=BK0310424<br><br> <br><br>书目名称Energy Storage and Release through the Solar Activity Cycle网络公开度学科排名<br> http://impactfactor.cn/atr/?ISSN=BK0310424<br><br> <br><br>书目名称Energy Storage and Release through the Solar Activity Cycle被引频次<br> http://impactfactor.cn/tc/?ISSN=BK0310424<br><br> <br><br>书目名称Energy Storage and Release through the Solar Activity Cycle被引频次学科排名<br> http://impactfactor.cn/tcr/?ISSN=BK0310424<br><br> <br><br>书目名称Energy Storage and Release through the Solar Activity Cycle年度引用<br> http://impactfactor.cn/ii/?ISSN=BK0310424<br><br> <br><br>书目名称Energy Storage and Release through the Solar Activity Cycle年度引用学科排名<br> http://impactfactor.cn/iir/?ISSN=BK0310424<br><br> <br><br>书目名称Energy Storage and Release through the Solar Activity Cycle读者反馈<br> http://impactfactor.cn/5y/?ISSN=BK0310424<br><br> <br><br>书目名称Energy Storage and Release through the Solar Activity Cycle读者反馈学科排名<br> http://impactfactor.cn/5yr/?ISSN=BK0310424<br><br> <br><br>
syncope
发表于 2025-3-22 00:08:52
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Lineage
发表于 2025-3-22 03:03:49
Coronal Shock Waves, EUV Waves, and Their Relation to CMEs. II. Modeling MHD Shock Wave Propagationof the modeling of the propagation of shock-associated extreme-ultraviolet (EUV) waves as well as Moreton waves along the solar surface in the simplest solar corona model. The calculations reveal deceleration and lengthening of the waves. In contrast, waves considered in the linear approximation keep their length unchanged and slightly accelerate.
松软
发表于 2025-3-22 07:28:43
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代替
发表于 2025-3-22 09:51:45
mission and fundamental radio physicsFor nearly sixty years, radio observations have provided a unique insight into the physics of the active and quiescent solar atmosphere. Thanks to the variety of emission mechanisms and to the large altitude range available to observations, fundamental plasma par
流动性
发表于 2025-3-22 13:17:03
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流动性
发表于 2025-3-22 17:02:43
James K. Whitesell,Mark A. Mintonof the modeling of the propagation of shock-associated extreme-ultraviolet (EUV) waves as well as Moreton waves along the solar surface in the simplest solar corona model. The calculations reveal deceleration and lengthening of the waves. In contrast, waves considered in the linear approximation keep their length unchanged and slightly accelerate.
异端邪说下
发表于 2025-3-23 01:12:52
https://doi.org/10.1007/978-3-662-10051-6nection between the parameters of the radio emission from three different layers of the solar atmosphere and the solar wind velocity near the Earth’s orbit was discovered. Such a connection is suggestive of a common mechanism of solar wind acceleration from chromospheric heights to the upper corona.
稀释前
发表于 2025-3-23 03:32:15
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Keratectomy
发表于 2025-3-23 08:53:04
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