INEPT
发表于 2025-3-21 19:25:16
书目名称Coronal Disturbances影响因子(影响力)<br> http://impactfactor.cn/2024/if/?ISSN=BK0238289<br><br> <br><br>书目名称Coronal Disturbances影响因子(影响力)学科排名<br> http://impactfactor.cn/2024/ifr/?ISSN=BK0238289<br><br> <br><br>书目名称Coronal Disturbances网络公开度<br> http://impactfactor.cn/2024/at/?ISSN=BK0238289<br><br> <br><br>书目名称Coronal Disturbances网络公开度学科排名<br> http://impactfactor.cn/2024/atr/?ISSN=BK0238289<br><br> <br><br>书目名称Coronal Disturbances被引频次<br> http://impactfactor.cn/2024/tc/?ISSN=BK0238289<br><br> <br><br>书目名称Coronal Disturbances被引频次学科排名<br> http://impactfactor.cn/2024/tcr/?ISSN=BK0238289<br><br> <br><br>书目名称Coronal Disturbances年度引用<br> http://impactfactor.cn/2024/ii/?ISSN=BK0238289<br><br> <br><br>书目名称Coronal Disturbances年度引用学科排名<br> http://impactfactor.cn/2024/iir/?ISSN=BK0238289<br><br> <br><br>书目名称Coronal Disturbances读者反馈<br> http://impactfactor.cn/2024/5y/?ISSN=BK0238289<br><br> <br><br>书目名称Coronal Disturbances读者反馈学科排名<br> http://impactfactor.cn/2024/5yr/?ISSN=BK0238289<br><br> <br><br>
充满人
发表于 2025-3-21 21:24:41
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PAN
发表于 2025-3-22 01:31:00
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肉体
发表于 2025-3-22 07:49:55
Bulk growth of widegap II–VI single crystalson whether the electrons propagate along the axes of coronal streamers. Several important burst properties appear to be significantly affected by ray scattering on small-scale size density irregularities in the corona.
发生
发表于 2025-3-22 11:36:27
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champaign
发表于 2025-3-22 16:44:45
II–VI electroluminescent devicesd the accelerated electrons provide the energy necessary for all the observed electromagnetic emissions produced during the flash phase of small solar flares. Models of the impulsive phase emissions in which energetic electrons play a prominant role are examined and crucial tests to check the accuracy of these models are indicated (Table IV).
champaign
发表于 2025-3-22 19:31:38
Bulk growth of widegap II–VI single crystalsions were joined by extended field lines with the acceleration mechanism somewhere in between. Although nothing was visible in Hα (such as surges or post flare ejections) that would indicate connecting field lines, higher coronal structures could explain the similarity in hard X-rays from two separate regions.
ESO
发表于 2025-3-22 21:29:52
Distribution of Circularly Polarized Emission across the Solar Disk at λ =4.3cmd a ‘neutral line’ divide the two polarized hemispheres, showing a contour that depends strongly on the presence of active centres and on their displacement with solar rotation. This suggest that the polarized features are strongly controlled, if not completely, by the presence of photospheric underlying magnetic areas.
尖酸一点
发表于 2025-3-23 01:32:16
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Lineage
发表于 2025-3-23 08:29:12
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