EFFCT
发表于 2025-3-21 17:15:50
书目名称Astrophysics in the Extreme Ultraviolet影响因子(影响力)<br> http://impactfactor.cn/2024/if/?ISSN=BK0163701<br><br> <br><br>书目名称Astrophysics in the Extreme Ultraviolet影响因子(影响力)学科排名<br> http://impactfactor.cn/2024/ifr/?ISSN=BK0163701<br><br> <br><br>书目名称Astrophysics in the Extreme Ultraviolet网络公开度<br> http://impactfactor.cn/2024/at/?ISSN=BK0163701<br><br> <br><br>书目名称Astrophysics in the Extreme Ultraviolet网络公开度学科排名<br> http://impactfactor.cn/2024/atr/?ISSN=BK0163701<br><br> <br><br>书目名称Astrophysics in the Extreme Ultraviolet被引频次<br> http://impactfactor.cn/2024/tc/?ISSN=BK0163701<br><br> <br><br>书目名称Astrophysics in the Extreme Ultraviolet被引频次学科排名<br> http://impactfactor.cn/2024/tcr/?ISSN=BK0163701<br><br> <br><br>书目名称Astrophysics in the Extreme Ultraviolet年度引用<br> http://impactfactor.cn/2024/ii/?ISSN=BK0163701<br><br> <br><br>书目名称Astrophysics in the Extreme Ultraviolet年度引用学科排名<br> http://impactfactor.cn/2024/iir/?ISSN=BK0163701<br><br> <br><br>书目名称Astrophysics in the Extreme Ultraviolet读者反馈<br> http://impactfactor.cn/2024/5y/?ISSN=BK0163701<br><br> <br><br>书目名称Astrophysics in the Extreme Ultraviolet读者反馈学科排名<br> http://impactfactor.cn/2024/5yr/?ISSN=BK0163701<br><br> <br><br>
strdulate
发表于 2025-3-21 20:49:37
Flex with Photoshop and Illustrator,exposure time, we have measured over 200 emission features with S/N ≥ 3.0 in the summed spectrum. We report here initial results from the analysis of this spectrum. We can now identify lines of Fe VIII and X-XIV, as well as a number of electron density and abundance diagnostic lines.
运动吧
发表于 2025-3-22 02:03:30
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切掉
发表于 2025-3-22 04:39:09
Dissecting the EUV Spectrum of Capellaexposure time, we have measured over 200 emission features with S/N ≥ 3.0 in the summed spectrum. We report here initial results from the analysis of this spectrum. We can now identify lines of Fe VIII and X-XIV, as well as a number of electron density and abundance diagnostic lines.
Explicate
发表于 2025-3-22 12:27:43
Are Some Stellar Coronae Optically Thick?nse, hot flare plasmas. The electron densities of the 5–15 MK component are some three orders of magnitude higher than typical of the solar-like component around 2 MK; the volume filling factors of the hot components are therefore expected to be relatively small.
inspiration
发表于 2025-3-22 14:43:02
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induct
发表于 2025-3-22 20:13:02
Foundation Flash CS4 for DesignersI review some of the major achievements of the . extreme-ultraviolet all-sky survey, including the results of the recently completed 2RE source catalogue and associated study of temporal variability in EUV sources.
性别
发表于 2025-3-22 22:58:55
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Deduct
发表于 2025-3-23 03:17:13
Introducing Flex and Flex Builder 3,“Yes, it will be a long time before people know what I know. How much of iron and other metal there is in the sun and the stars is easy to find out, but anything which exposes our swinishness is difficult, terribly difficult” (Tolstoy 1889).
饶舌的人
发表于 2025-3-23 09:10:48
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