孵化 发表于 2025-3-21 16:59:59
书目名称Initial Results from the Fast Imaging Solar Spectrograph (FISS)影响因子(影响力)<br> http://figure.impactfactor.cn/if/?ISSN=BK0466491<br><br> <br><br>书目名称Initial Results from the Fast Imaging Solar Spectrograph (FISS)影响因子(影响力)学科排名<br> http://figure.impactfactor.cn/ifr/?ISSN=BK0466491<br><br> <br><br>书目名称Initial Results from the Fast Imaging Solar Spectrograph (FISS)网络公开度<br> http://figure.impactfactor.cn/at/?ISSN=BK0466491<br><br> <br><br>书目名称Initial Results from the Fast Imaging Solar Spectrograph (FISS)网络公开度学科排名<br> http://figure.impactfactor.cn/atr/?ISSN=BK0466491<br><br> <br><br>书目名称Initial Results from the Fast Imaging Solar Spectrograph (FISS)被引频次<br> http://figure.impactfactor.cn/tc/?ISSN=BK0466491<br><br> <br><br>书目名称Initial Results from the Fast Imaging Solar Spectrograph (FISS)被引频次学科排名<br> http://figure.impactfactor.cn/tcr/?ISSN=BK0466491<br><br> <br><br>书目名称Initial Results from the Fast Imaging Solar Spectrograph (FISS)年度引用<br> http://figure.impactfactor.cn/ii/?ISSN=BK0466491<br><br> <br><br>书目名称Initial Results from the Fast Imaging Solar Spectrograph (FISS)年度引用学科排名<br> http://figure.impactfactor.cn/iir/?ISSN=BK0466491<br><br> <br><br>书目名称Initial Results from the Fast Imaging Solar Spectrograph (FISS)读者反馈<br> http://figure.impactfactor.cn/5y/?ISSN=BK0466491<br><br> <br><br>书目名称Initial Results from the Fast Imaging Solar Spectrograph (FISS)读者反馈学科排名<br> http://figure.impactfactor.cn/5yr/?ISSN=BK0466491<br><br> <br><br>amnesia 发表于 2025-3-21 21:16:47
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,Chromospheric Sunspot Oscillations in Hα and Ca , 8542 Å,roscopy in Hα and Ca . 8542 Å with the . (FISS) at the 1.6 meter . at the Big Bear Solar Observatory. A bisector method is applied to spectral observations to construct chromospheric Doppler-velocity maps. Temporal-sequence analysis of these shows enhanced high-frequency oscillations inside the sunsnegotiable 发表于 2025-3-22 23:17:46
,Doppler Shifts of the Hα Line and the Ca , 854.2 nm Line in a Quiet Region of the Sun Observed withea of 16″×40″ was observed for about half an hour with the Fast Imaging Solar Spectrograph (FISS) of the 1.6 meter New Solar Telescope (NST) at Big Bear Solar Observatory. The observed area contains a network region and an internetwork region, and identified in the network region are fibrils and bri元音 发表于 2025-3-23 05:03:35
Temperature of Solar Prominences Obtained with the Fast Imaging Solar Spectrograph on the 1.6 m New determine the temperature of the prominence material, we applied a nonlinear least-squares fitting of the radiative transfer model. From the Doppler broadening of the Hα and Ca . lines, we determined the temperature and nonthermal velocity separately. The ranges of temperature and nonthermal veloci后退 发表于 2025-3-23 09:35:42
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