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Titlebook: Initial Results from the Fast Imaging Solar Spectrograph (FISS); Jongchul Chae Book 2015 Springer International Publishing Switzerland 201

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发表于 2025-3-21 16:59:59 | 显示全部楼层 |阅读模式
书目名称Initial Results from the Fast Imaging Solar Spectrograph (FISS)
编辑Jongchul Chae
视频video
概述Describes the instruments and initial results of the Fast Imaging Solar Spectrograph (FISS) at the Big Bear Solar Observatory.Discusses the connection between chromospheric events and photospheric dyn
图书封面Titlebook: Initial Results from the Fast Imaging Solar Spectrograph (FISS);  Jongchul Chae Book 2015 Springer International Publishing Switzerland 201
描述.Describes the instruments and initial results of the Fast Imaging Solar Spectrograph (FISS) at the Big Bear Solar Observatory..This collection of papers describes the instrument and initial results obtained from the Fast Imaging Solar Spectrograph (FISS), one of the post-focus instruments of the 1.6 meter New Solar Telescope at the Big Bear Solar Observatory. The FISS primarily aims at investigating structures and dynamics of chromospheric features. This instrument is a dual-band Echelle spectrograph optimized for the simultaneous recording of the H I 656.3 nm band and the Ca II 854.2 nm band. The imaging is done with the fast raster scan realized by the linear motion of a two-mirror scanner, and its quality is determined by the performance of the adaptive optics of the telescope..These papers illustrate the capability of the early FISS observations in the study of chromospheric features. Since the imaging quality has been improved a lot with the advance of the adaptive optics, one can obtain much better data with the current FISS observations..This volume is aimed at graduate students and researchers working in the field of solar physics and space sciences..Originally published i
出版日期Book 2015
关键词Big Bear Solar Observatory; Ca II 854; 2 nm Line; Dynamics Chromospheric Features; FISS Instruments; Fast
版次1
doihttps://doi.org/10.1007/978-3-319-12123-9
isbn_softcover978-3-319-38584-6
isbn_ebook978-3-319-12123-9
copyrightSpringer International Publishing Switzerland 2015
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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 suns
发表于 2025-3-22 23:17:46 | 显示全部楼层
,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
发表于 2025-3-23 05:03:35 | 显示全部楼层
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
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