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Initial results from the Fast Imagin...

Chae, Jongchul.

Initial results from the Fast Imaging Solar Spectrograph (FISS)[electronic resource] /

紀錄類型:	書目-語言資料,印刷品 : Monograph/item
杜威分類號:	523.70287
書名/作者:	Initial results from the Fast Imaging Solar Spectrograph (FISS)/ edited by Jongchul Chae.
其他作者:	Chae, Jongchul.
出版者:	Cham : : Springer International Publishing :, 2015.
面頁冊數:	vii, 136 p. : : ill., digital ;; 24 cm.
Contained By:	Springer eBooks
標題:	Spectrum, Solar.
標題:	Astronomical spectroscopy.
標題:	Physics.
標題:	Extraterrestrial Physics, Space Sciences.
標題:	Measurement Science and Instrumentation.
標題:	Spectroscopy and Microscopy.
ISBN:	9783319121239 (electronic bk.)
ISBN:	9783319121222 (paper)
摘要、提要註:	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 in Solar Physics, Vol. 288, Issue 1, 2013, and Vol. 289, Issue 11, 2014.
電子資源:	http://dx.doi.org/10.1007/978-3-319-12123-9

Initial results from the Fast Imaging Solar Spectrograph (FISS)[electronic resource] /
Initial results from the Fast Imaging Solar Spectrograph (FISS)[electronic resource] /edited by Jongchul Chae. - Cham :Springer International Publishing :2015. - vii, 136 p. :ill., digital ;24 cm.

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 in Solar Physics, Vol. 288, Issue 1, 2013, and Vol. 289, Issue 11, 2014.

ISBN: 9783319121239 (electronic bk.)

Standard No.: 10.1007/978-3-319-12123-9doiSubjects--Topical Terms:

394300
Spectrum, Solar.

LC Class. No.: QB551

Dewey Class. No.: 523.70287

Initial results from the Fast Imaging Solar Spectrograph (FISS)[electronic resource] /
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520 $a 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 in Solar Physics, Vol. 288, Issue 1, 2013, and Vol. 289, Issue 11, 2014.
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650 0 $a Astronomical spectroscopy. $3 512238
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