Initial Results from the Fast Imaging Solar Spectrograph (FISS) [electronic resource] /
Chae, Jongchul.editor.
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.
"Previously published in Solar Physics Volume 288, Issue 1, 2013 and Volume 289, Issue 11, 2014".
Includes bibliographical references at the end of each chapters.
Fast Imaging Solar Spectrograph of the 1.6 Meter New Solar Telescope at Big Bear Solar Observatory -- FISS Observations of Vertical Motion of Plasma in Tiny Pores -- Velocities and Temperatures of an Ellerman Bomb and Its Associated Features -- Connection Between Chromospheric Events and Photospheric Dynamics -- Chromospheric Sunspot Oscillations in Hα and Ca II 8542 Å -- Doppler Shifts of the Hα Line and the Ca II 854.2 nm Line in a Quiet Region of the Sun Observed with the FISS/NST -- Temperature of Solar Prominences Obtained with the Fast Imaging Solar Spectrograph on the 1.6 m New Solar Telescope at the Big Bear Solar Observatory -- Active Region Coronal Rain Event Observed by the Fast Imaging Solar Spectrograph on the NST.
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.
Space sciences.
Physical measurements.
Measurement   .
Spectroscopy.
Microscopy.
Space Sciences (including Extraterrestrial Physics, Space Exploration and Astronautics).
Measurement Science and Instrumentation.
Spectroscopy and Microscopy.