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MARTIŠEK, K. DRUCKMÜLLEROVÁ, H.
Original Title
A Numerical Method for the Visualization of the Fe XIV Emission in the Solar Corona Using Broadband Filters
Type
journal article in Web of Science
Language
English
Original Abstract
The goal of this article is to demonstrate how the emission from the Fe XIV 530.3 nm coronal emission line, also known as the green line, can be extracted from images taken during total solar eclipses with commercially available color cameras. This concept is technically feasible because Fe XIV is the brightest optical emission line in the inner corona, and because the sensors of these cameras are retrofitted with a standard Bayer mask, namely, a square grid of spectrally broad (about 100 nm) green, blue, and red filters in the ratio of 2:1:1. The technique presented here, and developed for this purpose, yields qualitatively accurate Fe XIV images, as tested by comparing with Fe XIV eclipse images taken with a 0.15 nm narrow-bandpass filter. While this approach cannot replace narrow-bandpass Fe XIV images for quantitative studies of the corona, it provides a simple and affordable tool for studying the morphology of coronal structures emitting preferentially at the peak ionization temperature of Fe XIV, namely, 1.8 x 10^6 K.
Keywords
methods: data analysis – methods: numerical – Sun: corona – techniques: image processing
Authors
MARTIŠEK, K.; DRUCKMÜLLEROVÁ, H.
RIV year
2011
Released
23. 11. 2011
Publisher
IOP Publising
Location
Bristol, UK
ISBN
0067-0049
Periodical
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
Year of study
197
Number
2
State
United States of America
Pages from
23
Pages to
29
Pages count
7
BibTex
@article{BUT75495, author="Karel {Martišek} and Hana {Druckmüllerová}", title="A Numerical Method for the Visualization of the Fe XIV Emission in the Solar Corona Using Broadband Filters", journal="ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES", year="2011", volume="197", number="2", pages="23--29", issn="0067-0049" }