Imaging the structure of the low K‐corona

The first 2‐D distributions of the polarization angle and of the relative color index for the K‐corona of 29 March 2006 are presented. The distributions illustrate the efficiency of the total solar eclipse approach for high‐precision measurements of the K‐corona continuum in the range

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Bibliographische Detailangaben
Veröffentlicht in:	Journal of geophysical research. Space physics 2017-01, Vol.122 (1), p.77-88
Hauptverfasser:	Kim, I. S., Nasonova, L. P., Lisin, D. V., Popov, V. V., Krusanova, N. L.
Format:	Artikel
Sprache:	eng
Schlagworte:	2‐D linear polarimetry 2‐D relative color index imaging Color Computing time Corona Coronagraphs Earth Eclipses Illumination Imaging K‐corona Mars Mars (planet) Mathematical analysis Mercury Mercury (planet) Moon Planets Polarimetry Polarization Recording Solar eclipses Solar physics total solar eclipses in space Venus
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Beschreibung
Zusammenfassung:	The first 2‐D distributions of the polarization angle and of the relative color index for the K‐corona of 29 March 2006 are presented. The distributions illustrate the efficiency of the total solar eclipse approach for high‐precision measurements of the K‐corona continuum in the range
ISSN:	2169-9380 2169-9402
DOI:	10.1002/2016JA022623