Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/7460
Title: Characteristics of the solar coronal line profiles from Fabry–Perot interferometric observations
Authors: Maya Prabhakar
Raju, K. P
Chandrasekhar, T
Keywords: Corona, E;Eclipse observations;Spectral line, broadening;Spectrum, visible
Issue Date: Mar-2019
Publisher: Springer
Citation: Solar Physics, Vol. 294, No. 3, 26
Abstract: This article reports the analysis of a set of Fabry–Perot interferograms that were studied to probe the physical parameters of the inner solar corona. The observations were carried out in the coronal green line, Fe xiv 5302.86 Å, during the total solar eclipse of 21 June 2001 that occurred in Lusaka, Zambia. The study was performed in the radial range of 1.1--1.5 R⊙ and examines the Doppler velocity, half-width, centroid, and asymmetry and their correlations with each other at various points in the corona. We found that 59% of the line profiles are blueshifted, 34% are single components, and only 7% are redshifted. The variations in half-width and Doppler velocity with respect to coronal height have a large scatter and show no significant changes. We found that the variation in half-width with Doppler velocity or centroid follows a parabolic trend with a weak correlation, whereas the relation between half-width and asymmetry is inconclusive. These results may provide more insight into the coronal dynamics and help in understanding the physical problems in the corona.
Description: Restricted Access
The original publication is available at springerlink.com
URI: http://hdl.handle.net/2248/7460
ISSN: 1573-093X
???metadata.dc.rights???: © Springer
???metadata.dc.relation.uri???: https://doi.org/10.1007/s11207-019-1409-7
Appears in Collections:IIAP Publications

Files in This Item:
File Description SizeFormat 
Characteristics of the Solar Coronal Line Profiles from Fabry Perot Interferometric Observations.pdfRestricted Access807 kBAdobe PDFView/Open    Request a copy


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.