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Title: Calculated resonance line profiles of [Mg II], [C II], and [Si IV] in the solar atmosphere

Abstract

NASA's Interface Region Imaging Spectrograph space mission, launched 2013 June 27, is intended to study the structure of the solar chromosphere and the transition region between the chromosphere and corona. The spectral lines to be observed include the Mg II k line at 2796.5 Å, the C II 1334.5 Å line, and the Si IV line at 1393.8 Å, which are formed in the middle chromosphere, the upper chromosphere, and the lower transition region, respectively. Here we calculate the profiles of these lines from four models of the solar atmosphere, intended to represent the faint and mean internetwork, a network lane, and bright network. We show how the profiles change from the center of the solar disk toward the limb of the Sun and in response to outflows and inflows. These results are intended to cover the range of expected quiet-Sun observations and assist in their interpretation. We expect that the observations will lead to improvements in the models, which can then be used to estimate the required non-radiative heating in the different regions.

Authors:
;  [1];  [2]
  1. Smithsonian Astrophysical Observatory, 60 Garden Street, Cambridge, MA 02138 (United States)
  2. Department of Atmospheric, Oceanic and Space Sciences, University of Michigan, Ann Arbor, MI 48109 (United States)
Publication Date:
OSTI Identifier:
22348432
Resource Type:
Journal Article
Journal Name:
Astrophysical Journal
Additional Journal Information:
Journal Volume: 779; Journal Issue: 2; Other Information: Country of input: International Atomic Energy Agency (IAEA); Journal ID: ISSN 0004-637X
Country of Publication:
United States
Language:
English
Subject:
79 ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; CARBON; CHROMOSPHERE; COSMOLOGY; INTERFACES; LIMBS; MAGNESIUM; NASA; SILICON; SOLAR ATMOSPHERE; SPACE; SUN

Citation Formats

Avrett, E., McKillop, S., and Landi, E. Calculated resonance line profiles of [Mg II], [C II], and [Si IV] in the solar atmosphere. United States: N. p., 2013. Web. doi:10.1088/0004-637X/779/2/155.
Avrett, E., McKillop, S., & Landi, E. Calculated resonance line profiles of [Mg II], [C II], and [Si IV] in the solar atmosphere. United States. https://doi.org/10.1088/0004-637X/779/2/155
Avrett, E., McKillop, S., and Landi, E. 2013. "Calculated resonance line profiles of [Mg II], [C II], and [Si IV] in the solar atmosphere". United States. https://doi.org/10.1088/0004-637X/779/2/155.
@article{osti_22348432,
title = {Calculated resonance line profiles of [Mg II], [C II], and [Si IV] in the solar atmosphere},
author = {Avrett, E. and McKillop, S. and Landi, E.},
abstractNote = {NASA's Interface Region Imaging Spectrograph space mission, launched 2013 June 27, is intended to study the structure of the solar chromosphere and the transition region between the chromosphere and corona. The spectral lines to be observed include the Mg II k line at 2796.5 Å, the C II 1334.5 Å line, and the Si IV line at 1393.8 Å, which are formed in the middle chromosphere, the upper chromosphere, and the lower transition region, respectively. Here we calculate the profiles of these lines from four models of the solar atmosphere, intended to represent the faint and mean internetwork, a network lane, and bright network. We show how the profiles change from the center of the solar disk toward the limb of the Sun and in response to outflows and inflows. These results are intended to cover the range of expected quiet-Sun observations and assist in their interpretation. We expect that the observations will lead to improvements in the models, which can then be used to estimate the required non-radiative heating in the different regions.},
doi = {10.1088/0004-637X/779/2/155},
url = {https://www.osti.gov/biblio/22348432}, journal = {Astrophysical Journal},
issn = {0004-637X},
number = 2,
volume = 779,
place = {United States},
year = {Fri Dec 20 00:00:00 EST 2013},
month = {Fri Dec 20 00:00:00 EST 2013}
}