Infrared solar physics from the South Pole

Infrared (IR) observations of the sun could greatly benefit from the quality of the South Pole as an IR site, and the potential for multi-day sequences of uninterrupted observations. A nearly continuous picture of the evolution of the magnetic field in solar active regions could be obtained using ve...

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Bibliographic Details
Main Author: Deming, Drake
Language:unknown
Published: 1989
Subjects:
92
South Pole
South pole
Online Access:http://ntrs.nasa.gov/search.jsp?R=19920039808
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record_format openpolar
spelling ftnasantrs:oai:casi.ntrs.nasa.gov:19920039808 2023-05-15T18:21:50+02:00 Infrared solar physics from the South Pole Deming, Drake Unclassified, Unlimited, Publicly available JAN 1, 1989 http://ntrs.nasa.gov/search.jsp?R=19920039808 unknown http://ntrs.nasa.gov/search.jsp?R=19920039808 Accession ID: 92A22432 Copyright Other Sources 92 1989 ftnasantrs 2012-02-15T19:28:29Z Infrared (IR) observations of the sun could greatly benefit from the quality of the South Pole as an IR site, and the potential for multi-day sequences of uninterrupted observations. A nearly continuous picture of the evolution of the magnetic field in solar active regions could be obtained using vector magnetographs, especially vector magnetographs which incorporate IR array detectors. Observations of the sun over a range of wavelengths in the IR continuum could also be used to study the vertical propagation characteristics of the solar p-mode oscillations. Other/Unknown Material South pole NASA Technical Reports Server (NTRS) South Pole
institution Open Polar
collection NASA Technical Reports Server (NTRS)
op_collection_id ftnasantrs
language unknown
topic 92
spellingShingle 92
Deming, Drake
Infrared solar physics from the South Pole
topic_facet 92
description Infrared (IR) observations of the sun could greatly benefit from the quality of the South Pole as an IR site, and the potential for multi-day sequences of uninterrupted observations. A nearly continuous picture of the evolution of the magnetic field in solar active regions could be obtained using vector magnetographs, especially vector magnetographs which incorporate IR array detectors. Observations of the sun over a range of wavelengths in the IR continuum could also be used to study the vertical propagation characteristics of the solar p-mode oscillations.
author Deming, Drake
author_facet Deming, Drake
author_sort Deming, Drake
title Infrared solar physics from the South Pole
title_short Infrared solar physics from the South Pole
title_full Infrared solar physics from the South Pole
title_fullStr Infrared solar physics from the South Pole
title_full_unstemmed Infrared solar physics from the South Pole
title_sort infrared solar physics from the south pole
publishDate 1989
url http://ntrs.nasa.gov/search.jsp?R=19920039808
op_coverage Unclassified, Unlimited, Publicly available
geographic South Pole
geographic_facet South Pole
genre South pole
genre_facet South pole
op_source Other Sources
op_relation http://ntrs.nasa.gov/search.jsp?R=19920039808
Accession ID: 92A22432
op_rights Copyright
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