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Exploring the Sun with ALMA
Authors
Miroslav Barta
Timothy Bastian
+16 more
Roman Brajša
Bin Chen
Bart Walter De Pontieu
G. Fleishman
D. E. Gary
Antonio Hales
Hugh Hudson
K Iwai
S Kim
A. Kobelski
Maria Loukitcheva
Masumi Shimojo
I. Skokić
Sven Wedemeyer
Stephen White
Y Yan
Publication date
1 January 2018
Publisher
Doi
Cite
Abstract
The Atacama Large Millimeter/submillimeter Array (ALMA) Observatory opens a new window onto the Universe. The ability to perform continuum imaging and spectroscopy of astrophysical phenomena at millimetre and submillimetre wavelengths with unprecedented sensitivity opens up new avenues for the study of cosmology and the evolution of galaxies, the formation of stars and planets, and astrochemistry. ALMA also allows fundamentally new observations to be made of objects much closer to home, including the Sun. The Sun has long served as a touchstone for our understanding of astrophysical processes, from the nature of stellar interiors, to magnetic dynamos, non-radiative heating, stellar mass loss, and energetic phenomena such as solar flares. ALMA offers new insights into all of these processes. © 2018 European Southern Observatory (ESO
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NORA - Norwegian Open Research Archives
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oai:www.duo.uio.no:10852/67713
Last time updated on 03/05/2019