DocumentCode
1260512
Title
Acoustic Events in the Solar Atmosphere
Author
Malherbe, Jean-Marie ; Roudier, Thierry ; Berger, Thomas ; Frank, Zoe
Author_Institution
LESIA, Obs. de Paris, Meudon, France
Volume
39
Issue
11
fYear
2011
Firstpage
2706
Lastpage
2707
Abstract
New observations have been obtained on September 4, 2010, by the Solar Optical Telescope on board the satellite HINODE, in the magnetically insensitive Fel 557.6-nm line formed in the solar atmosphere. Acoustic events (AEs, defined as spatially concentrated propagating waves) have been derived in the photosphere from amplitudes and phases of vertical Doppler velocities with outstanding spatial resolution (0.3") and field of view. AEs have a mean lifetime of 500 s and contain about 2 × 1019 J each. Most AEs are upward and occur in intergranular lanes and converging regions associated to permanent plasma downflow. They partly contribute (10%) to energy transport involved in chromospheric heating and could be the drivers of solar oscillations. More than 106 events are simultaneously present on the Sun with a birth/decay rate of 2000 events per second.
Keywords
chromosphere; photosphere; solar pulsations; AD 2010 09 04; HINODE satellite; Solar Optical Telescope; acoustic events; chromospheric heating; converging region; energy transport; intergranular lane; magnetically insensitive Fe I line; permanent plasma downflow; photosphere; solar atmosphere; solar oscillation; spatial resolution; spatially concentrated propagating waves; vertical Doppler velocity; wavelength 557.6 nm; Acoustics; Atmospheric waves; Manganese; Oscillators; Spatial resolution; Sun; Acoustic waves; astronomy; astrophysics; the Sun;
fLanguage
English
Journal_Title
Plasma Science, IEEE Transactions on
Publisher
ieee
ISSN
0093-3813
Type
jour
DOI
10.1109/TPS.2011.2154344
Filename
5934431
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