Coronal transverse magnetohydrodynamic waves in a solar prominence

Science

Volumn 318, Issue 5856, 2007, Pages 1577-1580

  Okamoto, T J ^a,b   Tsuneta, S ^a   Berger, T E ^c   Ichimoto, K ^a   Katsukawa, Y ^a   Lites, B W ^d   Nagata, S ^b   Shibata, K ^b   Shimizu, T ^e   Shine, R A ^c   Suematsu, Y ^a   Tarbell, T D ^c   Title, A M ^c  

^a NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

^b KYOTO UNIVERSITY   (Japan)

^c LOCKHEED MARTIN   (United States)

^d NATIONAL CENTER FOR ATMOSPHERIC RESEARCH   (United States)

^e JAPAN AEROSPACE EXPLORATION AGENCY   (Japan)

Author keywords

[No Author keywords available]

Indexed keywords

ATMOSPHERIC WAVE; CORONA; MAGNETIC FIELD; MAGNETOHYDRODYNAMICS; PLASMA;

ARTICLE; ATMOSPHERE; HIGH TEMPERATURE; MATHEMATICAL MODEL; PRIORITY JOURNAL; SOLAR ENERGY; SOLAR RADIATION; SUN;

EID: 36849042638     PISSN: 00368075     EISSN: 10959203     Source Type: Journal    
DOI: 10.1126/science.1145447     Document Type: Article

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31. The authors thank H. Shibahashi, T. Sekii, R. Erdélyi, and V. Nakariakov for comments. Hinode is a Japanese mission developed and launched by ISAS/JAXA, with NAOJ as domestic partner and NASA and Science and Technology Facilities Council (STFC) (UK) as international partners. It is operated by these agencies in cooperation with European Space Agency and Norwegian Space Centre (Norway). This work was carried out at the NAOJ Hinode science center, which was supported by the Grant-in-Aid for Creative Scientific Research, the Basic Study of Space Weather Prediction (head investigator, K.S.) from the Ministry of Education, Culture, Sports, Science, and Technology, Japan, donation from Sun Microsystems Incorporated, and NAOJ internal funding. The National Center for Atmospheric Research is sponsored by NSF. T.J.O. is supported by research fellowships from the Japan Society for the Promotion of Science for Young Scientists.