Coronal Transverse Magnetohydrodynamic Waves in a Solar Prominence-Reference-Cited by-同舟云学术

Coronal Transverse Magnetohydrodynamic Waves in a Solar Prominence

Published:2007-12-07 Issue:5856 Volume:318 Page:1577-1580
ISSN:0036-8075
Container-title:Science
language:en
Short-container-title:Science

Author:

Okamoto T. J.¹²³⁴⁵,Tsuneta S.¹²³⁴⁵,Berger T. E.¹²³⁴⁵,Ichimoto K.¹²³⁴⁵,Katsukawa Y.¹²³⁴⁵,Lites B. W.¹²³⁴⁵,Nagata S.¹²³⁴⁵,Shibata K.¹²³⁴⁵,Shimizu T.¹²³⁴⁵,Shine R. A.¹²³⁴⁵,Suematsu Y.¹²³⁴⁵,Tarbell T. D.¹²³⁴⁵,Title A. M.¹²³⁴⁵

Affiliation:

1. National Astronomical Observatory (NAOJ), Mitaka, Tokyo 181-8588, Japan.

2. Kwasan and Hida Observatories, Kyoto University, Yamashina, Kyoto 607-8471, Japan.

3. Lockheed Martin Solar and Astrophysics Laboratory, B/252, 3251 Hanover Street, Palo Alto, CA 94304, USA.

4. High Altitude Observatory, National Center for Atmospheric Research, Post Office Box 3000, Boulder CO 80307–3000, USA.

5. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (ISAS/JAXA), Sagamihara, Kanagawa 229-8510, Japan.

Abstract

Solar prominences are cool 10 4 kelvin plasma clouds supported in the surrounding 10 6 kelvin coronal plasma by as-yet-undetermined mechanisms. Observations from Hinode show fine-scale threadlike structures oscillating in the plane of the sky with periods of several minutes. We suggest that these represent Alfvén waves propagating on coronal magnetic field lines and that these may play a role in heating the corona.

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

Reference31 articles.

1. Thin Threads of Solar Filaments

2. Profiles of Hi (La), Mgii (h and k), Caii (H and K) Lines of an active filament at the limb, with the LPSP instrument aboard the OSO-8 Satellite

3. J. M. Malherbe, B. Schmieder, E. Ribes, P. Mein, Astron. Astrophys.119, 197 (1983).

4. G. Simon, B. Schmieder, P. Démoulin, A. I. Poland, Astron. Astrophys.166, 319 (1986).

5. B. Schmieder, M. A. Raadu, J. E. Wiik, Astron. Astrophys.252, 353 (1991).

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