Coronal Quasi-periodic Fast-mode Propagating Wave Trains

Author:

Shen YuandengORCID,Zhou XinpingORCID,Duan YadanORCID,Tang ZehaoORCID,Zhou Chengrui,Tan Song

Funder

Natural Science Foundation of China

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference261 articles.

1. Arregui, I., Oliver, R., Ballester, J.L.: 2018, Prominence oscillations. Liv. Rev. Solar Phys. 15, 3. DOI. ADS.

2. Aschwanden, M.J.: 2004, The role of observed MHD oscillations and waves for coronal heating. In: Walsh, R.W., Ireland, J., Danesy, D., Fleck, B. (eds.) SOHO 15 Coronal Heating SP-575, ESA, Noordwijk, 97. ADS.

3. Aschwanden, M.J.: 2005, Physics of the Solar Corona. An Introduction with Problems and Solutions, 2nd edn. Springer, Cham. ADS.

4. Aschwanden, M.J., Fletcher, L., Schrijver, C.J., Alexander, D.: 1999, Coronal loop oscillations observed with the transition region and coronal explorer. Astrophys. J. 520, 880. DOI. ADS.

5. Bárta, M., Karlický, M., Žemlička, R.: 2008, Plasmoid dynamics in flare reconnection and the frequency drift of the drifting pulsating structure. Solar Phys. 253, 173. DOI. ADS.

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