Homologous Extreme Ultraviolet Waves in the Emerging Flux Region Observed by the Solar Dynamics Observatory

Details Homologous Extreme Ultraviolet Waves in the Emerging Flux Region Observed by the Solar Dynamics Observatory Homologous Extreme Ultraviolet Waves in the Emerging Flux Region Observed by the Solar Dynamics Observatory

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012apj...747...67z&link_type=abstract

The Astrophysical Journal, Volume 747, Issue 1, article id. 67 (2012).

Astronomy and Astrophysics

Astronomy

1

Sun: Activity, Sun: Corona, Sun: Coronal Mass Ejections: Cmes

Scientific paper

Taking advantage of the high temporal and spatial resolution of the Solar Dynamics Observatory (SDO) observations, we present four homologous extreme ultraviolet (EUV) waves within 3 hr on 2010 November 11. All EUV waves emanated from the same emerging flux region (EFR), propagated in the same direction, and were accompanied by surges, weak flares, and faint coronal mass ejections (CMEs). The waves had the basically same appearance in all EUV wavebands of the Atmospheric Imaging Assembly on SDO. The waves propagated at constant velocities in the range of 280-500 km s-1, with little angular dependence, which indicated that the homologous waves could be likely interpreted as fast-mode waves. The waves are supposed to likely involve more than one driving mechanism, and it was most probable that the waves were driven by the surges, due to their close timing and location relations. We also propose that the homologous waves were intimately associated with the continuous emergence and cancellation of magnetic flux in the EFR, which could supply sufficient energy and trigger the onsets of the waves.

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