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The Astrophysical Journal, 724:10831098, 2010 December 1 doi:10.1088/0004-637X/724/2/1083 C 2010. The American Astronomical Society. All rights reserved. Printed in the U.S.A.
 

Summary: The Astrophysical Journal, 724:1083­1098, 2010 December 1 doi:10.1088/0004-637X/724/2/1083
C 2010. The American Astronomical Society. All rights reserved. Printed in the U.S.A.
MULTIWAVELENGTH OBSERVATIONS OF SMALL-SCALE RECONNECTION EVENTS
TRIGGERED BY MAGNETIC FLUX EMERGENCE IN THE SOLAR ATMOSPHERE
S. L. Guglielmino1
, L. R. Bellot Rubio2
, F. Zuccarello1
, G. Aulanier3
, S. Vargas Dom´inguez4
, and S. Kamio5
1 Dipartimento di Fisica e Astronomia, Universit`a di Catania, I 95123 Catania, Italy; salvo.guglielmino@oact.inaf.it
2 Instituto de Astrof´isica de Andaluc´ia (CSIC), Apdo. de Correos 3004, E 18080 Granada, Spain
3 LESIA, Observatoire de Paris, CNRS, UPMC, Universit´e Paris Diderot, 5 place Jules Janssen, 92190 Meudon, France
4 Mullard Space Science Laboratory, RH5 6NT Holmbury St. Mary, Dorking, Surrey, UK
5 Max-Planck-Institut f¨ur Sonnensystemforschung, D 37191 Katlenburg-Lindau, Germany
Received 2010 May 18; accepted 2010 July 17; published 2010 November 11
ABSTRACT
The interaction between emerging magnetic flux and the pre-existing ambient field has become a "hot" topic for both
numerical simulations and high-resolution observations of the solar atmosphere. The appearance of brightenings
and surges during episodes of flux emergence is believed to be a signature of magnetic reconnection processes.

  

Source: Aulanier, Guillaume - Observatoire de Paris

 

Collections: Physics