Author
Listed:
- J. W. Cirtain
(Marshall Space Flight Center, NASA, Mail Code ZP13, MSFC, Alabama 36812, USA)
- L. Golub
(Harvard-Smithsonian Center for Astrophysics, 60 Garden Street)
- A. R. Winebarger
(Marshall Space Flight Center, NASA, Mail Code ZP13, MSFC, Alabama 36812, USA)
- B. De Pontieu
(Lockheed Martin Solar and Astrophysics Laboratory, 3251 Hanover Street)
- K. Kobayashi
(Center for Space and Aeronautic Research, University of Alabama-Huntsville, 320 Sparkman Avenue, Huntsville, Alabama 35812, USA)
- R. L. Moore
(Marshall Space Flight Center, NASA, Mail Code ZP13, MSFC, Alabama 36812, USA)
- R. W. Walsh
(University of Central Lancashire, Preston, Lancashire PR1 2HE, UK)
- K. E. Korreck
(Harvard-Smithsonian Center for Astrophysics, 60 Garden Street)
- M. Weber
(Harvard-Smithsonian Center for Astrophysics, 60 Garden Street)
- P. McCauley
(Harvard-Smithsonian Center for Astrophysics, 60 Garden Street)
- A. Title
(Lockheed Martin Solar and Astrophysics Laboratory, 3251 Hanover Street)
- S. Kuzin
(Lebedev Physical Institute, 53 Leninski Prospekt, 119991 Moscow, Russia)
- C. E. DeForest
(Southwest Research Institute, 1050 Walnut Street, Suite 300, Boulder, Colorado 80302, USA)
Abstract
Solar observations at a resolution of 0.2 arc seconds show the reconnection and relaxation of magnetic braids in a coronal active region, leading to the dissipation of sufficient energy to heat the structures to about 4,000,000 K.
Suggested Citation
J. W. Cirtain & L. Golub & A. R. Winebarger & B. De Pontieu & K. Kobayashi & R. L. Moore & R. W. Walsh & K. E. Korreck & M. Weber & P. McCauley & A. Title & S. Kuzin & C. E. DeForest, 2013.
"Energy release in the solar corona from spatially resolved magnetic braids,"
Nature, Nature, vol. 493(7433), pages 501-503, January.
Handle:
RePEc:nat:nature:v:493:y:2013:i:7433:d:10.1038_nature11772
DOI: 10.1038/nature11772
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