Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/7068
Title: Unravelling the Components of a Multi-Thermal Coronal Loop Using Magnetohydrodynamic Seismology
Authors: Prasad, S. K
Jess, D. B
Klimchuk, J. A
Banerjee, D
Keywords: Magnetohydrodynamics (MHD);Sun: corona;Sun: fundamental parameters;Sun: oscillations;Sunspots
Issue Date: 10-Jan-2017
Publisher: IOP Publishing
Citation: The Astrophysical Journal, Vol. 834, No. 2, 103
Abstract: Coronal loops, constituting the basic building blocks of the active Sun, serve as primary targets to help understand the mechanisms responsible for maintaining multi-million Kelvin temperatures in the solar and stellar coronae. Despite significant advances in observations and theory, our knowledge on the fundamental properties of these structures is limited. Here, we present unprecedented observations of accelerating slow magnetoacoustic waves along a coronal loop that show differential propagation speeds in two distinct temperature channels, revealing the multi-stranded and multithermal nature of the loop. Utilizing the observed speeds and employing nonlinear force-free magnetic field extrapolations, we derive the actual temperature variation along the loop in both channels, and thus are able to resolve two individual components of the multithermal loop for the first time. The obtained positive temperature gradients indicate uniform heating along the loop, rather than isolated footpoint heating.
Description: Restricted Access
URI: http://hdl.handle.net/2248/7068
ISSN: 0004-637X
???metadata.dc.rights???: © The American Astronomical Society
???metadata.dc.relation.uri???: http://dx.doi.org/10.3847/1538-4357/834/2/103
Appears in Collections:IIAP Publications

Files in This Item:
File Description SizeFormat 
Unravelling the Components of a Multi-Thermal Coronal Loop.pdfRestricted Access1.47 MBAdobe PDFView/Open


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.