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Long-lived Coronal Loop Profiles from TRACE
Authors:Lenz  Dawn D  DeLuca  Edward E  Golub  Leon  Rosner  Robert  Bookbinder  Jay A  Litwin  Christof  Reale  Fabio  Peres  Giovanni
Institution:(1) Department of Astronomy and Astrophysics, University of Chicago, 5640 South Ellis Avenue, Chicago, IL, 60637, U.S.A.;(2) Smithsonian Astrophysical Observatory, 60 Garden Street, Cambridge, MA, 02138, U.S.A;(3) Department of Astronomy and Astrophysics, University of Chicago, 5640 South Ellis Avenue, Chicago, IL, 60637, U.S.A.;(4) Smithsonian Astrophysical Observatory, 60 Garden Street, Cambridge, MA, 02138, U.S.A.;(5) Department of Astronomy and Astrophysics, University of Chicago, 5640 South Ellis Avenue, Chicago, IL, 60637, U.S.A.;(6) Dipartimento di Scienze Fisiche e Astronomiche, Sezione di Astronomia, Università di Palermo, Piazza del Parlamento 1, I-90134 Palermo, Italy
Abstract:An initial study of long-lived loops observed with TRACE (Lenz et al., 1999) shows that they have no significant temperature stratification and that they are denser than the classic loop model predicts. Models that agree better with the observations include a loop consisting of a bundle of filaments at different temperatures and a loop with momentum input by MHD waves. Some implications for coronal heating models and mechanisms are discussed.
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