Results 181 to 190 of about 2,286 (221)

Properties of solar coronal loops revealed with Yohkoh

, 1997
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Flying through an Eruption-associated Magnetic Reconnection Current Sheet in the Solar Corona

Patel R, Niembro T, Xie X, Seaton D, Badman S, Roy S, Rivera Y, Reeves K, Stenborg G, Hess P, West M, Feller A, Hirzberger J, Suarez DO, Solanki S, Strecker H, Valori G.   +16 more
europepmc   +1 more source

Solar coronal loops

, 1980
In the past few years it has been realised that loop structures are an important feature of the solar corona, Presumably, these struc­tures outline the local magnetic field and in this thesis some theoreti­cal aspects of solar coronal loops are considered.
Hood, A. W.
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Scaling of heating rates in solar coronal loops

Nature, 1995
THE gas of the solar corona is at a temperature of several million degrees, orders of magnitude hotter than the underlying photosphere. The nature of the physical process that heats the solar corona (and the coronae of solar-type stars more generally) has been a long-standing puzzle.
James A Klimchuk, Klimchuk James A
exaly   +2 more sources

Feature Exploration for Mining Coronal Loops from Solar Images

, 2008
Coronal loops are especially important in analyzing some important phenomena related to the Sun such as the controversial coronal heating problem. The analysis requires astrophysicists to manually sift through thousands of images in order to acquire ...
Nurcan Durak, Olfa Nasraoui
exaly   +2 more sources

Coronal loop detection from solar images

Pattern Recognition, 2009
zbMATH Open Web Interface contents unavailable due to conflicting licenses.
Nurcan Durak, Olfa Nasraoui, Joan Schmelz   +2 more
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Solar Coronal Loops and Coronal Heating Models

AIP Conference Proceedings, 2005
Ever since it was realized, some sixty five years ago, that the solar corona is three orders of magnitude hotter than the underlying photosphere, scientists have puzzled over the reason for these extreme conditions. A number of plausible ideas have been put forward, including the dissipation of magnetohydrodynamic (MHD) waves and the dissipation of ...
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Current confinement in solar coronal loops

Solar Physics, 1981
In this paper solar coronal loops are regarded as regions of localized current flows. The main purpose is to investigate the consequences of current confinement rather than to produce a model. The physical and observational basis for this assumption are presented as well as the connection with previous studies on loop structure.
Claudio Chiuderi, Giorgio Einaudi
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Modelling of a solar coronal loop

Journal of Plasma Physics, 1996
Montgomery and co-workers have developed a framework to describe the steady state of a turbulent magnetofluid, without the usual recourse to linearization. Thus the magnetic and velocity fields emerge in their fully nonlinear form as a consequence of the selective decays of the invariants of the system.
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Coronal Loops in Solar Active Regions

Publications of the Astronomical Society of Australia, 1989
AbstractWe discuss the appearance of solar active regions as seen in EUV line radiation in terms of a system of simple static coronal loop models. The loop models are based on those of Rosner et al. (1978) and may be understood in terms of the scaling laws introduced by these authors. We present here some generalized scaling laws which demonstrate that
C. J. Durrant, S. F. Brown
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