Results 181 to 190 of about 43,284 (218)

Improving the Spectral Resolution and Wavelength Scale of SDO/EVE MEGS-A Flare Observations. [PDF]

Sol Phys
Gonzalez G, Chamberlin P, Herde V.
europepmc   +1 more source

Ligand-Driven Optimization of Iron Oxide Nanoprobes for In Vivo MRI Enhancement at Ultra-High Field. [PDF]

Small
García-Acevedo P, Alonso-Alonso ML, Ortega-Espina S, Bañobre-López M, Piñeiro Y, Iglesias-Rey R, Rivas J.   +6 more
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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
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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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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.
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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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