Results 181 to 190 of about 3,072 (224)
Improving the Spectral Resolution and Wavelength Scale of SDO/EVE MEGS-A Flare Observations. [PDF]
Gonzalez G, Chamberlin P, Herde V.
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Observation of super-Alfvénic slippage of reconnecting magnetic field lines on the Sun. [PDF]
Lörinčík J +5 more
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IMAP's Role in Understanding Particle Injection and Energization Throughout the Heliosphere. [PDF]
Cohen CMS +30 more
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Triangulation of Hard X-Ray Sources in an X-Class Solar Flare with ASO-S/HXI and Solar Orbiter/STIX. [PDF]
Ryan DF +6 more
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Upper Atmosphere Dynamics and Drivers of Volatiles Loss from Terrestrial-Type (Exo)Planets. [PDF]
Kubyshkina D +9 more
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Magnetic star-planet interaction in the young exoplanet system DS Tucanae Ab
Santos Ld +13 more
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Understanding the Solar Chromosphere
AIP Conference Proceedings, 2008We discuss the latest high‐resolution ground and space‐based observations of the solar chromosphere and their relevance to problems of chromospheric modeling. In particular, we briefly review recent as well as previous attempts to understand the solar chromosphere as the atmospheric layer with an apparently increasing temperature.
Cristiana Dumitrache +2 more
exaly +2 more sources
The Boundary of the Solar Chromosphere
Nature, 1929THE question of the sudden ending of the chromosphere or its gradual fading away in accordance with Prof. Milne's theoretical views may not yet be settled finally by observation. Mr. R. W. Gurney is, however, under a misapprehension (NATURE, Feb. 16, p. 240) in thinking that the bright K line studied by Mr. P. A. Taylor and Mr. McCrea up to a height of
F. J. M. STRATTON, C. R. DAVIDSON
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Solar Wind and Chromospheric Network
Solar Physics, 1997A physical model of the transition region, including upflow of the plasma in magnetic field funnels that are open to the overlying corona, is presented. A numerical study of the effects of Alfven waves on the heating and acceleration of the nascent solar wind originating in the chromospheric network is carried out within the framework of a two-fluid ...
Marsch, E., Tu, C.
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