Results 181 to 190 of about 3,043 (224)

Observation of super-Alfvénic slippage of reconnecting magnetic field lines on the Sun. [PDF]

Nat Astron
Lörinčík J, Dudík J, Sainz Dalda A, Aulanier G, Polito V, De Pontieu B.   +5 more
europepmc   +1 more source

Upper Atmosphere Dynamics and Drivers of Volatiles Loss from Terrestrial-Type (Exo)Planets. [PDF]

Space Sci Rev
Kubyshkina D, Way MJ, Dandouras I, Lammer H, Lanza AF, Lingam M, Nakamura R, Persson M, Scherf M, Seki K.   +9 more
europepmc   +1 more source

Triangulation of Hard X-Ray Sources in an X-Class Solar Flare with ASO-S/HXI and Solar Orbiter/STIX. [PDF]

Sol Phys
Ryan DF, Massa P, Battaglia AF, Dickson ECM, Su Y, Chen W, Krucker S.   +6 more
europepmc   +1 more source

Magnetoacoustic wave propagation in the solar corona and filament dynamics. [PDF]

Sci Rep
Somaiyeh S, Stefaan P.
europepmc   +1 more source

Observations of fine coronal structures with high-order solar adaptive optics. [PDF]

Nat Astron
Schmidt D, Schad TA, Yurchyshyn V, Gorceix N, Rimmele TR, Goode PR.   +5 more
europepmc   +1 more source

Magnetic star-planet interaction in the young exoplanet system DS Tucanae Ab

Santos Ld, Owen J, Duvvuri G, Loyd ROP, Vidotto A, Presa A, Bourrier V, King G, Airapetian V, Ehrenreich D, France K, Lendl M, Lothringer J, Nielsen L.   +13 more
europepmc   +1 more source

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The Boundary of the Solar Chromosphere

Nature, 1929
THE 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
  +4 more sources

Solar Wind and Chromospheric Network

Solar Physics, 1997
A 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.
openaire   +2 more sources

Understanding the Solar Chromosphere

AIP Conference Proceedings, 2008
We 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.
P Heinzel, Vasile Mioc, Nedelia A Popescu   +2 more
exaly   +2 more sources