Results 211 to 220 of about 1,105,860 (262)

Coronal dimmings and what they tell us about solar and stellar coronal mass ejections. [PDF]

Living Rev Sol Phys
Veronig AM, Dissauer K, Kliem B, Downs C, Hudson HS, Jin M, Osten R, Podladchikova T, Prasad A, Qiu J, Thompson B, Tian H, Vourlidas A.   +12 more
europepmc   +1 more source

Mapping the Sun's coronal magnetic field using the Zeeman effect. [PDF]

Sci Adv
Schad TA, Petrie GJD, Kuhn JR, Fehlmann A, Rimmele T, Tritschler A, Woeger F, Scholl I, Williams R, Harrington D, Paraschiv AR, Szente J.   +11 more
europepmc   +1 more source

Searching for ultralight dark matter conversion in solar corona using Low Frequency Array data. [PDF]

Nat Commun
An H, Chen X, Ge S, Liu J, Luo Y.
europepmc   +1 more source

Mancha3D Code: Multipurpose Advanced Nonideal MHD Code for High-Resolution Simulations in Astrophysics. [PDF]

Sol Phys
Modestov M, Khomenko E, Vitas N, de Vicente A, Navarro A, González-Morales PA, Collados M, Felipe T, Martínez-Gómez D, Hunana P, Luna M, Koll Pistarini M, Popescu Braileanu B, Perdomo García A, Liakh V, Santamaria I, Gomez Miguez MM.   +16 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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Solar Chromosphere

Oxford Research Encyclopedia of Physics, 2019
This is an advance summary of a forthcoming article in the Oxford Research Encyclopedia of Physics. Please check back later for the full article. The solar chromosphere (color sphere) is a strongly structured and highly dynamic region (layer) of the Sun’s atmosphere, located above the bright, visible ...
S. Jafarzadeh
openaire   +2 more sources

New View of the Solar Chromosphere

Annual Review of Astronomy and Astrophysics, 2019
The solar chromosphere forms a crucial, yet complex and until recently poorly understood, interface between the solar photosphere and the heliosphere. ▪ Advances in high-resolution instrumentation, adaptive optics, image reconstruction techniques, and ...
M. Carlsson, B. Pontieu, V. Hansteen
semanticscholar   +1 more source

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, Cristiana Dumitrache, Nedelia A. Popescu   +3 more
openaire   +1 more source