Results 141 to 150 of about 285 (167)

Evidence of ubiquitous Alfvén pulses transporting energy from the photosphere to the upper chromosphere. [PDF]

Nat Commun, 2019
Liu J, Nelson CJ, Snow B, Wang Y, Erdélyi R.   +4 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

Element Abundances: A New Diagnostic for the Solar Wind. [PDF]

Astrophys J, 2019
Laming JM, Vourlidas A, Korendyke C, Chua D, Cranmer SR, Ko YK, Kuroda N, Provornikova E, Raymond JC, Raouafi NE, Strachan L, Tun-Beltran S, Weberg M, Wood BE.   +13 more
europepmc   +1 more source

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

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

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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Physical Properties of the Quiet Solar Chromosphere–Corona Transition Region

Astronomy Letters, 2016
The physical properties of the quiet solar chromosphere–corona transition region are studied. Here the structure of the solar atmosphere is governed by the interaction of magnetic fields above the photosphere. Magnetic fields are concentrated into thin tubes inside which the field strength is great.
Boris Somov
exaly   +2 more sources

SUMER Observations of the Quiet Solar Atmosphere: The Network Chromosphere and Lower Transition Region

Astrophysical Journal, 1997
We examine spectral properties of the network chromosphere and lower transition region from the SUMER instrument on the SOHO spacecraft, using time-series data sets discussed in an accompanying Letter by Carlsson, Judge, & Wilhelm. The data were obtained early in the mission with no tracking of solar features and so cannot generally be used to examine ...
Philip G Judge, Mats Carlsson, Klaus Wilhelm   +2 more
exaly   +3 more sources

The Quiet Chromosphere: Phase Relation With the Solar Cycle

Advances in Space Research, 2022
K J Li
exaly   +2 more sources