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The Unstable Chromosphere: Effects of the Thermal Farley-Buneman Instability Across a Broad Range of Solar Chromospheric Conditions

Samuel Evans, Meers Oppenheim, Juan Martínez-Sykora, Alexander Green   +3 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]

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

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

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

Butterfly Diagram and Other Properties of Plage Areas from Kodaikanal Ca ii K Photographs Covering 1904 - 2007. [PDF]

Sol Phys
Jha BK, Chatzistergos T, Banerjee D, Ermolli I, Krivova NA, Solanki SK, Priyadarshi A.   +6 more
europepmc   +1 more source

Exceptionally gigantic aurora in the polar cap on a day when the solar wind almost disappeared. [PDF]

Sci Adv
Hosokawa K, Kataoka R, Tsuda TT, Ogawa Y, Taguchi S, Zhang Y, Paxton LJ.   +6 more
europepmc   +1 more source

Direct imaging of magnetohydrodynamic wave mode conversion near a 3D null point on the sun. [PDF]

Nat Commun
Kumar P, Nakariakov VM, Karpen JT, Cho KS.   +3 more
europepmc   +1 more source

Magnetic Field Measurements in the Solar Chromosphere Using the H$_β$ 4861Å~Line I: Forward Modeling Based on 1D Models [PDF]

Jiasheng Wang, Wenxian Li, Xianyong Bai, Yingzi Sun, Yuanyong Deng, Jiaben Lin   +5 more
openalex  

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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Structure of the Solar Chromosphere

Nature, 1964
THE suggestion of Biermann1 and Schwarzschild2, that the radially increasing temperature of the solar atmosphere is to be ascribed to propagation of non-thermal energy, such as acoustic waves, is now generally accepted. The effect of magnetic field, and the possibility that the energy-carrying waves are of a magnetohydrodynamic character rather than ...
openaire   +3 more sources