Results 131 to 140 of about 3,957 (226)

Solar Chromospheric Heating by Magnetohydrodynamic Waves: Dependence on the Inclination of the Magnetic Field

The Astrophysical Journal
A proposed mechanism for solar chromospheric heating is magnetohydrodynamic waves propagating upward along magnetic field lines and dissipating their energy in the chromosphere.
Mayu Koyama, Toshifumi Shimizu
doaj   +1 more source

SUTO-Solar Through-Turbulence Open Image Dataset. [PDF]

Sensors (Basel), 2022
Popowicz A, Orlov V.
europepmc   +1 more source

Grand Challenges in the Physics of the Sun and Sun-like Stars

Frontiers in Astronomy and Space Sciences, 2014
Michael J. Thompson
doaj   +1 more source

Mapping solar magnetic fields from the photosphere to the base of the corona. [PDF]

Sci Adv, 2021
Ishikawa R, Bueno JT, Del Pino Alemán T, Okamoto TJ, McKenzie DE, Auchère F, Kano R, Song D, Yoshida M, Rachmeler LA, Kobayashi K, Hara H, Kubo M, Narukage N, Sakao T, Shimizu T, Suematsu Y, Bethge C, De Pontieu B, Dalda AS, Vigil GD, Winebarger A, Ballester EA, Belluzzi L, Štěpán J, Ramos AA, Carlsson M, Leenaarts J.   +27 more
europepmc   +1 more source

The Sun as a driver of the inner heliosphere: Modern investigations of fundamental plasma processes. [PDF]

Nat Commun
Ervin T, Nakhleh AJ, Bharati Das S.
europepmc   +1 more source

The Manifold Structure of the Chromosphere and Corona

, 1971
Although the photosphere is a uniform region for scales greater than the granulation, the fact that the magnetic field strength falls off less sharply than the gas pressure leads to strong magnetic influence at greater heights in the solar atmosphere ...
Zirin, H.
core  

Near infrared observations of solar chromosphere

, 2009
The solar chromosphere is an excellent medium to explore the intricate interplay between plasma and magnetic fields in a regime where both are relevant and alternately dominant.
Tejomoortula, Usha Sree
core  

Magnetic activity and spectral behavior of RS CVn binary system (IM Pegasi) in the ultraviolet. [PDF]

Sci Rep
Sanad MR, Rahman HIA, Badawy WA.
europepmc   +1 more source

Characteristics of acoustic-wave heating in simulations of the quiet Sun chromosphere

Understanding energy transfer through the chromosphere is paramount to solving the coronal heating problem. We investigated the energy dissipation of acoustic waves in the chromosphere of the quiet Sun using 3D radiative magnetohydrodynamic (rMHD ...
Elias R. Udnæs, Tiago M. D. Pereira
core   +1 more source

Spectroscopic Analysis and RHD Modeling of the First Ca II H and H ϵ Flare Spectra from DKIST/ViSP. [PDF]

Sol Phys
Tamburri C, Kowalski A, Cauzzi G, Kazachenko M, Tritschler A, Yadav R, French R, Notsu Y, Reardon K, Tristan I.   +9 more
europepmc   +1 more source