Results 21 to 30 of about 14,496 (257)
Accurately assessing the balance between acoustic wave energy fluxes and radiative losses is critical for understanding how the solar chromosphere is thermally regulated.
J. M. da Silva Santos +5 more
doaj +2 more sources
An overall view of temperature oscillations in the solar chromosphere with ALMA. [PDF]
Jafarzadeh S +14 more
europepmc +2 more sources
Collisional dissipation of Alfvén waves in a partially ionised solar chromosphere [PDF]
J. E. Leake +2 more
openalex +3 more sources
Chromospheric Jets and Their Properties [PDF]
In this study we review solar chromospheric jets and characteristics of them. The chromosphere and transition region are the interface between the solar photosphere and the corona, which plays a key role in the formation and acceleration of the solar ...
Ehsan Tavabi, Sima Zeighami
doaj +1 more source
The quiet sun at mm wavelengths as seen by ALMA
Solar observations at sub-mm, mm and cm wavelengths offer a straightforward diagnostic of physical conditions in the solar atmosphere because they yield measurement of brightness temperature which, for optically thick features, equals intrinsic ...
Costas E. Alissandrakis +2 more
doaj +1 more source
Chromosphere Activity Relation with Solar Dynamo Magnetic Activity Cycle [PDF]
In this article, we analyzed the abnormal thickness of the chromosphere above the coronal holes (CH) at the poles of the Sun for 13 years (2010-2022), on the 15th of every month, by using AIA/SDO telescope data.
Ehsan Tavabi, Mina Rajabi, Sima Zeighami
doaj +1 more source
CAII lines in a quiet region on the Sun I. Dynamic processes in the solar atmosphere
We have studied oscillation processes in the quiet Sun outside a coronal hole at different levels of the solar chromosphere. The study was based on spectroscopic observations of ionized calcium lines (K, H, and 849.8 nm) obtained by the Sayan Solar ...
Turova I. P. +2 more
doaj +1 more source
Why “Solar Tsunamis” Rarely Leave Their Imprints in the Chromosphere
Solar coronal waves frequently appear as bright disturbances that propagate globally from the eruption center in the solar atmosphere, just like the tsunamis in the ocean on Earth.
Ruisheng Zheng +12 more
doaj +1 more source
Alfvén Wave Connection between the Chromosphere and the Corona of the Sun: An Analytical Study
Alfvén waves are closely relevant to the three outstanding problems in the solar corona: coronal heating, solar wind acceleration, and the fractionization of low first ionization potential (FIP) elements.
Jongchul Chae, Kyoung-Sun Lee
doaj +1 more source

