Results 41 to 50 of about 429,319 (205)

Comparison of transient horizontal magnetic fields in a plage region and in the quiet Sun

open access: yes, 2008
Properties of transient horizontal magnetic fields (THMFs) in both plage and quiet Sun regions are obtained and compared. Spectro-polarimetric observations with the Solar Optical Telescope (SOT) on the Hinode satellite were carried out with a cadence of ...
Abbett   +25 more
core   +1 more source

Eruptions from quiet Sun coronal bright points [PDF]

open access: yesAstronomy & Astrophysics, 2018
Context. Eruptions from coronal bright points (CBPs) are investigated in a two-part study. Aims. The present study aims to explore in full detail the morphological and dynamical evolution of these eruptions in the context of the full lifetime evolution of CBPs.
Mou, Chauzhou   +3 more
openaire   +4 more sources

Incoherent Solar Radio Emission

open access: yesFrontiers in Astronomy and Space Sciences, 2020
Incoherent solar radio radiation comes from the free-free, gyroresonance, and gyrosynchrotron emission mechanisms. Free-free is primarily produced from Coulomb collisions between thermal electrons and ions.
Alexander Nindos
doaj   +1 more source

Observations of Locally Excited Waves in the Low Solar Atmosphere Using the Daniel K. Inouye Solar Telescope

open access: yesThe Astrophysical Journal Letters
We present an interpretation of the recent Daniel K. Inouye Solar Telescope (DKIST) observations of propagating wave fronts in the lower solar atmosphere.
Shah Mohammad Bahauddin   +7 more
doaj   +1 more source

Observations of coronal holes with the Siberian Radioheliograph

open access: yesSolar-Terrestrial Physics
Multi-wavelength observations of a coronal hole (CH) with two-dimensional spatial resolution have been made for the first time in the frequency range from 2.8 to 12 GHz.
Globa M. V.   +2 more
doaj   +1 more source

Numerical simulations of quiet Sun magnetic fields seeded by Biermann battery

open access: yes, 2017
The magnetic fields of the quiet Sun cover at any time more than 90\% of its surface and their magnetic energy budget is crucial to explain the thermal structure of the solar atmosphere. One of the possible origins of these fields is due to the action of
Collados, M.   +3 more
core   +1 more source

Chromospheric Spectra of Small-scale Dynamic Features Observed on and off Solar Disk with Goode Solar Telescope

open access: yesThe Astrophysical Journal
Our study of H α line profiles of rapid blue- and redshifted excursions measured with Goode Solar Telescope revealed an asymmetrical three-peak structure present in the blue wing of the H α line, suggesting complex internal velocity fields that may ...
Vasyl Yurchyshyn   +6 more
doaj   +1 more source

Modulation of Cosmic-Ray Antiprotons in the Heliosphere: Simulations for a Solar Cycle

open access: yesThe Astrophysical Journal, 2023
The precision measurements of galactic cosmic-ray protons from the Payload for Antimatter Matter Exploration and Light-nuclei Astrophysics and the Alpha Magnetic Spectrometer are reproduced using a well-established three-dimensional numerical model for ...
O. P. M. Aslam   +3 more
doaj   +1 more source

Inferring depth-dependent plasma motions from surface observations using the DeepVel neural network

open access: yesJournal of Space Weather and Space Climate, 2021
Coverage of plasma motions is limited to the line-of-sight component at the Sun’s surface. Multiple tracking and inversion methods were developed to infer the transverse motions from observational data.
Tremblay Benoit   +4 more
doaj   +1 more source

Magnetic Topology and Loop Statistics in Observed Coronal Holes Using Potential Field Modeling

open access: yesThe Astrophysical Journal
Potential field source surface (PFSS) models are widely used to study the solar corona and form the basis for solar wind forecasting, yet they often fail to reproduce observed properties of coronal holes.
Stephan G. Heinemann   +2 more
doaj   +1 more source

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