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Deciphering solar magnetic activity: The (solar) hale cycle terminator of 2021

open access: yesFrontiers in Astronomy and Space Sciences, 2023
We previously identified an event in the solar timeline that appeared to play a role in how sunspot Cycle 23 (SC23) transitioned into sunspot Cycle 24 (SC24). The timeframe for this transition was rapid, taking place over a very short time and perhaps in
Scott W. McIntosh   +3 more
doaj   +1 more source

Magnetic Field Re-configuration Associated With a Slow Rise Eruptive X1.2 Flare in NOAA Active Region 11944

open access: yesFrontiers in Astronomy and Space Sciences, 2022
Using multi-wavelength observations, we analysed magnetic field variations associated with a gradual X1.2 flare that erupted on January 7, 2014 in active region (AR) NOAA 11944 located near the disk center. A fast coronal mass ejection (CME) was observed
Vasyl Yurchyshyn   +8 more
doaj   +1 more source

An Analysis of Image-Reading of Sun from Propositions of Active Intellect and Light of All Lights in Suhrawardi’s Symbolic Treatises [PDF]

open access: yesادبیات عرفانی, 2021
Mega-metaphors or central images, as propositions, contain profound thoughts originated from the mystic's personal experiences. Hence, decoding and clarifying the secondary meanings of these mega-metaphors will help to have a closer look at the mystic's ...
Davoud Sparham   +3 more
doaj   +1 more source

The dynamic chromosphere at millimeter wavelengths

open access: yesFrontiers in Astronomy and Space Sciences, 2022
The chromosphere is one of the most complex and dynamic layers of the solar atmosphere. The dynamic phenomena occur on different spatial and temporal scales, not only in active regions but also in the so-called quiet Sun.
Alexander Nindos   +5 more
doaj   +1 more source

Magnetic Structure in Successively Erupting Active Regions: Comparison of Flare-Ribbons With Quasi-Separatrix Layers

open access: yesFrontiers in Physics, 2021
This paper studies the magnetic topology of successively erupting active regions (ARs) 11,429 and 12,371. Employing vector magnetic field observations from Helioseismic and Magnetic Imager, the pre-eruptive magnetic structure is reconstructed by a model ...
P. Vemareddy
doaj   +1 more source

Propagation and Damping of Longitudinal Intensity Oscillations in Solar Coronal Structures [PDF]

open access: yesIranian Journal of Astronomy and Astrophysics, 2017
Recently, the longitudinal oscillations of intensity have been frequently detected in the different structures of the solar corona using space telescope observations.
Abbas Abedini   +1 more
doaj   +1 more source

A Genetic Algorithm to Model Solar Radio Active Regions From 3D Magnetic Field Extrapolations

open access: yesFrontiers in Astronomy and Space Sciences, 2022
In recent decades our understanding of solar active regions (ARs) has improved substantially due to observations made with better angular resolution and wider spectral coverage.
Alexandre José de Oliveira e Silva   +12 more
doaj   +1 more source

High Resolution Soft X-ray Spectroscopy and the Quest for the Hot (5–10 MK) Plasma in Solar Active Regions

open access: yesFrontiers in Astronomy and Space Sciences, 2021
We discuss the diagnostics available to study the 5–10 MK plasma in the solar corona, which is key to understanding the heating in the cores of solar active regions.
Giulio Del Zanna   +8 more
doaj   +1 more source

Time Dependence of 50–250 MeV Galactic Cosmic-Ray Protons between Solar Cycles 24 and 25, Measured by the High-energy Particle Detector on board the CSES-01 Satellite

open access: yesThe Astrophysical Journal Letters, 2023
Time-dependent energy spectra of galactic cosmic rays (GCRs) carry crucial information regarding their origin and propagation throughout the interstellar environment.
M. Martucci   +56 more
doaj   +1 more source

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