Earth-affecting solar transients: a review of progresses in solar cycle 24
This review article summarizes the advancement in the studies of Earth-affecting solar
transients in the last decade that encompasses most of solar cycle 24. It is a part of the effort …
transients in the last decade that encompasses most of solar cycle 24. It is a part of the effort …
[HTML][HTML] Prediction of solar energetic events impacting space weather conditions
Aiming to assess the progress and current challenges on the formidable problem of the
prediction of solar energetic events since the COSPAR/International Living With a Star …
prediction of solar energetic events since the COSPAR/International Living With a Star …
The flare likelihood and region eruption forecasting (FLARECAST) project: flare forecasting in the big data & machine learning era
The European Union funded the FLARECAST project, that ran from January 2015 until
February 2018. FLARECAST had a research-to-operations (R2O) focus, and accordingly …
February 2018. FLARECAST had a research-to-operations (R2O) focus, and accordingly …
Critical Science Plan for the Daniel K. Inouye Solar Telescope (DKIST)
MP Rast, N Bello González, L Bellot Rubio, W Cao… - Solar Physics, 2021 - Springer
Abstract The National Science Foundation's Daniel K. Inouye Solar Telescope (DKIST) will
revolutionize our ability to measure, understand, and model the basic physical processes …
revolutionize our ability to measure, understand, and model the basic physical processes …
Toward improved understanding of magnetic fields participating in solar flares: Statistical analysis of magnetic fields within flare ribbons
MD Kazachenko, BJ Lynch, A Savcheva… - The Astrophysical …, 2022 - iopscience.iop.org
Violent solar flares and coronal mass ejections (CMEs) are magnetic phenomena. However,
how magnetic fields reconnecting in the flare differ from nonflaring magnetic fields remains …
how magnetic fields reconnecting in the flare differ from nonflaring magnetic fields remains …
The characteristics of flare-and CME-productive solar active regions
I Kontogiannis - Advances in Space Research, 2023 - Elsevier
Solar flares and coronal mass ejections (CMEs) cause immediate and adverse effects on the
interplanetary space and geospace. In an era of space-based technical civilization, the …
interplanetary space and geospace. In an era of space-based technical civilization, the …
Properties of Flare-imminent versus Flare-quiet Active Regions from the Chromosphere through the Corona. I. Introduction of the AIA Active Region Patches (AARPs)
K Dissauer, KD Leka, EL Wagner - The Astrophysical Journal, 2023 - iopscience.iop.org
We begin here a series of papers examining the chromospheric and coronal properties of
solar active regions. This first paper describes an extensive data set of images from the …
solar active regions. This first paper describes an extensive data set of images from the …
Investigating pre-eruptive magnetic properties at the footprints of erupting magnetic flux ropes
It is well established that solar eruptions are powered by free magnetic energy stored in the
current-carrying magnetic field in the corona. It has also been generally accepted that …
current-carrying magnetic field in the corona. It has also been generally accepted that …
Solar flare predictive features derived from polarity inversion line masks in active regions using an unsupervised machine learning algorithm
J Wang, Y Zhang, SAH Webber, S Liu… - The Astrophysical …, 2020 - iopscience.iop.org
The properties of the polarity inversion line (PIL) in solar active regions (ARs) are strongly
correlated to flare occurrences. The PIL mask, enclosing the PIL areas, has shown …
correlated to flare occurrences. The PIL mask, enclosing the PIL areas, has shown …
Solar active region magnetic parameters and their relationship with the properties of halo coronal mass ejections
A Shanmugaraju, P Vijayalakshmi… - Journal of Atmospheric …, 2023 - Elsevier
The coronal mass ejections (CMEs) from the sun consist of the plasma and strong magnetic
fields (∼ 4–5 G at 1.3 R⊙) and generally, the fast CMEs are often associated with energetic …
fields (∼ 4–5 G at 1.3 R⊙) and generally, the fast CMEs are often associated with energetic …