Results 151 to 160 of about 1,165,809 (269)

Plasma Turbulence and Stochastic Acceleration in Solar Flares [PDF]

, 1999
V. Petrosian
openalex   +1 more source

MICROWAVE TYPE III PAIR BURSTS IN SOLAR FLARES [PDF]

, 2016
Baolin Tan, Hana Meszarosova, Marian Karlický, Guang-li Huang, Chengming Tan, Baolin Tan, Hana Meszarosova, Marian Karlický, Guang-li Huang, Chengming Tan   +9 more
openalex   +1 more source

Recent Observations of Energetic Electrons in Solar Flares [PDF]

, 1980
S. R. Kane
openalex   +1 more source

Magnetic Field Evolution Leading to Solar Flares I. Cases with Low Magnetic Shear and Flux Emergence [PDF]

, 2000
Hui Li, Takashi Sakurai, Kiyoshi Ichimoto, S. Ueno   +3 more
openalex   +1 more source

Monitoring of solar far ultraviolet radiation from the OSO-5 satellite [PDF]

A spectrophotometer for monitoring the solar EUV in three broad wavelength bands is described. The kind of data obtained, along with sources of error, are presented. The content of the tape library which contains the data is outlined.
Parker, R., Rense, W. A.
core   +1 more source

Constraining the Mass Loss and the Kinetic Energy of Stellar Coronal Mass Ejections with Solar Far-ultraviolet Flares

The Astrophysical Journal
Stellar eruptive events, such as flares and coronal mass ejections (CMEs), can affect planetary habitability by disturbing the stability of their atmospheres.
Nuri Park, Evgenya L. Shkolnik, Joe Llama   +2 more
doaj   +1 more source

Time-Series Feature Selection for Solar Flare Forecasting

Universe
Solar flares are significant occurrences in solar physics, impacting space weather and terrestrial technologies. Accurate classification of solar flares is essential for predicting space weather and minimizing potential disruptions to communication ...
Yagnashree Velanki, Pouya Hosseinzadeh, Soukaina Filali Boubrahimi, Shah Muhammad Hamdi   +3 more
doaj   +1 more source

Solar Flares Triggered by a Filament Peeling Process Revealed by High-resolution GST Hα Observations

The Astrophysical Journal Letters
The dynamic structures of solar filaments prior to solar flares provide important physical clues about the onset of solar eruptions. Observations of those structures under subarcsecond resolution with high cadence are rare.
Mia Mancuso, Ju Jing, Haimin Wang, Wenda Cao   +3 more
doaj   +1 more source

Neutron and gamma ray production in the 1991 June X-class flares [PDF]

We present new calculations of pion radiation and neutron emission from solar flares. We fit the recently reported high energy GAMMA-1 observations with pion radiation produced in a solar flare magnetic loop. We calculate the expected neutron emission in
Hua, X. M., Kozlovsky, B., Lingenfelter, R. E., Mandzhavidze, N., Ramaty, R.   +4 more
core   +1 more source

Multiclass Classification of Solar Flares in Imbalanced Data Using Ensemble Learning and Sampling Methods

Proceedings of the International Florida Artificial Intelligence Research Society Conference
Solar flares are intense bursts of radiation across the electromagnetic spectrum on the surface of the Sun. They are categorized into four classes: B, C, M, and X, depending on their intensity, with X-class flares being the strongest.
Haodi Jiang, Ryoma Matsuura, Jason T. L. Wang   +2 more
doaj   +1 more source