Results 131 to 140 of about 150,775 (261)

Multiwavelength Study of M8.9/3B Solar Flare from AR NOAA 10960

, 2010
We present a multi-wavelength analysis of a long duration white-light solar flare (M8.9/3B) event that occurred on 4 June 2007 from NOAA AR 10960. The flare was observed by several spaceborne instruments, namely SOHO/MDI, Hinode/SOT, TRACE and STEREO ...
A. K. Srivastava, A.K. Srivastava, B. Filippov, B. Filippov, B. Kliem, B.P. Filippov, C. Liu, C.L. Gerrard, D. Nandy, D.M. Rust, D.R. Williams, G.A. Gary, H. Ji, H. Wang, H. Wang, J. Krall, J. Lin, K.H. Schatten, M.D. Altschuler, P. Kumar, P.C. Liewer, P.H. Scherrer, Pankaj Kumar, R. Liu, R.C. Canfield, S. Min, S. Tsuneta, S.F. Gissot, S.K. Antiochos, T. Amari, T. Török, T. Török, T.G. Forbes, T.T. Ishii, T.T. Ishii, W. Tend van, Wahab Uddin, Y. Fan, Y. Liu   +38 more
core   +1 more source

Solar flare accelerates nearly all electrons in a large coronal volume. [PDF]

Nature, 2022
Fleishman GD, Nita GM, Chen B, Yu S, Gary DE.   +4 more
europepmc   +1 more source

The solar flare environment [PDF]

Solar flare environment - solar atmosphere, photosphere, chromosphere, corona, and solar flare types, model, occurence, prediction, and ...
Roberts, W. T.
core   +1 more source

Seismic Emissions from a Highly Impulsive M6.7 Solar Flare

, 2008
On 10 March 2001 the active region NOAA 9368 produced an unusually impulsive solar flare in close proximity to the solar limb. This flare has previously been studied in great detail, with observations classifying it as a type 1 white-light flare with a ...
A. Kosovichev, A.-C. Donea, A.-C. Donea, A.-C. Donea, A.-C. Donea, C. Lindsey, D. Besliu-Ionescu, H. Moradi, H. Moradi, J. Aboudarham, J. C. Martínez-Oliveros, J.C. Martínez-Oliveros, J.J. Sudol, J.P. Li, M. Aschwanden, M.D. Ding, M.E. Machado, R. Chandra, S.P. Rajaguru, V.V. Zharkova, V.V. Zharkova, V.V. Zharkova, W. Uddin, Y. Liu   +23 more
core   +3 more sources

Two Types of Solar Confined Flares [PDF]

arXiv, 2019
With the aim of understanding the physical mechanisms of confined flares, we selected 18 confined flares during 2011-2017, and classified the confined flares into two types based on their different dynamic properties and magnetic configurations. "Type I" of confined flares are characterized by slipping reconnection, strong shear, and stable filament ...
arxiv  

A New Model of Solar Flares

The Astrophysical Journal, 1964
Abstract : A model is proposed for solar flares, involving a slow build-up of the pre-flare configuration in which gases circulate in the chromosphere and corona. At some stage this configuration becomes unstable and the flash phase of the flare occurs.
Peter A. Sturrock, B. Coppi
openaire   +4 more sources

Data set for solar flare prediction using helioseismic and magnetic imager vector magnetic field data. [PDF]

Data Brief, 2021
Hollanda A, Antunes Da Silva AE, Cinto T.   +2 more
europepmc   +1 more source

Observation of a Solar Flare at 4.3-mm. Wave-length [PDF]

, 1958
R. J. Coates
openalex   +1 more source

Temporal Variation of Flare Occurrence Rates via the Spot Evolution on the Sun and Solar-type Stars [PDF]

arXiv
The spot evolution on the Sun and solar-type stars is important for understanding the nature of consequential flaring activity. This study statistically investigates the variance of flare occurrence rate through the time evolution of spots on the Sun and solar-type stars.
arxiv  

On the Increase in Cosmic Ray Intensity and the Electromagnetic State in Interplanetary Space during the Solar Flare of Feb. 23, 1956 [PDF]

, 1958
D. Eckhartt
openalex   +1 more source