Results 111 to 120 of about 16,204 (260)
Which Upstream Solar Wind Conditions Matter Most in Predicting Bz within Coronal Mass Ejections
, 2023 Pete Riley +2 more
openalex +1 more source
Two classes of solar energetic particle events associated with impulsive and long duration soft X-ray flares [PDF]
Solar energetic particle events observed in space have different properties depending on the class of associated flare. Impulsive flares, which occur low in the corona in regions of high energy density, are associated with particle events which are ...
Cane, H. V. +2 more
core +1 more source
Quantitative Analysis of CME Deflections in the Corona
, 2011 In this paper, ten CME events viewed by the STEREO twin spacecraft are analyzed to study the deflections of CMEs during their propagation in the corona.
Gui, Bin +6 more
core +1 more source
The Astrophysical JournalWe performed an analysis of the extreme-ultraviolet (EUV) wave event on 2022 March 31. The event originated from active region (AR) 12975 located at N13W52 in the field of view of the Atmospheric imaging Assembly (AIA) and exactly at the west limb viewed
Ramesh Chandra, P. F. Chen, Pooja Devi
doaj +1 more source
Intensity variation of large solar energetic particle events associated with coronal mass ejections [PDF]
, 2004 N. Gopalswamy +4 more
openalex +1 more source
MHD Forecasting of Solar Wind With Coronal Mass Ejections
Space WeatherWe present a model, implemented as an online service, for predicting the speed and density of solar wind in the inner heliosphere and near Earth. The model is based on a numerical magnetohydrodynamics code PLUTO.
S. Arutyunyan +3 more
doaj +1 more source
Characteristics of coronal mass ejections in the near Sun interplanetary space [PDF]
Geofísica Internacional, 2004 Based on the observations from the Large Angle and Spectrometric Coronagraph (LASCO) on board the Solar and Heliospheric Observatory (SOHO) spacecraft we studied coronal mass ejections (CME) parameters between 6 and 10 solar radii from the Sun.
Nat Gopalswamy +2 more
doaj
Workshop on Solar Activity, Solar Wind, Terrestrial Effects, and Solar Acceleration [PDF]
A summary of the proceedings from the workshop are presented. The areas covered were solar activity, solar wind, terrestrial effects, and solar acceleration.
core +1 more source
Role of coronal mass ejections in the heliospheric Hale cycle [PDF]
, 2007 [1] The 11-year solar cycle variation in the heliospheric magnetic field strength can be explained by the temporary buildup of closed flux released by coronal mass ejections (CMEs).
Crooker, N. U. +4 more
core +1 more source