Results 91 to 100 of about 15,851 (215)

Spatial Relationship between CMEs and Prominence Eruptions during SC 24 and SC 25

The Astrophysical Journal
During their propagation, coronal mass ejections (CMEs) and prominences sometimes display a nonradial motion. During the years after the solar minimum, the CME central position angle tended to be offset closer to the equator compared to that of the ...
Kostadinka Koleva, Nat Gopalswamy, Pooja Devi, Seiji Yashiro, Grzegorz Michalek   +4 more
doaj   +1 more source

Serendipitous observation of a coronal mass ejection during the total solar eclipse of 14 December 2020

, 2021
Guillermo Abramson
openalex   +2 more sources

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, J. Américo González-Esparza, Alejandro Lara   +2 more
doaj  

First Simultaneous In Situ Measurements of a Coronal Mass Ejection by Parker Solar Probe and STEREO-A [PDF]

, 2021
R. M. Winslow, Noé Lugaz, Camilla Scolini, A. B. Galvin   +3 more
openalex   +1 more source

On flare-CME characteristics from Sun to Earth combining remote-sensing image data with in-situ measurements supported by modeling

, 2017
We analyze the well observed flare-CME event from October 1, 2011 (SOL2011-10-01T09:18) covering the complete chain of action - from Sun to Earth - for a better understanding of the dynamic evolution of the CME and its embedded magnetic field.
Dissauer, K., Hinterreiter, J., Rodriguez, L., Temmer, M., Thalmann, J. K., Tschernitz, J., Veronig, A. M.   +6 more
core   +1 more source

Direct Evidence of the Hybrid Nature of Extreme-ultraviolet Waves and the Reflection of the Fast-mode Wave

The Astrophysical Journal
We 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

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., Mcguire, R. E., Vonrosenvinge, T. T.   +2 more
core   +1 more source

Can solar wind viscous drag account for CME deceleration?

, 2012
The forces acting on solar Coronal Mass Ejections (CMEs) in the interplanetary medium have been evaluated so far in terms of an empirical drag coefficient $C_{\rm D} \sim 1$ that quantifies the role of the aerodynamic drag experienced by a typical CME ...
Borgazzi, Andrea, Lara, Alejandro, Subramanian, Prasad   +2 more
core   +1 more source

Transport in the interplanetary medium of coronal mass ejections [PDF]

Geofísica Internacional, 2008
Coronal mass ejections (CMEs) are large scale structures of plasma and magnetic field expelled from the Sun to the interplanetary medium and generally observed in white light coronagraphs.
A. Ventura, A. Lara, A. Borgazzi
doaj  

Probabilistic forecasting of ionospheric scintillation and GNSS receiver signal tracking performance at high latitudes

Annals of Geophysics, 2013
At high latitudes, phase scintillation occurs predominantly on the dayside in the ionospheric footprint of the magnetospheric cusp, and in the nightside auroral oval. A new technique of probabilistic forecasting of phase scintillation occurrence relative
Paul Prikryl, Veettil Sreeja, Marcio Aquino, Periyadan T. Jayachandran   +3 more
doaj   +1 more source