Results 121 to 130 of about 30,967 (299)

Solar origins of coronal mass ejections [PDF]

open access: yes
The large scale properties of coronal mass ejections (CMEs), such as morphology, leading edge speed, and angular width and position, have been cataloged for many events observed with coronagraphs on the Skylab, P-78, and SMM spacecraft.
Kahler, Stephen
core   +1 more source

Solar Coronal Mass Ejection and Post–Coronal Mass Ejection Blob Formation in Two-fluid Simulations

open access: yesThe Astrophysical Journal
Abstract A coronal mass ejection (CME) and post-CME blob phenomena in the solar atmosphere, associated with shear flow and convergent flow perturbations in the photosphere, are investigated using a resistive two-fluid (electron–ion) code. It is found that there are notable deviations between the two-fluid and previous magnetohydrodynamic
J. C. Du, Z. W. Ma
openaire   +2 more sources

Evolution of Anemone AR NOAA 10798 and the Related Geo-Effective Flares and CMEs

open access: yes, 2008
We present a detailed examination of the features of the Active Region (AR) NOAA 10798. This AR generated coronal mass ejections (CMEs) that caused a large geomagnetic storm on 24 August 2005 with the minimum Dst index of -216 nT.
Alexander   +63 more
core   +1 more source

Coronal Mass Ejections and Solar Radio Emissions (invited) [PDF]

open access: yesPLANETARY RADIO EMISSIONS VII, 2011
Three types of low-frequency nonthermal radio bursts are associated with coronal mass ejections (CMEs): Type III bursts due to accelerated electrons propagating along open magnetic field lines, type II bursts due to electrons accelerated in shocks, and type IV bursts due to electrons trapped in post-eruption arcades behind CMEs.
openaire   +1 more source

Quantitative Analysis of CME Deflections in the Corona

open access: yes, 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

Large-scale Coronal Dimming Foreshadowing a Solar Eruption on 2011 October 1

open access: yesThe Astrophysical Journal
Understanding large-scale solar eruptions requires detailed investigation of the entire system’s evolution, including the magnetic environment enveloping the source region and searches for precursor activity prior to event onset.
Chunming Zhu   +6 more
doaj   +1 more source

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

open access: yesThe 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   +4 more
doaj   +1 more source

Characteristics of Magnetic Clouds and Interplanetary Coronal Mass Ejections which Cause Intense Geomagnetic Storms

open access: yesTerrestrial, Atmospheric and Oceanic Sciences, 2013
We present the results of a statistical data analysis of the geo-effectiveness of non-magnetic-cloud interplanetary coronal mass ejections (ICMEs) and compare them with those of magnetic-cloud (MC) interplanetary coronal mass ejections observed during ...
Chin-Chun Wu   +3 more
doaj   +1 more source

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