Results 101 to 110 of about 16,204 (260)

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

Observations on a series of merging magnetic flux ropes within an interplanetary coronal mass ejection

open access: yes, 2018
Coronal mass ejections (CMEs) are intense solar explosive eruptions. CMEs are highly important players in solar-terrestrial relationships, and they have important consequences for major geomagnetic storms and energetic particle events.
Feng, Hengqiang   +4 more
core   +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

Automated detection of solar eruptions

open access: yesJournal of Space Weather and Space Climate, 2015
Observation of the solar atmosphere reveals a wide range of motions, from small scale jets and spicules to global-scale coronal mass ejections (CMEs).
Hurlburt N.
doaj   +1 more source

Coronal mass ejections and sunspot number over solar cycle 24

open access: diamond, 2021
Preetam Singh Gour   +2 more
openalex   +1 more source

Cospatial Multiwavelength Observations of an Eruptive Prominence as the Bright Core of a Coronal Mass Ejection

open access: yesThe Astrophysical Journal Letters
Coronal mass ejections (CMEs), as seen in white-light (WL) coronagraphs, often exhibit a classic three-part structure consisting of a bright front, a dark cavity, and a bright core.
Bin Zhuang   +10 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

Solar Energetic Particle Acceleration by a Shock Wave Accompanying a Coronal Mass Ejection in the Solar Atmosphere [PDF]

open access: bronze, 2017
Anastasia Petukhova   +3 more
openalex   +1 more source

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