Results 131 to 140 of about 16,696 (216)

Solar Cycle Variation of the Mass-loss Rate of Coronal Mass Ejections

The Astrophysical Journal Supplement Series
Coronal mass ejections (CMEs) are known as the main drivers of the most severe space weather disturbances. Usually, the most severe geomagnetic storms are caused by massive and fast CMEs.
Yijia Tang, Xiaojuan Zhang, Hui Deng, Feng Wang, Linhua Deng, Ying Mei   +5 more
doaj   +1 more source

Why Could a Newborn Active Region Produce Coronal Mass Ejections?

The Astrophysical Journal
Solar active regions (ARs) are the main sources of flares and coronal mass ejections (CMEs). NOAA AR 12089, which emerged on 2014 June 10, produced two C-class flares accompanied by CMEs within 5 hr after its emergence.
Hanzhao Yang, Lijuan Liu
doaj   +1 more source

Modeling observations of solar coronal mass ejections with heliospheric imagers verified with the Heliophysics System Observatory. [PDF]

Space Weather, 2017
Möstl C, Isavnin A, Boakes PD, Kilpua EKJ, Davies JA, Harrison RA, Barnes D, Krupar V, Eastwood JP, Good SW, Forsyth RJ, Bothmer V, Reiss MA, Amerstorfer T, Winslow RM, Anderson BJ, Philpott LC, Rodriguez L, Rouillard AP, Gallagher P, Nieves-Chinchilla T, Zhang TL.   +21 more
europepmc   +1 more source

Turn on the super-elastic collision nature of coronal mass ejections through low approaching speed. [PDF]

Sci Rep, 2016
Shen F, Wang Y, Shen C, Feng X.
europepmc   +1 more source

Solar Coronal Mass Ejection Modeling

, 2014
Final presentations of the Center for Astrophysics HEA/SSP Solar Summer Intern Program.
openaire   +1 more source

Global ozone loss following extreme solar proton storms based on the July 2012 coronal mass ejection. [PDF]

Sci Rep, 2023
Kalakoski N, Verronen PT, Szeląg ME, Jackman CH.   +3 more
europepmc   +1 more source

History of two mass loss processes in VY CMa. [PDF]

Proc Int Astron Union, 2023
Quintana-Lacaci G, Velilla L, Fonfría JP, Cernicharo J, Castro-Carrizo A, Agúndez M, Decin L.   +6 more
europepmc   +1 more source

Turbulent convection as a significant hidden provider of magnetic helicity in solar eruptions. [PDF]

Sci Rep, 2023
Toriumi S, Hotta H, Kusano K.
europepmc   +1 more source

Observations of successive CMEs and their successive Type II solar radio bursts in the corona. [PDF]

Sci Rep
Vasanth V.
europepmc   +1 more source

Measuring the magnetic fields in the chromospheres of low-mass stars [PDF]

Nat Commun
Cang T, Petit P, Donati J, Tian H, Fu J, Li H, Bellotti S, Hu X, Ma X, Ariste AL, Xing K, Morin J, Lu H, Zong W.   +13 more
europepmc   +2 more sources