Results 251 to 260 of about 54,745 (274)

Geoeffectivity of Coronal Mass Ejections

Space Science Reviews, 2007
Coronal mass ejections and post-shock streams driven by them are the most efficient drivers of strong magnetospheric activity, magnetic storms. For this reason there is considerable interest in trying to make reliable forecasts for the effects of CMEs as much in advance as possible. To succeed this requires understanding of all aspects related to CMEs,
H. E. J. Koskinen, K. E. J. Huttunen
openaire   +1 more source

The Interaction of Successive Coronal Mass Ejections: A Review

, 2016
We present a review of the different aspects associated with the interaction of successive coronal mass ejections (CMEs) in the corona and inner heliosphere, focusing on the initiation of series of CMEs, their interaction in the heliosphere, the particle
N. Lugaz, M. Temmer, Yuming Wang, C. Farrugia   +3 more
semanticscholar   +1 more source

Coronal Mass Ejections and Magnetic Helicity

2005
Coronal mass ejections (CMEs) are the most energetic events in the solar system, expelling up to 1016 g of coronal material at speeds of several hundreds or thousands of km s−1 from the Sun. As CMEs are the primary cause of space weather disturbances, we need to understand their underlying cause(s) in order to be able to predict them. After an overview
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Deceleration of Coronal Mass Ejections

Solar Physics, 2001
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Cross helicity of interplanetary coronal mass ejections at 1 au

Monthly Notices of the Royal Astronomical Society, 2022
Simon Good, Matti Ala-Lahti, A Osmane
exaly  

Effects of solar flares and coronal mass ejections on Earth’s horizontal magnetic field and solar wind parameters during the minimum solar cycle 24

Monthly Notices of the Royal Astronomical Society, 2021
R Umar, Nor Hazmin Sabri, A Yoshikawa
exaly  

Type II radio bursts and their association with coronal mass ejections in solar cycles 23 and 24

Astronomy and Astrophysics, 2023
Anshu Kumari, D E Morosán, E K J Kilpua   +2 more
exaly  

Forbush decreases associated with coronal mass ejections from active and non-active regions: statistical comparison

Monthly Notices of the Royal Astronomical Society, 2022
A A Melkumyan, A V Belov, M A Abunina
exaly  

In-Situ Solar Wind and Magnetic Field Signatures of Interplanetary Coronal Mass Ejections

Space Science Reviews, 2006
T H Zurbuchen, I G Richardson, Zurbuchen Thomas H   +2 more
exaly  

Hannibal the Coronal (mass ejection)

Tre intensi brillamenti solari in tre giorni, dalla regione attiva Ar 4274, ai quali hanno fatto seguito altrettante espulsioni coronali di massa dirette verso il nostro pianeta. Nelle prossime ore potrebbero in parte sovrapporsi, dando luogo a una forte tempesta geomagnetica.
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