Results 231 to 240 of about 16,204 (260)

3D Patchy Reconnection in Solar Coronal Mass Ejections

IEEE Conference Record - Abstracts. 2005 IEEE International Conference on Plasma Science, 2005
Summary form only given. Coronal mass ejections (CME's), sudden eruptions of coronal plasma and magnetic field into the interplanetary medium, are one of the most dynamic phenomena in the solar corona. These CME's are an important driver of space weather both through their interaction with the Earth's magnetosphere and through the magnetic reconnection
Mark G. Linton, Dana W. Longcope, Spiro K. Antiochos   +2 more
openaire   +1 more source

The solar sources of coronal mass ejections

2008
Despite nearly two decades of observations and study of coronal mass ejections (CMEs), the question of the physical and phenomenological origins of CMEs remains unanswered. This question has been addressed in several different types of studies, each having important limitations.
openaire   +1 more source

The source regions of solar coronal mass ejections

Solar Physics, 1990
Knowledge of the origin of the solar coronal mass ejection (CME) may be crucial to our understanding of several active solar phenomena, such as flares, as well as to the structure and stability of the corona and the prediction of interplanetary disturbances.
openaire   +1 more source

The Solar Cycle Dependence of Coronal Mass Ejections

1986
The Solwind white light coronagraph on P78-1 has been making routine observations of the solar corona since 28 March 1979. Data from the 1984/1985 time period has just been analyzed. During this interval, a period of low solar activity, coronal mass ejections (CMEs) occurred at the rate of 0.2– 0.4/day, in contrast to the rate of 1.8/day during the ...
R. A. Howard, N. R. Sheeley, D. J. Michels, M. J. Koomen   +3 more
openaire   +1 more source

Coronal mass ejections: Relationship with solar flares and coronal holes

2002
Abstract The Coronal Mass Ejections (CMEs) observed by the LASCO coronagraph and associated solar activity phenomena whose locations were identified by EIT and solar Hα flare observations during year 2000 indicate that about 40%, 26% and 30% of CMEs were observed when there were coronal holes (CHs) within 1–10, 11–20 and 21–40 degrees, respectively
openaire   +1 more source

Solar Radar Detection of Coronal Mass Ejections (CMEs)

2000
Abstract : This report results from a contract tasking Institute of Radio Astronomy (RIAN) as follows: The contractor will investigate the use of powerful HF radars to detect coronal mass ejections from the sun.
openaire   +1 more source

Tailoring inorganic–polymer composites for the mass production of solid-state batteries

Nature Reviews Materials, 2021
Li-Zhen Fan, Hongcai He, Ce-Wen Nan
exaly  

Artificial channels for confined mass transport at the sub-nanometre scale

Nature Reviews Materials, 2021
Jie Shen, Gong-Ping Liu, Yu Han
exaly  

Molecular engineering of contact interfaces for high-performance perovskite solar cells

Nature Reviews Materials, 2022
Furkan H Isikgor, Shingis Zhumagali, Iain McCulloch   +2 more
exaly  

Obesity and adverse breast cancer risk and outcome: Mechanistic insights and strategies for intervention

Ca-A Cancer Journal for Clinicians, 2017
Cynthia Morata-Tarifa, Joyce M Slingerland   +1 more
exaly