Results 81 to 90 of about 8,519 (215)

Coronal dimming and the coronal mass ejection onset [PDF]

, 2003
R. A. Harrison, P. Bryans, G. M. Simnett, M. A. Lyons   +3 more
openalex   +1 more source

Energy Conversion and Exchange in a Magnetosheath Jet

Journal of Geophysical Research: Space Physics, Volume 130, Issue 11, November 2025.
Abstract Magnetosheath jets are regions with an extremely large dynamic pressure compared to that of the background plasma. We present a case study of a magnetosheath jet examining energy conversion processes and its interaction with the surrounding magnetosheath plasma.
O. W. Roberts, Z. Vörös, A. Settino, F. Koller, S. Raptis, M. Temmer, C. Simon Wedlund, X. Li, R. Nakamura   +8 more
wiley   +1 more source

Ensemble Simulations of Coronal Mass Ejections in Interplanetary Space with Elliptical Cone Models [PDF]

Johan Muhamad, Tiar Dani, Muhamad Zamzam Nurzaman, Rasdewita Kesumaningrum, Santi Sulistiani, Farahhati Mumtahana, Gerhana Puannandra Putri, Ayu Dyah Pangestu, Ahmad Zulfiana Utama   +8 more
openalex   +3 more sources

Multi-instrument observations and tracking of a coronal mass ejection front from low to middle corona

Journal of Space Weather and Space Climate
The shape and dynamics of coronal mass ejections (CMEs) vary significantly based on the instrument and wavelength used. This has led to significant debate about the proper definitions of CME/shock fronts, pile-up/compression regions, and core ...
Stepanyuk Oleg, Kozarev Kamen
doaj   +1 more source

Solar Mini-Dimming Kinematics and Their Positive Correlations with Coronal Mass Ejections and Prominence [PDF]

, 2013
Nasibe Alipour, Hossein Safari
openalex   +1 more source

Spatial Variability and Correlation Lengths Within Stream Interaction Regions at 1 au: Comparison Between ACE and Wind

Journal of Geophysical Research: Space Physics, Volume 130, Issue 11, November 2025.
Abstract Understanding the spatial variability and correlation lengths throughout Stream Interaction Regions (SIRs) has importance both for fundamentally understanding the structuring of the solar wind and SIRs and for space weather operations. SIR observations from Advanced Composition Explorer and Wind are utilized to characterize the spatial ...
R. C. Allen, V. Toy‐Edens, S. K. Vines, S. Eriksson, J. M. Raines, S. Lepri, G. Li, Y. Wu, A. Russell, G. C. Ho   +9 more
wiley   +1 more source

A Deep Learning Method for Automatic Coronal Mass Ejection Feature Identification

The Astrophysical Journal Supplement Series
Coronal mass ejections (CMEs), intense solar eruptive phenomena, are the primary drivers of extreme space weather storms on Earth. As space activities become increasingly frequent and infrastructure more reliant on space-based systems, the rapid and ...
P. Yang, H. S. Fu, J. B. Cao, F. Shen
doaj   +1 more source

Observations of Core Fallback during Coronal Mass Ejections [PDF]

, 2002
Y.‐M. Wang, N. R. Sheeley
openalex   +1 more source

Serendipitous observation of a coronal mass ejection during the total solar eclipse of 14 December 2020

, 2021
Guillermo Abramson
openalex   +2 more sources

Can Spacecraft‐Borne Contamination Compromise Our Understanding of Lunar Ice Chemistry?

Journal of Geophysical Research: Planets, Volume 130, Issue 11, November 2025.
Abstract Recent detections of water ice in the permanently shadowed regions (PSRs) at the lunar poles have reignited scientific and commercial interest in the exploration of Earth's closest neighbor. The frigid temperatures in PSRs operate as cold traps for volatiles and may represent large reservoirs of materials, including water ice and prebiotic ...
Francisca S. Paiva, Silvio Sinibaldi
wiley   +1 more source