Driving Dynamical Inner‐Heliosphere Models With In Situ Solar Wind Observations
Accurately reconstructing the solar wind throughout the inner heliosphere is essential for understanding solar–terrestrial interactions and improving space‐weather forecasts.
M. J. Owens +10 more
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Modeling observations of solar coronal mass ejections with heliospheric imagers verified with the Heliophysics System Observatory. [PDF]
Möstl C +21 more
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This study examines the statistical properties of coronal mass ejections (CMEs) over two and a half solar cycles (1996–2025) using coronal observations from the SOHO LASCO CDAW and CACTus catalogs, supplemented by sunspot number records and in situ ...
Olga Khabarova +4 more
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Turn on the super-elastic collision nature of coronal mass ejections through low approaching speed. [PDF]
Shen F, Wang Y, Shen C, Feng X.
europepmc +1 more source
Solar Coronal Mass Ejection Modeling
Final presentations of the Center for Astrophysics HEA/SSP Solar Summer Intern Program.
openaire +1 more source
Observations of successive CMEs and their successive Type II solar radio bursts in the corona. [PDF]
Vasanth V.
europepmc +1 more source
Magnetoacoustic wave propagation in the solar corona and filament dynamics. [PDF]
Somaiyeh S, Stefaan P.
europepmc +1 more source
Simulating high-speed solar wind streams from coronal holes using an L5-L1 configuration of lagrangian points. [PDF]
Podladchikova T +3 more
europepmc +1 more source
Martian ionospheric response during the may 2024 solar superstorm. [PDF]
Parrott J +7 more
europepmc +1 more source
Global ozone loss following extreme solar proton storms based on the July 2012 coronal mass ejection. [PDF]
Kalakoski N +3 more
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