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High Energy Solar Particle Events and Their Relationship to Associated Flare, CME and GLE Parameters
DOI: 10.1029/2022SW003334 Bibcode: 2023SpWea..2103334W

Vainio, R.; Dalla, S.; Raukunen, O. +3 more

Large solar eruptive events, including solar flares and coronal mass ejections (CMEs), can lead to solar energetic particle (SEP) events. During these events, protons are accelerated up to several GeV and pose numerous space weather risks. These risks include, but are not limited to, radiation hazards to astronauts and disruption to satellites and…

2023 Space Weather
SOHO 14
Detection and Characterization of a Coronal Mass Ejection Using Interplanetary Scintillation Measurements From the Murchison Widefield Array
DOI: 10.1029/2022SW003396 Bibcode: 2023SpWea..2103396M

Morgan, J.; Ekers, R.; McCauley, P. I. +2 more

We have shown previously that the Murchison Widefield Array (MWA), can detect 100s of Interplanetary Scintillation (IPS) sources simultaneously across a field of view (FoV) ∼30° in extent. To test if we can use this capability to track heliospheric structures, we undertook a search of 88 hr of MWA IPS data, and identified an observation likely to …

2023 Space Weather
SOHO 5
Upstream Solar Wind Prediction up to Mars by an Operational Solar Wind Prediction System
DOI: 10.1029/2022SW003281 Bibcode: 2023SpWea..2103281W

Luo, Bingxian; Zhong, Qiuzhen; Liu, Siqing +10 more

Combining the upstream solar wind observations measured by Mars Atmosphere and Volatile Evolution (MAVEN), Advanced Composition Explorer(ACE) and Deep Space Climate Observatory (DSCOVR) from October 2014 to April 2021, we investigate the statistical properties of the background solar wind at Mars and Earth. By applying an operational solar wind pr…

2023 Space Weather
SOHO 3
Partially Erupted Prominence Material as a Diagnostic of Coronal Mass Ejection Trajectory
DOI: 10.1029/2022SW003256 Bibcode: 2023SpWea..2103256H

Thompson, B. J.; Mason, E. I.; Hovis-Afflerbach, B. A.

Coronal mass ejections (CMEs) are energetic releases of large-scale magnetic structures from the Sun. CMEs can have impacts on spacecraft and at Earth. This trajectory is typically assumed to be radial, but often the CME moves outward with some spatial offset from the source region where the eruption initially occurred. A CME is frequently accompa…

2023 Space Weather
SOHO 1
L1 and Off Sun-Earth Line Visible-Light Imaging of Earth-Directed CMEs: An Analysis of Inconsistent Observations
DOI: 10.1029/2022SW003358 Bibcode: 2023SpWea..2103358H

Möstl, Christian; Barnes, David; Davies, Jackie A. +1 more

The efficacy of coronal mass ejection (CME) observations as a key input to space weather forecasting is explored by comparing on and off Sun-Earth line observations from the ESA/NASA SOHO and NASA STEREO spacecraft. A comparison is made of CME catalogs based on L1 coronagraph imagery and off Sun-Earth line coronagraph and heliospheric imager obser…

2023 Space Weather
SOHO 0