[HTML][HTML] Coronal mass ejections: Observations
DF Webb, TA Howard - Living Reviews in Solar Physics, 2012 - Springer
Solar eruptive phenomena embrace a variety of eruptions, including flares, solar energetic
particles, and radio bursts. Since the vast majority of these are associated with the eruption …
particles, and radio bursts. Since the vast majority of these are associated with the eruption …
Understanding the origins of problem geomagnetic storms associated with “stealth” coronal mass ejections
NV Nitta, T Mulligan, EKJ Kilpua, BJ Lynch… - Space Science …, 2021 - Springer
Geomagnetic storms are an important aspect of space weather and can result in significant
impacts on space-and ground-based assets. The majority of strong storms are associated …
impacts on space-and ground-based assets. The majority of strong storms are associated …
Nine outstanding questions of solar wind physics
NM Viall, JE Borovsky - Journal of Geophysical Research …, 2020 - Wiley Online Library
In situ measurements of the solar wind have been available for almost 60 years, and in that
time plasma physics simulation capabilities have commenced and ground‐based solar …
time plasma physics simulation capabilities have commenced and ground‐based solar …
Mesoscale structure in the solar wind
Structures in the solar wind result from two basic mechanisms: structures injected or
imposed directly by the Sun, and structures formed through processing en route as the solar …
imposed directly by the Sun, and structures formed through processing en route as the solar …
Compositional Metrics of Fast and Slow Alfvénic Solar Wind Emerging from Coronal Holes and Their Boundaries
We seek to understand the composition and variability of fast solar wind (FSW) and slow
Alfvénic solar wind emerging from coronal holes (CHs). We leverage an opportune …
Alfvénic solar wind emerging from coronal holes (CHs). We leverage an opportune …
Relating streamer flows to density and magnetic structures at the Parker solar probe
AP Rouillard, A Kouloumvakos… - The Astrophysical …, 2020 - iopscience.iop.org
The physical mechanisms that produce the slow solar wind are still highly debated. Parker
Solar Probe's (PSP's) second solar encounter provided a new opportunity to relate in situ …
Solar Probe's (PSP's) second solar encounter provided a new opportunity to relate in situ …
Overview of the remote sensing observations from PSP solar encounter 10 with perihelion at 13.3 R⊙
The closest perihelion pass of Parker Solar Probe (PSP), so far, occurred between 2021
November 16 and 26 and reached∼ 13.29 R☉ from Sun center. This pass resulted in very …
November 16 and 26 and reached∼ 13.29 R☉ from Sun center. This pass resulted in very …
Reconstruction and prediction of variations in the open solar magnetic flux and interplanetary conditions
M Lockwood - Living Reviews in Solar Physics, 2013 - Springer
Historic geomagnetic activity observations have been used to reveal centennial variations in
the open solar flux and the near-Earth heliospheric conditions (the interplanetary magnetic …
the open solar flux and the near-Earth heliospheric conditions (the interplanetary magnetic …
Flux rope and dynamics of the heliospheric current sheet-study of the parker solar probe and solar orbiter conjunction of June 2020
Context. Solar Orbiter and Parker Solar Probe jointly observed the solar wind for the first
time in June 2020, capturing data from very different solar wind streams: calm, Alfvénic wind …
time in June 2020, capturing data from very different solar wind streams: calm, Alfvénic wind …
Detection of small magnetic flux ropes from the third and fourth Parker Solar Probe encounters
Context. Aims. We systematically search for magnetic flux rope structures in the solar wind to
within the closest distance to the Sun of~ 0.13 AU, using data from the third and fourth orbits …
within the closest distance to the Sun of~ 0.13 AU, using data from the third and fourth orbits …