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Waves in the lower solar atmosphere: the dawn of next-generation solar telescopes
Waves and oscillations have been observed in the Sun's atmosphere for over half a century.
While such phenomena have readily been observed across the entire electromagnetic …
While such phenomena have readily been observed across the entire electromagnetic …
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 …
[HTML][HTML] The solar orbiter mission-science overview
Aims. Solar Orbiter, the first mission of ESA's Cosmic Vision 2015–2025 programme and a
mission of international collaboration between ESA and NASA, will explore the Sun and …
mission of international collaboration between ESA and NASA, will explore the Sun and …
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 …
First results from the solar orbiter heavy ion sensor
Aims. Solar Orbiter launched in February 2020 with the goal of revealing the connections
between the Sun's interior, atmosphere, and the heliosphere. The Solar Orbiter Heavy Ion …
between the Sun's interior, atmosphere, and the heliosphere. The Solar Orbiter Heavy Ion …
Observation of Alfvén wave reflection in the solar chromosphere: Ponderomotive force and first ionization potential effect
We investigate the propagation of Alfvén waves in the solar chromosphere, distinguishing
between upward and downward propagating waves. We find clear evidence for the …
between upward and downward propagating waves. We find clear evidence for the …
How do shock waves define the space-time structure of gradual solar energetic particle events?
We revisit the full variety of observed temporal and spatial distributions of energetic solar
protons in “gradual” solar energetic-particle (SEP) events resulting from the spatial …
protons in “gradual” solar energetic-particle (SEP) events resulting from the spatial …
Defining the middle corona
The middle corona, the region roughly spanning heliocentric distances from 1.5 to 6 solar
radii, encompasses almost all of the influential physical transitions and processes that …
radii, encompasses almost all of the influential physical transitions and processes that …
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 …
Four distinct pathways to the element abundances in solar energetic particles
Based upon recent evidence from abundance patterns of chemical elements in solar
energetic particles (SEPs), and, ironically, the belated inclusion of H and He, we can …
energetic particles (SEPs), and, ironically, the belated inclusion of H and He, we can …