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Multi-source connectivity as the driver of solar wind variability in the heliosphere
The ambient solar wind that fills the heliosphere originates from multiple sources in the solar
corona and is highly structured. It is often described as high-speed, relatively homogeneous …
corona and is highly structured. It is often described as high-speed, relatively homogeneous …
[HTML][HTML] Stirring the base of the solar wind: On heat transfer and vortex formation
Context. Current models of the solar wind must approximate (or ignore) the small-scale
dynamics within the solar atmosphere; however, these are likely important in sha** the …
dynamics within the solar atmosphere; however, these are likely important in sha** the …
Direct evidence for magnetic reconnection at the boundaries of magnetic switchbacks with Parker Solar Probe
Context. The first encounters of Parker Solar Probe (PSP) with the Sun revealed the
presence of ubiquitous localised magnetic deflections in the inner heliosphere; these …
presence of ubiquitous localised magnetic deflections in the inner heliosphere; these …
Flux rope merging and the structure of switchbacks in the solar wind
A major discovery of Parker Solar Probe (PSP) was the presence of large numbers of
localized increases in the radial solar wind speed and associated sharp deflections of the …
localized increases in the radial solar wind speed and associated sharp deflections of the …
On the Origin of the Sudden Heliospheric Open Magnetic Flux Enhancement During the 2014 Pole Reversal
Coronal holes are recognized as the primary sources of heliospheric open magnetic flux
(OMF). However, a noticeable gap exists between in situ measured OMF and that derived …
(OMF). However, a noticeable gap exists between in situ measured OMF and that derived …
The contribution of alpha particles to the solar wind angular momentum flux in the inner heliosphere
Context. An accurate assessment of the Sun's angular momentum (AM) loss rate is an
independent constraint for models that describe the rotation evolution of Sun-like stars …
independent constraint for models that describe the rotation evolution of Sun-like stars …
Statistical evidence for small-scale interchange reconnection at a coronal hole boundary
Much of coronal hole (CH) research is focused upon determining the boundary and
calculating the open flux as accurately as possible. However, the observed boundary itself is …
calculating the open flux as accurately as possible. However, the observed boundary itself is …
Non-Gaussian speed distributions: OMNI multisatellite data and simulations based on two temperature model
A Shah, Q UL-Haque, S Mahmood… - Physics of Plasmas, 2022 - pubs.aip.org
The multi-satellite OMNI solar wind speed data are analyzed, and six distinct types of non-
Gaussian probability distributions are investigated. These include the three and four peak …
Gaussian probability distributions are investigated. These include the three and four peak …