Parker solar probe: Four years of discoveries at solar cycle minimum
Abstract Launched on 12 Aug. 2018, NASA's Parker Solar Probe had completed 13 of its
scheduled 24 orbits around the Sun by Nov. 2022. The mission's primary science goal is to …
scheduled 24 orbits around the Sun by Nov. 2022. The mission's primary science goal is to …
Large gradual solar energetic particle events
M Desai, J Giacalone - Living Reviews in Solar Physics, 2016 - Springer
Solar energetic particles, or SEPs, from suprathermal (few keV) up to relativistic (∼∼ few
GeV) energies are accelerated near the Sun in at least two ways:(1) by magnetic …
GeV) energies are accelerated near the Sun in at least two ways:(1) by magnetic …
Diffusive shock acceleration simulations of radio relics
Recent radio observations have identified a class of structures, so-called radio relics, in
clusters of galaxies. The radio emission from these sources is interpreted as synchrotron …
clusters of galaxies. The radio emission from these sources is interpreted as synchrotron …
[HTML][HTML] Shock propagation and associated particle acceleration in the presence of ambient solar-wind turbulence
The topic of this review paper is on the influence of solar wind turbulence on shock
propagation and its consequence on the acceleration and transport of energetic particles at …
propagation and its consequence on the acceleration and transport of energetic particles at …
Electron injection by whistler waves in non-relativistic shocks
MA Riquelme, A Spitkovsky - The Astrophysical Journal, 2011 - iopscience.iop.org
Electron acceleration to non-thermal, ultra-relativistic energies (∼ 10–100 TeV) is revealed
by radio and X-ray observations of shocks in young supernova remnants (SNRs). The …
by radio and X-ray observations of shocks in young supernova remnants (SNRs). The …
Turbulence-dominated shock waves: 2D hybrid kinetic simulations
M Nakanotani, GP Zank, LL Zhao - The Astrophysical Journal, 2022 - iopscience.iop.org
We investigate the interaction of turbulence with shock waves by performing 2D hybrid
kinetic simulations. We inject force-free magnetic fields upstream that are unstable to the …
kinetic simulations. We inject force-free magnetic fields upstream that are unstable to the …
Energetic electron observations by Parker Solar Probe/IS⊙ IS during the first widespread SEP event of solar cycle 25 on 2020 November 29
JG Mitchell, GA De Nolfo, ME Hill… - The Astrophysical …, 2021 - iopscience.iop.org
At the end of 2020 November, two coronal mass ejections (CMEs) erupted from the Sun and
propagated through the interplanetary medium in the direction of Parker Solar Probe while …
propagated through the interplanetary medium in the direction of Parker Solar Probe while …
Radio observations of coronal mass ejection initiation and development in the low solar corona
EP Carley, N Vilmer, A Vourlidas - Frontiers in Astronomy and Space …, 2020 - frontiersin.org
Coronal mass ejections (CMEs) are large eruptions of plasma and magnetic field from the
low solar corona into the heliosphere. These eruptions are often associated with energetic …
low solar corona into the heliosphere. These eruptions are often associated with energetic …
Flare versus shock acceleration of high-energy protons in solar energetic particle events
EW Cliver - The Astrophysical Journal, 2016 - iopscience.iop.org
Recent studies have presented evidence for a significant to dominant role for a flare-resident
acceleration process for high-energy protons in large (" gradual") solar energetic particle …
acceleration process for high-energy protons in large (" gradual") solar energetic particle …
Imaging-spectroscopy of a band-split type II solar radio burst with the Murchison Widefield Array
Type II solar radio bursts are caused by magnetohydrodynamic (MHD) shocks driven by
solar eruptive events such as coronal mass ejections (CMEs). Often, both fundamental and …
solar eruptive events such as coronal mass ejections (CMEs). Often, both fundamental and …