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 …
Prediction and Verification of Parker Solar Probe Solar Wind Sources at 13.3 R⊙
Drawing connections between heliospheric spacecraft and solar wind sources is a vital step
in understanding the evolution of the solar corona into the solar wind and contextualizing in …
in understanding the evolution of the solar corona into the solar wind and contextualizing in …
Using Parker Solar Probe observations during the first four perihelia to constrain global magnetohydrodynamic models
P Riley, R Lionello, RM Caplan, C Downs… - Astronomy & …, 2021 - aanda.org
Context. Parker Solar Probe (PSP) is providing an unprecedented view of the Sun's corona
as it progressively dips closer into the solar atmosphere with each solar encounter. Each set …
as it progressively dips closer into the solar atmosphere with each solar encounter. Each set …
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 …
Application of a modified spheromak model to simulations of coronal mass ejection in the inner heliosphere
The magnetic fields of interplanetary coronal mass ejections (ICMEs), which originate close
to the Sun in the form of a flux rope, determine their geoeffectiveness. Therefore, robust flux …
to the Sun in the form of a flux rope, determine their geoeffectiveness. Therefore, robust flux …
Three-Dimensional MHD Modeling of Interplanetary Solar Wind Using Self-Consistent Boundary Condition Obtained from Multiple Observations and Machine …
Y Yang, F Shen - Universe, 2021 - mdpi.com
Three-dimensional (3-d) magnetohydrodynamics (MHD) modeling is a key method for
studying the interplanetary solar wind. In this paper, we introduce a new 3-d MHD solar wind …
studying the interplanetary solar wind. In this paper, we introduce a new 3-d MHD solar wind …
Impact of solar magnetic field amplitude and geometry on cosmic rays diffusion coefficients in the inner heliosphere
Cosmic rays are remarkable tracers of solar events when they are associated with solar
flares, but also galactic events such as supernova remnants when they come from outside …
flares, but also galactic events such as supernova remnants when they come from outside …
Tracking IMF fluctuations nearby Sun using wavelet analysis: Parker solar probe first encounter data
Abstract The Parker Solar Probe (PSP) satellite was launched by NASA in 2018 to study the
Sun's environment from a closer distance than any spacecraft has ever reached before …
Sun's environment from a closer distance than any spacecraft has ever reached before …
Improving the Arrival Time Estimates of Coronal Mass Ejections by Using Magnetohydrodynamic Ensemble Modeling, Heliospheric Imager Data, and Machine …
The arrival time prediction of coronal mass ejections (CMEs) is an area of active research.
Many methods with varying levels of complexity have been developed to predict CME …
Many methods with varying levels of complexity have been developed to predict CME …
Magnetohydrodynamic Simulation of a Coronal Mass Ejection Observed During the Near-radial Alignment of Solar Orbiter and Earth
Interplanetary Coronal Mass Ejections (ICMEs) are the primary sources of geomagnetic
storms at Earth. Negative out-of-ecliptic component (Bz) of magnetic field in the ICME or its …
storms at Earth. Negative out-of-ecliptic component (Bz) of magnetic field in the ICME or its …