Results 21 to 30 of about 15,397 (165)
Redefining flux ropes in heliophysics
Magnetic flux ropes manifest as twisted bundles of magnetic field lines. They carry significant amounts of solar mass in the heliosphere. This paper underlines the need to advance our understanding of the fundamental physics of heliospheric flux ropes ...
Teresa Nieves-Chinchilla +32 more
doaj +1 more source
Plasma Dynamics in Low-Electron-Beta Environments
Recent in situ measurements by the MMS and Parker Solar Probe missions bring interest to small-scale plasma dynamics (waves, turbulence, magnetic reconnection) in regions where the electron thermal energy is smaller than the magnetic one.
Stanislav Boldyrev +3 more
doaj +1 more source
Exclusion of Tiny Interstellar Dust Grains from the Heliosphere [PDF]
The distribution of interstellar dust grains (ISDG) observed in the Solar System depends on the nature of the interstellar medium-solar wind interaction.
Avinash, K. +13 more
core +2 more sources
Solar energetic particle time series analysis with Python
Solar Energetic Particles (SEPs) are charged particles accelerated within the solar atmosphere or the interplanetary space by explosive phenomena such as solar flares or Coronal Mass Ejections (CMEs). Once injected into the interplanetary space, they can
Christian Palmroos +8 more
doaj +1 more source
In this report some properties of the electron strahl at 1 AU are examined to assess the strahl at 272 eV as an indicator of the quality of the magnetic connection of the near-Earth solar wind to the Sun.
Joseph E. Borovsky
doaj +1 more source
Improving Predictions of High‐Latitude Coronal Mass Ejections Throughout the Heliosphere
Predictions of the impact of coronal mass ejections (CMEs) in the heliosphere mostly rely on cone CME models, whose performances are optimized for locations in the ecliptic plane and at 1 AU (e.g., at Earth).
C. Scolini +4 more
doaj +1 more source
The large-scale structure and evolution of the solar wind are typically reproduced with reasonable fidelity using three-dimensional magnetohydrodynamic (MHD) models.
Opal Issan , Pete Riley
doaj +1 more source
What is the heliopause? Importance of magnetic reconnection and measurement requirements
We highlight the importance of magnetic reconnection at the heliopause, both as one of the key processes driving the interaction between solar and interstellar media, but also as an element of the definition of the heliopause itself.
B. Lavraud +24 more
doaj +1 more source
Complementary interstellar detections from the heliotail
The heliosphere is a protective shield around the solar system created by the Sun’s interaction with the local interstellar medium (LISM) through the solar wind, transients, and interplanetary magnetic field.
Sarah A. Spitzer +5 more
doaj +1 more source
On the importance of investigating CME complexity evolution during interplanetary propagation
This perspective paper brings to light the need for comprehensive studies on the evolution of interplanetary coronal mass ejection (ICME) complexity during propagation. To date, few studies of ICME complexity exist.
Réka M. Winslow +29 more
doaj +1 more source

