Results 21 to 30 of about 19,278 (241)
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
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
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Extracting Inner‐Heliosphere Solar Wind Speed Information From Heliospheric Imager Observations [PDF]
AbstractWe present evidence that variability in the STEREO‐A Heliospheric Imager (HI) data is correlated with in situ solar wind speed estimates from WIND, STEREO‐A, and STEREO‐B. For 2008–2012, we compute the variability in HI differenced images in a plane‐of‐sky shell between 20 to 22.5 solar radii and, for a range of position angles, compare daily ...
L. A. Barnard +3 more
openaire +2 more sources
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
Expansion of magnetic clouds in the outer heliosphere [PDF]
A large amount of magnetized plasma is frequently ejected from the Sun as coronal mass ejections (CMEs). Some of these ejections are detected in the solar wind as magnetic clouds (MCs) that have flux rope signatures.
A. M. Gulisano +45 more
core +4 more sources
Evolving outer heliosphere: Large-scale stability and time variations observed by the Interstellar Boundary Explorer [PDF]
The first all-sky maps of Energetic Neutral Atoms (ENAs) from the Interstellar Boundary Explorer (IBEX) exhibited smoothly varying, globally distributed flux and a narrow ribbon of enhanced ENA emissions.
Bzowski, M. +14 more
core +2 more sources
The long-term variability of cosmic ray protons in the heliosphere: A modeling approach
Galactic cosmic rays are charged particles created in our galaxy and beyond. They propagate through interstellar space to eventually reach the heliosphere and Earth. Their transport in the heliosphere is subjected to four modulation processes: diffusion,
M.S. Potgieter +4 more
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
Heliospheric plasma sheets [PDF]
As a high‐beta feature on scales of hours or less, the heliospheric plasma sheet (HPS) encasing the heliospheric current sheet shows a high degree of variability. A study of 52 sector boundaries identified in electron pitch angle spectrograms in Wind data from 1995 reveals that only half concur with both high‐beta plasma and current sheets, as required
Crooker, N. U. +5 more
openaire +2 more sources

