Results 21 to 30 of about 5,692 (228)
The Electron Structure of the Solar Wind
Frontiers in Astronomy and Space Sciences, 2021 Time-series measurements of the number density ncore and temperature Tcore of the core-electron population of the solar wind are examined at 1 AU and at 0.13 AU using measurements from the WIND and Parker Solar Probe spacecraft, respectively.
Joseph E. Borovsky +2 more
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Global asymmetry of the heliosphere [PDF]
AIP Conference Proceedings, 2006 6 pages, 5 figures, AIP Proceedings of the 5th IGPP "The Physics of the Inner Heliosheath: Voyager Observations, Theory and Future Prospects"
Opher, Merav +3 more
openaire +3 more sources
MANIFESTATIONS OF TWO BRANCHES OF SOLAR ACTIVITY IN THE HELIOSPHERE AND GCR INTENSITY
Solar-Terrestrial Physics, 2019 This paper provides insight into heliospheric processes and galactic cosmic ray (GCR) modulation occurring due to the presence of two branches of solar activity in this solar layer.
Krainev M.B.
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Redefining flux ropes in heliophysics
Frontiers in Astronomy and Space Sciences, 2023 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
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Plasma Dynamics in Low-Electron-Beta Environments
Frontiers in Astronomy and Space Sciences, 2021 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
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Solar energetic particle time series analysis with Python
Frontiers in Astronomy and Space Sciences, 2022 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
Frontiers in Astronomy and Space Sciences, 2021 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
Additional acceleration of solar-wind particles in current sheets of the heliosphere [PDF]
, 2015 Particles of fast solar wind in the vicinity of the heliospheric current sheet (HCS) or in a front of interplanetary coronal mass ejections (ICMEs) often reveal very peculiar energy or velocity profiles, density distributions with double or triple peaks,
V. Zharkova +4 more
core +1 more source
Modeling of the heliospheric interface: multi-component nature of the heliospheric plasma [PDF]
Astronomy & Astrophysics, 2005 A&A ...
Malama, Yury G. +2 more
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The Astrophysical Journal, 2021 Abstract In late 2016, the Interstellar Boundary Explorer (IBEX) observed an enhancement of hydrogen energetic neutral atom (ENA) flux in ∼20° south from the nose direction. This enhancement was a consequence of an abrupt increase of the solar wind (SW) dynamic pressure observed at 1 au in late 2014.
Justyna M. Sokół +5 more
openaire +1 more source