Results 121 to 130 of about 2,118 (212)
The Astrophysical JournalThe gradient and curvature of the Parker spiral interplanetary magnetic field give rise to curvature and gradient guiding-center drifts on cosmic rays (CRs). The plasma turbulence present in interplanetary space is thought to suppress the drifts; however,
T. Laitinen, S. Dalla
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Division II: Sun and Heliosphere [PDF]
Transactions of the International Astronomical Union, 2001 Arnold O. Benz +6 more
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Solar energetic particles in the inner heliosphere
, 2016 Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2016, Tutora: Neus Agueda CostafredaThe upcoming missions Solar Orbiter (SolO) and Solar Probe Plus (SPP) will explore the inner region of the heliosphere.
Adillón Corbera, Mariona
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Astrospheres and Solar-like Stellar Winds
Living Reviews in Solar Physics, 2004 Stellar analogs for the solar wind have proven to be frustratingly difficult to detect directly. However, these stellar winds can be studied indirectly by observing the interaction regions carved out by the collisions between these winds and the ...
Wood Brian E.
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The Astrophysical Journal Supplement SeriesEnergetic neutral atom (ENA) observations provide valuable insights into the plasma conditions in the heliosphere and the surrounding interstellar medium.
Paweł Swaczyna +2 more
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Earth and Planetary PhysicsResearch on the interstellar medium and its interaction with the solar system constitutes a significant topic in planetary physics. As the Sun traverses the local interstellar cloud, interstellar neutrals penetrate the heliosphere, forming the ...
JiaLing Lyu +3 more
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Solar Wind Turbulence at Kinetic Scales in the Inner Heliosphere
, 2019 International audienceWe study magnetic fluctuations at sub-ion scales and down to sub-electron scales using Helios/SCM measurements in the inner Heliosphere and Cluster/STAFF data at the Earth's orbit.
Shprits, Y. +4 more
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Consequences of Hot Electrons for the Structure of the Outer Heliosphere
The Astrophysical JournalThe temperature of electrons is largely unknown in the outer heliosphere because there is a gap in Voyager measurements from ∼3 eV to 22 keV. Most models assume that the electrons have the same temperature as the bulk cold thermal solar wind (10 ^4 K ...
Ethan Schuyler Bair +5 more
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Dynamical Age of Alfvénic Turbulence in the Solar Wind
The Astrophysical Journal LettersAn evolving turbulent flow like the solar wind can be meaningfully characterized by its “turbulence age”—an estimate of the number of nonlinear times that have elapsed during the plasma’s propagation from the Sun to the point of observation.
Rohit Chhiber +3 more
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Division II: Sun and Heliosphere (Soleil Et Heliosphere) [PDF]
Transactions of the International Astronomical Union, 2007 openaire +1 more source