Results 131 to 140 of about 652 (175)

Theory and observations of the interaction between magnetohydrodynamic waves and shocks. [PDF]

Proc Natl Acad Sci U S A
Zhao L, Zhu X, Silwal A, Zank GP, Pitňa A.   +4 more
europepmc   +1 more source

Flux equipartition in astrophysical plasma turbulence. [PDF]

Sci Adv
Marino R, Xie JH.
europepmc   +1 more source

The Electric Field Instrument (EFI) for the TRACERS Mission. [PDF]

Space Sci Rev
Bonnell JW, Ludlam M, Slagle A, Goodrich K, LaBelle JW.   +4 more
europepmc   +1 more source

Future opportunities in solar system plasma science through ESA's exploration programme. [PDF]

NPJ Microgravity
Holmstrom M, Lester M, Sanchez-Cano B.
europepmc   +1 more source

Electromotive field in space and astrophysical plasmas. [PDF]

Rev Mod Plasma Phys
Bourdin PA, Narita Y.
europepmc   +1 more source

The Compact Dual Ion Composition Experiment (CoDICE) for the IMAP Mission. [PDF]

Space Sci Rev
Livi SA, Desai MI, Ogasawara K, Kistler L, Möbius E, Starkey MJ, Dayeh MA, Kataria D, Elliott HA, Hart S, Alterman B, McComas DJ, Pollock CJ, Mukherjee J, Trevino J, Ferrell S, Brenner T, Pope SE, Tapley M, Pavlas K, Rankin JS, Shen MM, Khoo L, Alimaganbetov M, Teifert J, Roemer EM, Shaw-Lecerf M, Escobar J, Christian ER, Schwadron NA, Gkioulidou M, Grubbs G, Brysch M, Epperly M, George D, Dunn G, Ford J, Schwendeman CL, Commons M, Persyn S, Jaskulek S, Weidner S, Bert C, Ferris M, Rodriguez B, Nunez C, Urdiales C, Cortinas S, Rodriguez H.   +48 more
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The Sun and Heliosphere at Solar Maximum

Science, 2003
Recent Ulysses observations from the Sun's equator to the poles reveal fundamental properties of the three-dimensional heliosphere at the maximum in solar activity. The heliospheric magnetic field originates from a magnetic dipole oriented nearly perpendicular to, instead of nearly parallel to, the Sun's rotation axis.
David J McComas, Louis J. Lanzerotti, M Landgraf   +2 more
exaly   +5 more sources

Sun–Heliosphere Observation-based Ionization Rates Model [PDF]

Astrophysical Journal, 2020
Abstract The solar wind (SW) and the extreme ultraviolet (EUV) radiation modulate fluxes of interstellar and heliospheric particles inside the heliosphere both in time and in space. Understanding this modulation is necessary to correctly interpret measurements of particles of interstellar origin inside the heliosphere.
David J McComas, Munetoshi Tokumaru, Justyna M. Sokół   +2 more
exaly   +3 more sources

The Sun and the Heliosphere in Three Dimensions

Astrophysics and Space Science Library, 1986
Section I: The Corona.- Coronal Magnetic Fields - a Mini Survey.- Origins of the Solar Wind in the Corona.- The Heliospheric Energy Source.- Coronal Spectroscopy and Imaging from Spartan during the Polar Passage of Ulysses.- The Structure and Rotation of the Solar Corona: Implications for the Heliosphere.- OVI Diagnostics of Solar Wind Generation ...
exaly   +2 more sources

MAGNETIZED JETS DRIVEN BY THE SUN: THE STRUCTURE OF THE HELIOSPHERE REVISITED [PDF]

Astrophysical Journal Letters, 2015
19 pages, 5 figures; Astrophysical Journal Letters; in ...
Tamás G. Gombosi, Merav Opher, James F. Drake   +2 more
exaly   +4 more sources