Results 151 to 160 of about 288 (182)

Enhanced response of thermospheric cooling emission to negative pressure pulse. [PDF]

Sci Rep
Bag T, Ogawa Y.
europepmc   +1 more source

Origin of reconnecting current sheets in shocked turbulent plasma. [PDF]

Sci Adv
Wang S, Lu S, Lu Q, Wang R, Ren J, Gao X, Guo J.   +6 more
europepmc   +1 more source

SMILE Modeling Working Group: Modeling and Analysis of X-ray and Ultraviolet Images of Solar Wind - Earth Interactions. [PDF]

Space Sci Rev
Connor HK, Sun T, Samsonov A, Liang J, Read A, Li D, Cucho-Padin G, Jung J, Bickner B, Philippe Escoubet C, Forsyth C, Sembay S, Sibeck D, Spanswick E, Sydorenko D, Wang C.   +15 more
europepmc   +1 more source

Ohm's Law, the Reconnection Rate, and Energy Conversion in Collisionless Magnetic Reconnection. [PDF]

Space Sci Rev
Liu YH, Hesse M, Genestreti K, Nakamura R, Burch JL, Cassak PA, Bessho N, Eastwood JP, Phan T, Swisdak M, Toledo-Redondo S, Hoshino M, Norgren C, Ji H, Nakamura TKM.   +14 more
europepmc   +1 more source

The Interplay Between Collisionless Magnetic Reconnection and Turbulence. [PDF]

Space Sci Rev
Stawarz JE, Muñoz PA, Bessho N, Bandyopadhyay R, Nakamura TKM, Eriksson S, Graham DB, Büchner J, Chasapis A, Drake JF, Shay MA, Ergun RE, Hasegawa H, Khotyaintsev YV, Swisdak M, Wilder FD.   +15 more
europepmc   +1 more source

Hyperfine-resolved rovibrational and rotational spectroscopy of OH⁺ (<i>X</i>³Σ^-).

Phys Chem Chem Phys
Silva WGDP, Schneider L, Graf UU, Müller HSP, Jusko P, Jacob AM, Riechers D, Schlemmer S, Asvany O.   +8 more
europepmc   +1 more source

Outstanding Questions and Future Research on Magnetic Reconnection. [PDF]

Space Sci Rev
Nakamura R, Burch JL, Birn J, Chen LJ, Graham DB, Guo F, Hwang KJ, Ji H, Khotyaintsev YV, Liu YH, Oka M, Payne D, Sitnov MI, Swisdak M, Zenitani S, Drake JF, Fuselier SA, Genestreti KJ, Gershman DJ, Hasegawa H, Hoshino M, Norgren C, Shay MA, Shuster JR, Stawarz JE.   +24 more
europepmc   +1 more source

Some of the next articles are maybe not open access.

Related searches:

Planetary bow shocks

Geophysical Monograph Series, 1985
Planetary bow shocks provide insight into both the behavior of collisionless shocks and the nature of the planetary obstacle responsible for creating those bow shocks. This review paper first presents a survey of the microstructure of planetary bow shocks using data obtained at Mercury, Venus, the earth, Mars, Jupiter, and Saturn.
Christopher Russell
exaly   +2 more sources

Overshoots in planetary bow shocks

Nature, 1982
The parametric variation with solar wind conditions in the overshoot in magnetic field strength observed in planetary bow shocks and believed to be associated with the ion reflection process is examined based on both terrestrial and planetary bow shock data.
Christopher Russell, Russell C T
exaly   +2 more sources

A comparative analysis of terrestrial and planetary bow shocks

2011 XXXth URSI General Assembly and Scientific Symposium, 2011
Collisionless shocks, such as the Earth bow shock, are very spectacular and energetic events in the Universe. For instance, generated by supernovae, stellar winds, and the solar wind collisonless shock have important effects. They are considered to be efficient particle accelerators and they act galactic nebula and therefore they are considered to ...
H Kucharek
exaly   +2 more sources