Results 171 to 180 of about 2,661,265 (220)

Electric Fields Can Assist Prebiotic Reactivity on Hydrogen Cyanide Surfaces. [PDF]

ACS Cent Sci
Cappelletti M, Sandström H, Rahm M.
europepmc   +1 more source

Cosmic Ray Irradiation of Interstellar Ices on Sulfur-Rich Grains: A Possible Source of Sulfur-Bearing Molecules. [PDF]

ACS Earth Space Chem
Mifsud DV, Kaňuchová Z, Auriacombe O, Herczku P, Qasim D, Kovács STS, Rácz R, Sulik B, Juhász Z, Rajta I, Vajda I, Biri S, McCullough RW, Ioppolo S, Raut U, Mason NJ.   +15 more
europepmc   +1 more source

Photochemical Haze Formation on Titan and Uranus: A Comparative Review. [PDF]

Int J Mol Sci
Dubois D.
europepmc   +1 more source

Uncovering the integral spectral characteristics of the planetary nebula IC 4642. [PDF]

Sci Rep
Mohery M, Ali A, Hamam KA, Khames AA, Alsubaie AS.   +4 more
europepmc   +1 more source

Perpendicular ion heating in turbulence and reconnection: magnetic moment breaking by coherent fluctuations. [PDF]

J Plasma Phys
Mallet A, Klein K, Chandran BDG, Ervin T, Bowen TA.   +4 more
europepmc   +1 more source

Revealing an unexpectedly low electron injection threshold via reinforced shock acceleration. [PDF]

Nat Commun
Raptis S, Lalti A, Lindberg M, Turner DL, Caprioli D, Burch JL.   +5 more
europepmc   +1 more source

Compact Spatial Heterodyne Spectrographs for Future Space-Based Observations: Instrument Modeling and Applications. [PDF]

Sensors (Basel)
Sahoo A, Mathew J, Battisti A, Tucker B.
europepmc   +1 more source

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Interaction of the interstellar medium with the solar wind

Space Science Reviews, 1973
The possibilities for making observations of the region of interaction between the solar wind and the interstellar medium, and of the interstellar medium itself, are discussed. It is emphasized that missions to the outer planets undertaken in 1977–1979 are ideally suited for making such observations.
W I Axford
exaly   +2 more sources

Gasdynamics of the solar wind interaction with the interstellar medium

Space Science Reviews, 1990
A survey of the present-day situation in gasdynamical models of solar wind interaction with the local interstellar medium is presented. A role of these models in interpreting a number of observed physical phenomena is investigated. Experimental data and possible observations are considered from the viewpoint of their interpretation on the basis of ...
V B Baranov
exaly   +2 more sources