Results 131 to 140 of about 705 (177)

Atacama Large Aperture Submillimeter Telescope (AtLAST) Science: Planetary and Cometary Atmospheres. [PDF]

Open Res Eur
Cordiner M, Thelen A, Cavalie T, Cosentino R, Fletcher LN, Gurwell M, de Kleer K, Kuan YJ, Lellouch E, Moullet A, Nixon C, de Pater I, Teanby N, Butler B, Charnley S, Milam S, Moreno R, Booth M, Klaassen P, Cicone C, Mroczkowski T, Di Mascolo L, Johnstone D, van Kampen E, Lee M, Liu D, Maccarone T, Saintonge A, Smith M, Wedemeyer S.   +29 more
europepmc   +1 more source

Discs no more: the morphology of low-mass simulated galaxies in FIREbox. [PDF]

Mon Not R Astron Soc
Benavides JA, Sales LV, Wetzel A, Moreno J, Feldmann R, Mercado FJ, Bullock JS, Hopkins PF, Faucher-Giguère CA, Stern J, Wheeler C, Kereš D.   +11 more
europepmc   +1 more source

Magnetic star-planet interaction in the young exoplanet system DS Tucanae Ab

Santos Ld, Owen J, Duvvuri G, Loyd ROP, Vidotto A, Presa A, Bourrier V, King G, Airapetian V, Ehrenreich D, France K, Lendl M, Lothringer J, Nielsen L.   +13 more
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, Axford W I, 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, Baranov V B
exaly   +2 more sources

Effects of Interstellar and Solar Wind Ionized Helium on the Interaction of the Solar Wind with the Local Interstellar Medium

Astrophysical Journal, 2003
The Sun is moving through a warm ($\sim$6500 K) and partly ionized local interstellar cloud (LIC) with a velocity of $\sim$26 km/s. Recent measurements of the ionization of the LIC (Wolff et al., 1999) suggest that interstellar helium in the vicinity of the Sun is 30-40 % ionized, while interstellar hydrogen is less ionized.
Vladislav Izmodenov
exaly   +3 more sources

Anisotropic fluid turbulence in the interstellar medium and solar wind

Physics of Plasmas, 2003
The interstellar medium and solar wind is permeated by a magnetic field that renders magnetohydrodynamic turbulence anisotropic. In the classic work of Iroshnikov [Astron. Zh. 40, 742 (1963)] and Kraichnan [Phys. Fluids 8, 1385 (1965)], it is assumed that the turbulence is isotropic, and an inertial range energy spectrum that scales as k−3/2 is deduced
Amitava Bhattacharjee, Kai Germaschewski, Bhattacharjee A   +2 more
exaly   +2 more sources

The interaction of the solar wind and stellar winds with the partially ionized interstellar medium

Physics of Plasmas, 2001
Plasmas in the laboratory and interstellar and interplanetary space are frequently partially ionized. Thus, the solar wind and stellar winds often interact with an interplanetary medium that is an admixture of protons, electrons, other charged ions, and neutral atoms.
Wood B E, Zank G P
exaly   +2 more sources

INTERACTION OF THE SOLAR WIND WITH THE LOCAL INTERSTELLAR MEDIUM

25th International Cosmic Ray Conference — Volume 8, 1995
First results from a two‐dimensional (axisymmetric) time‐dependent gas dynamic model for the interaction of the solar wind with the local interstellar medium are presented. The model includes the mutual influence of the interstellar and interplanetary plasma (protons and electrons) and the neutral interstellar hydrogen atoms. Neutrals created by charge
H. L. Pauls, G. P. Zank, L. L. Williams
openaire   +1 more source

Interaction Between the Solar Wind and the Interstellar Medium

Annual Review of Astronomy and Astrophysics, 1989
The heliospheric and interstellar parameters of importance in the interaction between the solar wind and the ISM are discussed. The observationally inferred values of these parameters, including the uncertainties, are addressed, and the basic physical processes that are likely to be important in the interaction are examined theoretically. The theory is
exaly   +2 more sources