Numerical simulations of shocks encountering clumpy regions

Author： Alūzas R.   Pittard J. M.   Hartquist T. W.   Falle S. A. E. G.   Langton R.  

Publisher： Oxford University Press

ISSN： 0035-8711

Source： Monthly Notices of the Royal Astronomical Society, Vol.425, Iss.3, 2012-09, pp. : 2212-2227

Disclaimer: Any content in publications that violate the sovereignty, the constitution or regulations of the PRC is not accepted or approved by CNPIEC.

Previous Menu Next

Abstract

Related content

Structure and stationarity of quasi-perpendicular shocks: Numerical simulations

By Hellinger P.  

Planetary and Space Science, Vol. 51, Iss. 11, 2003-09 ,pp. : 649-657

Elsevier

Access to resources Recommend Favorite

Numerical MHD Simulations of Solar Magnetoconvection and Oscillations in Inclined Magnetic Field Regions

By Kitiashvili I.   Kosovichev A.   Mansour N.   Wray A.  

Solar Physics, Vol. 268, Iss. 2, 2011-02 ,pp. : 283-291

Springer Publishing Company

Access to resources Recommend Favorite

High-redshift clumpy discs and bulges in cosmological simulations

By Ceverino Daniel   Dekel Avishai   Bournaud Frederic  

Monthly Notices of the Royal Astronomical Society, Vol. 404, Iss. 4, 2010-06 ,pp. : 2151-2169

Oxford University Press

Access to resources Recommend Favorite

Numerical overcooling in shocks

By Creasey Peter   Theuns Tom   Bower Richard G.   Lacey Cedric G.  

Monthly Notices of the Royal Astronomical Society, Vol. 415, Iss. 4, 2011-08 ,pp. : 3706-3720

Oxford University Press

Access to resources Recommend Favorite

Laboratory Simulations of Bow Shocks and Magnetospheres

By Horton W.  

Astrophysics and Space Science, Vol. 298, Iss. 1-2, 2005-07 ,pp. : 395-401

Springer Publishing Company

Access to resources Recommend Favorite