Statistics – Computation
Scientific paper
Feb 1980
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980jgr....85..727p&link_type=abstract
Journal of Geophysical Research, vol. 85, Feb. 1, 1980, p. 727-743.
Statistics
Computation
16
Adiabatic Flow, Hydrodynamics, Numerical Flow Visualization, Solar Wind, Three Dimensional Flow, Three Dimensional Models, Astronomical Models, Computational Fluid Dynamics, Streams, Transport Properties
Scientific paper
Theoretical aspects of corotating solar wind dynamics on a global scale are examined by means of numerical simulations executed with a nonlinear, inviscid, adiabatic, single fluid, three-dimensional hydrodynamic formulation. The factors most strongly affecting stream evolution, namely, the intrinsic correlations among density, temperature, and velocity existing near the source, the amplitude, longitudinal breadth and latitudinal breadth of the stream, and the heliographic latitude of the centroid of the stream, are considered. Calculations indicate that even in the presence of substantial meridional gradients, the latitudinal transport of mass, energy, and momentum by streams appears to have little impact on the overall evolution of the structure.
No associations
LandOfFree
A three-dimensional model of corotating streams in the solar wind. II - Hydrodynamic streams does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with A three-dimensional model of corotating streams in the solar wind. II - Hydrodynamic streams, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A three-dimensional model of corotating streams in the solar wind. II - Hydrodynamic streams will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1621320