A time dependent three-dimensional simulation of the earth's magnetosphere - Reconnection events
(Previously announced in STAR as N82-20718)
Engineering topics
Publications and source records attributed to Hain, K..
(Previously announced in STAR as N82-20718)
The effect of adding a By magnetic component to a solar wind already carrying a Bz magnetic component is studied using three-dimensional MHD computer simulations. It is found that the tail structure and the Bx lobe fields are rotated and become asymmetric. In addition, a By component is generated in the neutral sheet. These results are found to correlate with observational data.
Numerical solution to problems of theta pinches and solar flares in strong magnetic fields
Program to draw flowcharts automatically from PERT, Fortran II, Fortran IV, or FAP cards
Logical structure of automatic flow chart design, describing element ordering and sorting
Automatic flow chart design using computer program written in Fortran
Hydromagnetic waves in plasma with isotropic and nonisotropic pressure perpendicular to a magnetic field