Calibrating the BHB star distance scale and the halo kinematic distance to the Galactic Centre
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Computer program to calculate geomagnetically trapped particle shell model, drift rate, and bounce paths
Reduced gravity, pressure suit and load effect on human self-locomotion on lunar surface
Statistical space velocity distributions, gravitation field strength and vertex deviation for nearby young stars, using density wave theory of galactic spirals
A computer program which determines the geographic location of the auroral oval for given universal time and level of geomagnetic activity was developed for use on the IBM 7094 computer. The program provides both printed output of geographic coordinates of auroral oval boundaries and polar plots of the auroral oval. In addition, there is available a time-integration option which indicates how long a given location is under the auroral oval during a specified period. A description is given of the program and its use.
The nebular (O II) lambda 3726 and (O III) lambda 5007 radial velocity measures of Wilson, et al (1959) are presented in contour map form. The space motions of theta 1 and theta 2 Orionis and the nebular measures are discussed.