D. J. Scheeres, E. G. Fahnestock, S. J. Ostro, S. B. Broschart, ...
Simulation equations and model computation The specific equations of motion solved for our simulations are stated in a compact form as (1): m¨ri = Uri (1) ˙H I i = −T I ijɛjklT I mkU T I ml (2)...
Belitski, A., Gretton, A., Magri, C., Murayama, Y., Montemurro, M.A., Logothetis, N.K., ...
Local field potentials (LFPs) reflect subthreshold integrative processes that complement spike train measures. However, little is yet known about the differences between how LFPs and spikes encode...
Radar images of asteroid 100085 (1992 UY4) (2006)
Benner, Lance A. M., Busch, M. W., Ostro, S. J., Giorgini, J. D., Hine, A. A., Harmon, J. K., ...
NASA/JPL
Magri, C., Ostro, S. J., Rosema, K. D., Thomas, M. L., Mitchell, D. L., Campbell, D. B., ...
We report detailed results of Arecibo and Goldstone radar observations of 30 mainbelt asteroids (MBAs) during 1980-1997. In addition to estimates of radar cross section, radar albedo, and circular...
Plans for Radar Imaging of Asteroid 216 Kleopatra (2004)
Ostro, S., Hudson, R., Nolan, M., Magri, C., Campbell, D., Giorgini, J., ...
Radar observations of asteroid 216 Kleopatra (2004)
Ostro, S., Hudson, R., Nolan, M., Margot, J., Scheeres, D., Campbell, D., ...
Radar observations of the main-belt, M-class asteroid 216 Kleopatra reveal a dumbbell-shaped object with overall dimensions of 217 kilometers by 94 kilometers by 81 kilometers (+/-25%). The...