Abstract
We present a new 180th degree and order model of the Venus gravity field directly derived from line of sight Magellan residual Doppler data instead of usual line of sight residual acceleration data. We discuss the influence of the a priori covariance matrices on the deconvolution process, and compare our results with previous solutions.
Cite
CITATION STYLE
APA
Barriot, J. P., Valès, N., Balmino, G., & Rosenblatt, P. (1998). A 180th degree and order model of the Venus gravity field from Magellan line of sight residual Doppler data. Geophysical Research Letters, 25(19), 3743–3746. https://doi.org/10.1029/98GL02600
Register to see more suggestions
Mendeley helps you to discover research relevant for your work.
Already have an account? Sign in
Sign up for free