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Science (New York, N.Y.)|October 12, 1984
Venus: volcanism and rift formation in Beta regioD B Campbell, J W Head, J K Harmon, et al.Science (New York, N.Y.)|January 21, 2006
Formation of glaciers on Mars by atmospheric precipitation at high obliquityF Forget, R M Haberle, F Montmessin, et al.Science (New York, N.Y.)|May 6, 1994
Global variations in the geoid/topography admittance of venusM Simons, B H Hager, S C SolomonScience (New York, N.Y.)|August 12, 1983
Reports: venus: identification of banded terrain in the mountains of ishtar terraD B Campbell, J W Head, J K Harmon, et al.Science (New York, N.Y.)|March 10, 2000
Internal structure and early thermal evolution of Mars from Mars Global Surveyor topography and gravityM T Zuber, S C Solomon, R J Phillips, et al.Science (New York, N.Y.)|January 11, 1991
Venus southern hemisphere: geologic character and age of terrains in the themis-alpha-lada regionD B Campbell, D A Senske, J W Head, et al.Applied Optics|February 21, 2008
Imaging spectroscopy for two-dimensional characterization of auroral emissionsG R Swenson, R L Rairden, S C Solomon, et al.Science (New York, N.Y.)|December 11, 1999
Possible ancient oceans on Mars: evidence from Mars Orbiter Laser Altimeter dataJ W Head, H Hiesinger, M A Ivanov, et al.Science (New York, N.Y.)|November 27, 1992
The seismic attenuation structure of a fast-spreading mid-ocean ridgeW S Wilcock, S C Solomon, G M Purdy, et al.Science (New York, N.Y.)|June 29, 2023
Gullies on Mars could have formed by melting of water ice during periods of high obliquityJ L Dickson, A M Palumbo, J W Head, et al.Pageof 4