Laurence Soderblom, PhD (Former Employee)
Science and Products
Filter Total Items: 137
Preliminary geological mapping of Io Preliminary geological mapping of Io
Terrain units and their global distribution on Io are summarised. A map of the complex region of Io is also presented. ?? 1979 Nature Publishing Group.
Authors
H. Masursky, G. G. Schaber, L.A. Soderblom, R.G. Strom
The Jupiter system through the eyes of Voyager 1 The Jupiter system through the eyes of Voyager 1
The cameras aboard Voyager 1 have provided a closeup view of the Jupiter system, revealing heretofore unknown characteristics and phenomena associated with the planet's atmosphere and the surfaces of its five major satellites. On Jupiter itself, atmospheric motions—the interaction of cloud systems—display complex vorticity. On its dark side, lightning and auroras are observed. A ring was
Authors
B.A. Smith, L.A. Soderblom, T. V. Johnson, A.P. Ingersoll, S.A. Collins, E.M. Shoemaker, G.E. Hunt, H. Masursky, M. H. Carr, M. E. Davies, A.F. Cook, J. Boyce, G. E. Danielson, Tobias Owen, C. Sagan, R.F. Beebe, J. Veverka, R.G. Strom, J.F. McCauley, D. Morrison, G.A. Briggs, V.E. Suomi
Apollo over the Moon: A view from orbit Apollo over the Moon: A view from orbit
No abstract available.
Authors
Harold Masursky, G. W. Colton, Farouk El-Baz, Frederick J. Doyle, Richard E. Eggleton, Maurice J. Grolier, James W. Head, Carroll Ann Hodges, Keith A. Howard, Leon J. Kosofsky, Baerbel K. Lucchitta, Michael C. McEwen, Henry J. Moore, Gerald G. Schaber, David H. Scott, Laurence A. Soderblom, Mareta West, D.E. Wilhems
Global color variations on the Martian surface Global color variations on the Martian surface
Surface materials exposed throughout the equatorial region of Mars have been classified and mapped on the basis of spectral reflectance properties determined by the Viking II Orbiter vidicon cameras. Frames acquired at each of three wavelengths (0.45 ± 0.03 μm, 0.53 ± 0.05 μm, and 0.59 ± 0.05 μm) during the approach of Viking Orbiter II in Martian summer (Ls = 105°) were mosaicked by...
Authors
L.A. Soderblom, K. Edwards, E. M. Eliason, E.M. Sanchez, M.P. Charette
Possible fossil H2O liquid-ice interfaces in the Martian crust Possible fossil H2O liquid-ice interfaces in the Martian crust
Throughout the northern equatorial region of Mars, extensive areas have been uniformly stripped, roughly to a constant depth. These terrains vary widely in their relative ages. A model is described here to explain this phenomenon as reflecting the vertical distribution of H2O liquid and ice in the crust. Under present conditions the Martian equatorial regions are stratified in terms of...
Authors
L.A. Soderblom, D. B. Wenner
Voyager imaging experiment Voyager imaging experiment
The overall objective of this experiment is exploratory reconnaissance of Jupiter, Saturn, their satellites, and Saturn's rings. Such reconnaissance, at resolutions and phase angles unobtainable from Earth, can be expected to provide much new data relevant to the atmospheric and/or surface properties of these bodies. The experiment also has the following specific objectives: Observe and
Authors
B.A. Smith, G.A. Briggs, G. E. Danielson, A.F. Cook, M. E. Davies, G.E. Hunt, H. Masursky, L.A. Soderblom, T.C. Owen, C. Sagan, V.E. Suomi
Science and Products
Filter Total Items: 137
Preliminary geological mapping of Io Preliminary geological mapping of Io
Terrain units and their global distribution on Io are summarised. A map of the complex region of Io is also presented. ?? 1979 Nature Publishing Group.
Authors
H. Masursky, G. G. Schaber, L.A. Soderblom, R.G. Strom
The Jupiter system through the eyes of Voyager 1 The Jupiter system through the eyes of Voyager 1
The cameras aboard Voyager 1 have provided a closeup view of the Jupiter system, revealing heretofore unknown characteristics and phenomena associated with the planet's atmosphere and the surfaces of its five major satellites. On Jupiter itself, atmospheric motions—the interaction of cloud systems—display complex vorticity. On its dark side, lightning and auroras are observed. A ring was
Authors
B.A. Smith, L.A. Soderblom, T. V. Johnson, A.P. Ingersoll, S.A. Collins, E.M. Shoemaker, G.E. Hunt, H. Masursky, M. H. Carr, M. E. Davies, A.F. Cook, J. Boyce, G. E. Danielson, Tobias Owen, C. Sagan, R.F. Beebe, J. Veverka, R.G. Strom, J.F. McCauley, D. Morrison, G.A. Briggs, V.E. Suomi
Apollo over the Moon: A view from orbit Apollo over the Moon: A view from orbit
No abstract available.
Authors
Harold Masursky, G. W. Colton, Farouk El-Baz, Frederick J. Doyle, Richard E. Eggleton, Maurice J. Grolier, James W. Head, Carroll Ann Hodges, Keith A. Howard, Leon J. Kosofsky, Baerbel K. Lucchitta, Michael C. McEwen, Henry J. Moore, Gerald G. Schaber, David H. Scott, Laurence A. Soderblom, Mareta West, D.E. Wilhems
Global color variations on the Martian surface Global color variations on the Martian surface
Surface materials exposed throughout the equatorial region of Mars have been classified and mapped on the basis of spectral reflectance properties determined by the Viking II Orbiter vidicon cameras. Frames acquired at each of three wavelengths (0.45 ± 0.03 μm, 0.53 ± 0.05 μm, and 0.59 ± 0.05 μm) during the approach of Viking Orbiter II in Martian summer (Ls = 105°) were mosaicked by...
Authors
L.A. Soderblom, K. Edwards, E. M. Eliason, E.M. Sanchez, M.P. Charette
Possible fossil H2O liquid-ice interfaces in the Martian crust Possible fossil H2O liquid-ice interfaces in the Martian crust
Throughout the northern equatorial region of Mars, extensive areas have been uniformly stripped, roughly to a constant depth. These terrains vary widely in their relative ages. A model is described here to explain this phenomenon as reflecting the vertical distribution of H2O liquid and ice in the crust. Under present conditions the Martian equatorial regions are stratified in terms of...
Authors
L.A. Soderblom, D. B. Wenner
Voyager imaging experiment Voyager imaging experiment
The overall objective of this experiment is exploratory reconnaissance of Jupiter, Saturn, their satellites, and Saturn's rings. Such reconnaissance, at resolutions and phase angles unobtainable from Earth, can be expected to provide much new data relevant to the atmospheric and/or surface properties of these bodies. The experiment also has the following specific objectives: Observe and
Authors
B.A. Smith, G.A. Briggs, G. E. Danielson, A.F. Cook, M. E. Davies, G.E. Hunt, H. Masursky, L.A. Soderblom, T.C. Owen, C. Sagan, V.E. Suomi