Zobrazeno 1 - 10
of 21
pro vyhledávání: '"H. Herbert Breneman"'
Autor:
Jason Perry, Cynthia B. Phillips, Elizabeth P. Turtle, Kenneth P. Klaasen, M. P. Milazzo, Tilmann Denk, Alfred S. McEwen, Damon P. Simonelli, Windy L. Jaeger, David A. Williams, H. Herbert Breneman, Jani Radebaugh, Laszlo P. Keszthelyi, Paul E. Geissler
Publikováno v:
Icarus. 169:3-28
We present the observations of Io acquired by the Solid State Imaging (SSI) experiment during the Galileo Millennium Mission (GMM) and the strategy we used to plan the exploration of Io. Despite Galileo's tight restrictions on data volume and downlin
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::479417c68232dc6a467ab365057eac81
https://doi.org/10.1016/j.icarus.2003.10.014
https://doi.org/10.1016/j.icarus.2003.10.014
Autor:
H. Herbert Breneman, M. P. Milazzo, Cynthia B. Phillips, Elizabeth P. Turtle, Alfred S. McEwen, Tilmann Denk, Damon P. Simonelli, Paul Geissler, Jani Radebaugh, Greg Levanas, David A. Williams, Laszlo P. Keszthelyi, Kenneth P. Klaasen
Publikováno v:
Journal of Geophysical Research: Planets. 106:33025-33052
The Solid-State Imaging (SSI) instrument provided the first high- and medium-resolution views of Io as the Galileo spacecraft closed in on the volcanic body in late 1999 and early 2000. While each volcanic center has many unique features, the majorit
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::dd9ca710509d93a7c4b9518bc79f2cc6
https://doi.org/10.1029/2000je001383
https://doi.org/10.1029/2000je001383
Autor:
Shawn M. Brooks, David Morrison, Kenneth P. Klaasen, Frank C. Chuang, Steve Kadel, Erik Asphaug, Cynthia B. Phillips, Kevinm K. Williams, James W. Head, Robert Sullivan, Paul M. Schenk, Robert T. Pappalardo, H. Herbert Breneman, David A. Senske, Clark R. Chapman, Ronald Greeley, Jeffrey M. Moore, Gerhard Neukum, John W. Moreau, Michael J. S. Belton, James E. Klemaszewski, B. Bierhaus, Geoffrey C. Collins, Elizabeth P. Turtle, Bernd Giese, K. Magee
Publikováno v:
Icarus. 151:93-111
During the Galileo Europa Mission (GEM), impact features on Europa were observed with improved resolution and coverage was compared with Voyager or the Galileo nominal mission. We surveyed all primary impact features >4 km in diameter seen on Europa
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0a5845d0965a6331298ee50d2b2bb791
https://doi.org/10.1006/icar.2000.6558
https://doi.org/10.1006/icar.2000.6558
Autor:
David A. Williams, Elizabeth P. Turtle, Robert T. Pappalardo, R. Lopes-Gautier, Cynthia B. Phillips, H. Herbert Breneman, Laszlo P. Keszthelyi, Peter C. Thomas, K. Magee, Gerald Schubert, P. Schuster, Jeffrey M. Moore, Michael J. S. Belton, Gregory V. Hoppa, Damon P. Simonelli, Windy L. Jaeger, Kenneth P. Klaasen, Paul Geissler, Sarah A. Fagents, James W. Head, Torrence V. Johnson, M. P. Milazzo, Alfred S. McEwen, Ronald Greeley, Jani Radebaugh, Ryan C. Sullivan
Publikováno v:
Science. 288:1193-1198
During late 1999/early 2000, the solid state imaging experiment on the Galileo spacecraft returned more than 100 high-resolution (5 to 500 meters per pixel) images of volcanically active Io. We observed an active lava lake, an active curtain of lava,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c31418e76bcd8dfa56cce379840f05c3
https://doi.org/10.1126/science.288.5469.1193
https://doi.org/10.1126/science.288.5469.1193
Autor:
Louise M. Prockter, Paul Helfenstein, Geoffrey C. Collins, K. K. Williams, Elizabeth P. Turtle, Jeffrey M. Moore, Clark R. Chapman, Tilmann Denk, Paul Geissler, David A. Senske, Alfred S. McEwen, M. J. S. Belton, Cynthia B. Phillips, Bernd Giese, Kenneth P. Klaasen, S. D. Kadel, K. Magee, Sarah A. Fagents, Robert Wagner, Ronald Greeley, James W. Head, Gregory V. Hoppa, Gerhard Neukum, William B. Moore, Richard Greenberg, R. J. Sullivan, Michael H. Carr, Robert T. Pappalardo, B. R. Tufts, H. Herbert Breneman, Gerald Schubert, James E. Klemaszewski
Publikováno v:
Journal of Geophysical Research: Planets. 104:24015-24055
It has been proposed that Jupiter's satellite Europa currently possesses a global subsurface ocean of liquid water. Galileo gravity data verify that the satellite is differentiated into an outer H2O layer about 100 km thick but cannot determine the c
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::f7de5038984d6b343ebdfe9e8b5fb014
https://doi.org/10.1029/1998je000628
https://doi.org/10.1029/1998je000628
Autor:
Todd J. Jones, Andrew P. Ingersoll, H. Herbert Breneman, Ashwin R. Vasavada, David A. Senske, James M. Kaufman, Kenneth P. Klaasen, E. DeJong, K. Magee, Maureen Bell, Peter J. Gierasch, Don Banfield, Glenn S. Orton, Michael J. S. Belton
Publikováno v:
Icarus. 135:265-275
During the first six orbits of the Galileo spacecraft's prime mission, the Solid State Imaging (SSI) system acquired multispectral image mosaics of Jupiter's Great Red Spot, an equatorial belt/zone boundary, a “5-μm hot spot” similar to the Gali
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::578ed843a7e976e88257705df9005555
https://doi.org/10.1006/icar.1998.5984
https://doi.org/10.1006/icar.1998.5984
Autor:
Paul Helfenstein, Roland Wagner, Louise M. Prockter, Robert T. Pappalardo, Ursula Wolf, Ronald Greeley, Bernd Giese, David A. Senske, Clark R. Chapman, Gerhard Neukum, Jeffrey M. Moore, Jürgen Oberst, James W. Head, Michael J. S. Belton, H. Herbert Breneman
Publikováno v:
Icarus. 135:317-344
During its first two encounters with Ganymede, the Galileo spacecraft obtained images of a 16,500 km 2 portion of Galileo Regio, a large expanse of dark terrain, at high resolution (76–86 m/pixel). Through mapping of the G1 and G2 target sites with
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::f68e353ba13d9d5895f7a1c1eadc9811
https://doi.org/10.1006/icar.1998.5981
https://doi.org/10.1006/icar.1998.5981
Autor:
Geoffrey C. Collins, Randolph L. Kirk, Jürgen Oberst, B. Randy Tufts, David A. Senske, Jeffrey M. Moore, H. Herbert Breneman, Alfred S. McEwen, Paul Helfenstein, Kenneth P. Klaasen, James W. Head, Robert T. Pappalardo, Ronald Greeley, Clark R. Chapman, Gerhard Neukum, Bernd Giese
Publikováno v:
Icarus. 135:276-302
High-resolution Galileo imaging has provided important insight into the origin and evolution of grooved terrain on Ganymede. The Uruk Sulcus target site was the first imaged at high resolution, and considerations of resolution, viewing geometry, low
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::27b86f79f1bb59443a807970ce63822e
https://doi.org/10.1006/icar.1998.5966
https://doi.org/10.1006/icar.1998.5966
Autor:
Alfred S. McEwen, H. Herbert Breneman, M. J. S. Belton, Paul Geissler, K. Magee, James M. Kaufman, Kenneth P. Klaasen, Michael H. Carr, Laszlo P. Keszthelyi, David A. Senske, Damon P. Simonelli, Torrence V. Johnson, Todd J. Jones, Gerald Schubert
Publikováno v:
Icarus. 135:181-219
Active volcanism on Io has been monitored during the nominal Galileo satellite tour from mid 1996 through late 1997. The Solid State Imaging (SSI) experiment was able to observe many manifestations of this active volcanism, including (1) changes in t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::fed7925d7aa3a8c980b5ad6e7686e045
https://doi.org/10.1006/icar.1998.5972
https://doi.org/10.1006/icar.1998.5972
Autor:
Clark R. Chapman, Joseph Veverka, Alfred S. McEwen, Pascal Lee, Damon P. Simonelli, R. V. Wagner, James W. Head, Kenneth P. Klaasen, Torrence V. Johnson, Peter C. Thomas, Scott L. Murchie, Stefano Mottola, G. Neukum, J. Granahan, Michael J. S. Belton, Merton E. Davies, M. Robinson, H. Herbert Breneman, F. P. Fanale, Harold Garbeil, Randolph L. Kirk, Carl B. Pilcher, Beth E. Clark, Paul Helfenstein
Publikováno v:
Icarus. 107:37-60
Galileo images of Gaspra make it possible for the first time to determine a main-belt asteroid's photometric properties accurately by providing surface-resolved coverage over a wide range of incidence and emission angles and by extending the phase an
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::89f03528eb50dabc7c47da8111d17018
https://doi.org/10.1006/icar.1994.1005
https://doi.org/10.1006/icar.1994.1005