Zobrazeno 1 - 10
of 62
pro vyhledávání: '"K. D. Rosema"'
Autor:
David L. Mitchell, Steven J. Ostro, R. Scott Hudson, S. Denise Howard, D. Choate, Daniel J. Scheeres, R. Winkler, Jonathan D. Giorgini, Randy Rose, M. A. Slade, Donald K. Yeomans, Raymond F. Jurgens, K. D. Rosema
Publikováno v:
Icarus. 121:46-66
Goldstone radar observations of Geographos from August 28 through September 2, 1994 yield over 400 delay-Doppler images whose linear spatial resolutions range from approximately 75 - 151 m, and 138 pairs of dual-polarization (OC, SC) spectra with one
Autor:
Donald B. Campbell, Steven J. Ostro, John F. Chandler, Raymond F. Jurgens, Donald K. Yeomans, Lance A. M. Benner, R. Scott Hudson, K. D. Rosema, Irwin I. Shapiro
Publikováno v:
Icarus. 158:379-388
We report Doppler-only (cw) radar observations of basaltic near-Earth asteroid 3908 Nyx obtained at Arecibo and Goldstone in September and October of 1988. The circular polarization ratio of 0.75±0.03 exceeds ∼90% of those reported among radar-det
Publikováno v:
Icarus. 156:580-583
Arecibo radar echo spectra show the Q-class asteroid 1862 Apollo to have an elongation within 10% of 1.27, a pole-on silhouette with an average dimension of about 1.7 km, and disc-integrated radar properties that are typical for radar-detected near-E
Autor:
Daniel J. Scheeres, D. Choate, C. R. Franck, M. N. Meshkov, Jon D. Giorgini, Steven J. Ostro, D. Howard, D. Kelley, R. A. Cormier, R. Winkler, Alan W. Harris, Akiko M. Nakamura, Martin A. Slade, Alexander L. Zaitsev, Yusei Koyama, R. S. Hudson, R. Littlefair, P. W. Chodas, R. Frye, D. K. Yeomans, Lance A. M. Benner, Patrick Palmer, Randy Rose, David L. Mitchell, K. D. Rosema, Raymond F. Jurgens, Michael Thomas
Publikováno v:
Icarus. 148:37-51
We report 8510-MHz (3,5-cm) radar observations of the Earth crossing asteroid (ECA) 6489 Golevka (1991 JX) obtained between June 3 and June 15, 1995, at Goldstone, the Very Large Array and the Evpatoria (Ukraine) and Kashima (Japan) radio antennas.
Autor:
Lance A. M. Benner, Donald B. Campbell, Alan W. Harris, John F. Chandler, Irwin I. Shapiro, Michael K. Shepard, K. D. Rosema, Steven J. Ostro
Publikováno v:
Icarus. 147:520-529
We report Doppler-only (cw) radar observations of near-Earth Asteroid 2100 Ra-Shalom obtained at the Arecibo Observatory using a transmitter frequency of 2380 MHz (12.6 cm) on 1984 Aug. 18–22. Weighted and filtered sums of cw echoes achieve a maxim
Autor:
K. D. Rosema, Lance A. M. Benner, P.R. Mahapatra, Martin A. Slade, Donald K. Yeomans, Raymond F. Jurgens, Randy Rose, Jon D. Giorgini, Steven J. Ostro, R. Winkler
Publikováno v:
Planetary and Space Science. 47:987-995
We report Doppler-only radar observations of Icarus at Goldstone at a transmitter frequency of 8510 MHz (3.5 cm wavelength) during 8-10 June 1996, the first radar detection of the object since 1968. Optimally filtered and folded spectra achieve a max
Autor:
Donald K. Yeomans, John F. Chandler, David L. Mitchell, Jon D. Giorgini, Steven J. Ostro, Irwin I. Shapiro, Christopher Magri, K. D. Rosema, Donald B. Campbell, Michael Thomas
Publikováno v:
Icarus. 140:379-407
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 polarization ratio, we obtain new pole constraints fo
Autor:
K. D. Rosema, Martin A. Slade, Michael Thomas, David L. Mitchell, R. Scott Hudson, Raymond F. Jurgens, Lance A. M. Benner, Randy Rose, Donald K. Yeomans, Petr Pravec, Jon D. Giorgini, Steven J. Ostro, R. Winkler
Publikováno v:
Icarus. 139:309-327
We report Doppler-only (cw) and delay-Doppler radar observations of Bacchus obtained at Goldstone at a transmitter frequency of 8510 MHz (3.5 cm) on 1996 March 22, 24, and 29.
Autor:
R. A. Cormier, Randy Rose, Donald K. Yeomans, Ron Littlefair, R. Scott Hudson, Paul W. Chodas, Lance A. M. Benner, Raymond F. Jurgens, Jon D. Giorgini, Steven J. Ostro, R. Winkler, Michael Thomas, K. D. Rosema, Dan Kelley, D. Choate, Martin A. Slade
Publikováno v:
Icarus. 137:122-139
We report initial results of daily delay/Doppler observations of Toutatis with the Goldstone 8510-MHz (3.5-cm) radar during November 25 - December 3, 1996. Using the physical model of Toutatis derived form 1992 radar observations (Hudson and Ostro 19
Publikováno v:
Icarus. 131:4-14
We use new analysis techniques to constrain the shape of 433 Eros with Goldstone radar data obtained during the asteroid's close approach in 1975. A previous analysis of these data (Ostro, Rosema, and Jurgens, 1990, Icarus 84, 334–351) used estimat