Zobrazeno 1 - 10
of 14
pro vyhledávání: '"R G, French"'
Autor:
A. W. Shaw, D. L. Kaplan, P. Gandhi, T. J. Maccarone, E. S. Borowski, C. T. Britt, D. A. H. Buckley, K. B. Burdge, P. A. Charles, V. S. Dhillon, R. G. French, C. O. Heinke, R. I. Hynes, C. Knigge, S. P. Littlefair, Devraj Pawar, R. M. Plotkin, M. E. Ressler, P. Santos-Sanz, T. Shahbaz, G. R. Sivakoff, A. L. Stevens
Publikováno v:
The Astronomical Journal, Vol 169, Iss 1, p 21 (2024)
JWST, despite not being designed to observe astrophysical phenomena that vary on rapid timescales, can be an unparalleled tool for such studies. If timing systematics can be controlled, JWST will be able to open up the subsecond infrared timescale re
Externí odkaz:
https://doaj.org/article/f8dde5a8ec1b4aca9ca4d9b7e1e00493
INTRODUCTION Although Saturn's broad A, B, and C rings epitomize the concept of “planetary rings” in the minds of most people, much of our detailed knowledge of ring dynamics has come from the investigation of smaller-scale features such as densi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::150b644ea80a73f965627f2d4b24d0e5
https://doi.org/10.1017/9781316286791.011
https://doi.org/10.1017/9781316286791.011
Autor:
A. J. Kliore, J. D. Anderson, J. W. Armstrong, S. W. Asmar, C. L. Hamilton, N. J. Rappaport, H. D. Wahlquist, R. Ambrosini, F. M. Flasar, R. G. French, L. Iess, E. A. Marouf, A. F. Nagy
Publikováno v:
The Cassini-Huygens Mission ISBN: 1402031475
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::3b32f9201d8737cb3f787c209aab24e9
https://doi.org/10.1007/1-4020-3874-7_1
https://doi.org/10.1007/1-4020-3874-7_1
Publikováno v:
Science. 231:480-483
The γ and δ rings have by far the largest radial perturbations of any of the nine known Uranian rings. These two rings deviate from Keplerian orbits, having typical root-mean-square residuals of about 3 kilometers (compared to a few hundred meters
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8afd26dda045deb560d25dc06f79b8e9
https://doi.org/10.1126/science.231.4737.480
https://doi.org/10.1126/science.231.4737.480
Autor:
James B. Pollack, R. Tucker, Elliott C. Levinthal, B. Eross, R. G. French, Joseph Veverka, L. Quam, Russell Dubisch, Peter J. Gierasch, Joshua Lederberg, Carl Sagan, Paul J. Fox
Publikováno v:
Journal of Geophysical Research. 78:4163-4196
Systematic Mariner 9 monitoring of the space and time distribution of Martian bright and dark markings, the streaks and splotches, indicates a range of global correlations. The time-variable classical dark markings owe their configurations and variab
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::20822a431661100359a16224138ace45
https://doi.org/10.1029/jb078i020p04163
https://doi.org/10.1029/jb078i020p04163
Publikováno v:
Nature. 298:827-829
It is theoretically shown that at least seven of the nine rings of Uranus have orbits inclined to the equatorial plane of the planet. To the existing model of the Uranian rings, free parameters for the inclination of the rings and for the angle betwe
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::0a4f9bcdece25550287a9a47d3f7cdba
https://doi.org/10.1038/298827a0
https://doi.org/10.1038/298827a0
Publikováno v:
Science (New York, N.Y.). 231(4737)
The gamma and delta rings have by far the largest radial perturbations of any of the nine known Uranian rings. These two rings deviate from Keplerian orbits, having typical root-mean-square residuals of about 3 kilometers (compared to a few hundred m
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=pmid________::2fe8e8f53e050a1092cb8a4108d10701
https://pubmed.ncbi.nlm.nih.gov/17776019
https://pubmed.ncbi.nlm.nih.gov/17776019
Publikováno v:
Astronomical Journal; Jan2019, Vol. 157 Issue 1, p1-1, 1p
Autor:
C. Church, J. Veverka, Peter J. Gierasch, J. L. Elliot, Carl Sagan, E. W. Dunham, R. G. French
Publikováno v:
Science. 195:485-486
Epsilon Geminorum occultation data obtained on April 8, 1976, with the aid of a 91-cm telescope aboard the NASA Kuiper Airborne Observatory have provided a basis for the determination of temperature, pressure, and number density profiles of the Marti
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e69e556cbbdb92112f5e6974478c385f
https://doi.org/10.1126/science.195.4277.485
https://doi.org/10.1126/science.195.4277.485