Zobrazeno 1 - 10
of 10
pro vyhledávání: '"R. J. Oliversen"'
Autor:
J. E. P. Connerney, S. Timmins, R. J. Oliversen, J. R. Espley, J. L. Joergensen, S. Kotsiaros, P. S. Joergensen, J. M. G. Merayo, M. Herceg, J. Bloxham, K. M. Moore, A. Mura, A. Moirano, S. J. Bolton, S. M. Levin
Publikováno v:
Connerney, J E P, Timmins, S, Oliversen, R J, Espley, J R, Joergensen, J L, Kotsiaros, S, Joergensen, P S, Merayo, J M G, Herceg, M, Bloxham, J, Moore, K M, Mura, A, Moirano, A, Bolton, S J & Levin, S M 2022, ' A New Model of Jupiter's Magnetic Field at the Completion of Juno's Prime Mission ', Journal of Geophysical Research: Planets, vol. 127, no. 2, e2021JE007055 . https://doi.org/10.1029/2021JE007055
A spherical harmonic model of the magnetic field of Jupiter is obtained from vector magnetic field observations acquired by the Juno spacecraft during 32 of its first 33 polar orbits. These Prime Mission orbits sample Jupiter's magnetic field nearly
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a76260a2a71c9dc8274659dfd03fa420
https://resolver.caltech.edu/CaltechAUTHORS:20211221-866880000
https://resolver.caltech.edu/CaltechAUTHORS:20211221-866880000
Publikováno v:
The Astrophysical Journal. 581:770-775
We present quantitative measurements of cometary [C I] 9850 A emission obtained during observations of comet Hale-Bopp (C/1995 O1) in 1997 March and April. The observations were carried out using a high-resolution (λ/Δλ ≈ 40,000) Fabry-Perot/CCD
Publikováno v:
Icarus. 111:45-64
In November and December 1988, we acquired 157 spectra of (S II) lambda 6731 emissions from the Io plasma torus with a Fabry-Perot interferometer at the McMath-Pierce Solar Telescope facility on Kitt Peak. A major goal of this experiment was to exten
Autor:
R. J. Oliversen, A. G. Michalitsianos
Publikováno v:
Astrophysical Applications of Gravitational Lensing ISBN: 9780792339557
Determining the nature of spectral variability in gravitationally-lensed BAL (broad absorption line) quasars is important for time-delay and microlensing studies because the delay-times can be comparable with the time scales of intrinsic QSO ionizati
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::3b68f6bea623c5f817430ebc45d5cc04
https://doi.org/10.1007/978-94-009-0221-3_68
https://doi.org/10.1007/978-94-009-0221-3_68
Publikováno v:
The Astrophysical Journal. 461:593
Autor:
A. G. Michelitsianos, R. J. Oliversen
Publikováno v:
The Astrophysical Journal. 439:599
The UV line profile structure of high-ionization resonance lines found with the International Ultraviolet Explorer (IUE) in the brightest of four multiply imaged sources (images-A) in the candidate gravitational lens UM 425 = QSO 1120+019 indicates b
Autor:
Fred L. Roesler, Roger V. Yelle, A. L. Broadfoot, K. Magee, Frank Scherb, R. J. Oliversen, John M. Harlander, Ronald J. Reynolds
Publikováno v:
Advances in Space Research. 5:279-282
High-spectral-resolution line profiles and images of comet Halley were obtained in 1986 at the National Solar Observatory McMath telescope, using a dual-etalon Fabry-Perot spectrometer. The spectrometer was designed to obtain data in four distinct mo
Autor:
Fred L. Roesler, Donald G. York, T. B. Williams, R. J. Oliversen, Edward B. Jenkins, Kurt P. Jaehnig, Frank Scherb
Publikováno v:
SPIE Proceedings.
A description is presented of the use of a CCD imaging spectrometer which has been employed at a 2.1 m telescope to obtain monochromatic images in the red and near infrared. The system studied was Jupiter's plasma torus which circles the planet with
Autor:
J. M. Hollis, F. Yusef-Zadeh, T. J. Cornwell, R. J. Oliversen, A. G. Michalitsianos, M. Kafatos
Publikováno v:
The Astrophysical Journal. 337:514
Subarcsecond observations of the RX Puppis symbiotic system with the VLA have resolved 2 cm continuum emission which deviates from a previously reported circularly symmetric radio distribution. The radio structure is comprised of at least three nearl
Autor:
Donald G. York, D. Long, T. B. Williams, Frank Scherb, J. M. Lattis, R. J. Oliversen, Fred L. Roesler, Paul Zucchino, Edward B. Jenkins, John L. Lowrance
Publikováno v:
The Astrophysical Journal. 259:900