Zobrazeno 1 - 10
of 203
pro vyhledávání: '"R W, Carlson"'
Publikováno v:
Geochemistry, Geophysics, Geosystems, Vol 21, Iss 8, Pp n/a-n/a (2020)
Abstract Continental flood basalts are more prone to compositional modification from passage through thicker and (or) more felsic crust in comparison to their oceanic counterparts. The Steens Basalt in southeast Oregon (~17 Ma) is among the oldest an
Externí odkaz:
https://doaj.org/article/f3beb98500c343a8a9921ff5504d501b
Autor:
B. E. Morgado, A. R. Gomes-Júnior, F. Braga-Ribas, R. Vieira-Martins, J. Desmars, V. Lainey, E. D’aversa, D. Dunham, J. Moore, K. Baillié, D. Herald, M. Assafin, B. Sicardy, S. Aoki, J. Bardecker, J. Barton, T. Blank, D. Bruns, N. Carlson, R. W. Carlson, K. Cobble, J. Dunham, D. Eisfeldt, M. Emilio, C. Jacques, T. C. Hinse, Y. Kim, M. Malacarne, P. D. Maley, A. Maury, E. Meza, F. Oliva, G. S. Orton, C. L. Pereira, M. Person, C. Plainaki, R. Sfair, G. Sindoni, M. Smith, E. Sussenbach, P. Stuart, J. Vrolijk, O. C. Winter
Publikováno v:
The Astronomical Journal
The Astronomical Journal, 2022, 163, ⟨10.3847/1538-3881/ac6108⟩
The Astronomical Journal, 2022, 163, ⟨10.3847/1538-3881/ac6108⟩
A stellar occultation occurs when a Solar System object passes in front of a star for an observer. This technique allows the determination of sizes and shapes of the occulting body with kilometer precision. Also, this technique constrains the occulti
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cb8f473e6267f2b981186ea231a020a6
http://arxiv.org/abs/2203.11711
http://arxiv.org/abs/2203.11711
Autor:
Mauro Ciarniello, Andrea Raponi, Emiliano D'Aversa, Gianrico Filacchione, R. W. Carlson, Giovanna Rinaldi, Fabrizio Capaccioni
Introduction The Visible channel of the Rosetta VIRTIS spectrometer is known to be affected by significant straylight, which makes it difficult to take advantage of its whole 230-1040 nm spectral range [1]. Straylight is by definition an extra signal
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::2a49aea6306f8da46101b1f7833e3860
https://doi.org/10.5194/epsc2021-231
https://doi.org/10.5194/epsc2021-231
Publikováno v:
Molecular Plant-Microbe Interactions, Vol 16, Iss 12, Pp 1085-1093 (2003)
The elucidation of the structure of the O-antigen of Rhizo-bium etli CE3 predicts that the R. etli CE3 genome must contain genes encoding acetyl- and methyltransferases to confer the corresponding modifications to the O-antigen. We identified three o
Externí odkaz:
https://doaj.org/article/cf9792ee39ed4321b8f349245ef3b267
Autor:
Kevin P. Hand, R. W. Carlson
Publikováno v:
IEEE Transactions on Nuclear Science. 62:2273-2282
There is great scientific interest of Jupiter’s moon Europa and in performing further spacecraft investigations. However, successful measurements at this satellite are difficult because transient charge pulses produced by Jupiter’s magnetospheric
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::19c2292dd81b4fe04f5b0e154880cb45
https://doi.org/10.1109/tns.2015.2460674
https://doi.org/10.1109/tns.2015.2460674
Autor:
David H. Grinspoon, Kevin H. Baines, Pierre Drossart, James B. Pollack, Fredric W. Taylor, Th. Encrenaz, R. W. Carlson, L. W. Kamp
Using Venus nightside data obtained by the Galileo Near-Infrared Mapping Spectrometer (NIMS), we have studied the correlation of 1.74 and 2.30 micrometer radiation which is transmitted through the clouds. Since the scattering and absorption propertie
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e719b3d85b04dc15536cd202b929cc10
https://doi.org/10.1016/0032-0633(93)90030-6
https://doi.org/10.1016/0032-0633(93)90030-6
Thin-film transmission spectra of ammonium hydrosulfide (NH4SH) ice and ammonia (NH3) ice between 1300 and 12,000 cm-1 were used to determine the ice's optical constants. The films were grown on a sapphire substrate, and a Fourier-transform spectrome
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2e77c8af1721e2afe71ecf545334c815
https://ora.ox.ac.uk/objects/uuid:bd8fc79c-e3be-49e7-8948-ee2fea79e2dd
https://ora.ox.ac.uk/objects/uuid:bd8fc79c-e3be-49e7-8948-ee2fea79e2dd
The Galileo Near Infrared Mapping Spectrometer (NIMS) has returned many spectra of the Jovian atmosphere in the range 0.7-5.2 mum. Although communications restrictions have limited the data return, several wide-area maps have been recorded at near fu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b5ccf5b08ca7a4b4f493b41bb216b338
https://ora.ox.ac.uk/objects/uuid:a181df80-bef9-492b-b663-e761e44ede72
https://ora.ox.ac.uk/objects/uuid:a181df80-bef9-492b-b663-e761e44ede72
Autor:
Th. Encrenaz, L. W. Kamp, S. B. Calcutt, Bruno Bézard, R. W. Carlson, A.D. Collard, Emmanuel Lellouch, Kevin H. Baines, Pierre Drossart, Fredric W. Taylor
A large number of i.r. spectra of Venus was obtained using the Near-Infrared Mapping Spectrometer (NIMS) on the Galileo spacecraft, during the February 1990 encounter. Preliminary results show an apparent increase in the tropospheric CO volume mixing
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2bea211a86118dd34052088f3c088fc2
https://doi.org/10.1016/0032-0633(93)90031-v
https://doi.org/10.1016/0032-0633(93)90031-v