Zobrazeno 1 - 10
of 525
pro vyhledávání: '"Orton G"'
Autor:
Bockelee-Morvan, D., Lellouch, E., Poch, O., Quirico, E., Cazaux, S., de Pater, I., Fouchet, T., Fry, P. M., Rodriguez-Ovalle, P., Tosi, F., Wong, M. H., Boshuizen, I., de Kleer, K., Fletcher, L. N., Meunier, L., Mura, A., Roth, L., Saur, J., Schmitt, B., Trumbo, S. K., Brown, M. E., O'Donoghue, J., Orton, G. S., Showalter, M. R.
Publikováno v:
A&A 681, A27 (2024)
JWST NIRSpec IFU (2.9-5.3 mu) and MIRI MRS (4.9-28.5 mu) observations were performed on both the leading and trailing hemispheres of Ganymede with a spectral resolution of ~2700. Reflectance spectra show signatures of water ice, CO2 and H2O2. An abso
Externí odkaz:
http://arxiv.org/abs/2310.13982
Autor:
Morgado, B. E., Gomes-Júnior, A. R., Braga-Ribas, F., Vieira-Martins, R., Desmars, J., Lainey, V., D'aversa, E., Dunham, D., Moore, J., Baillié, K., Herald, D., Assafin, M., Sicardy, B., Aoki, S., Bardecker, J., Barton, J., Blank, T., Bruns, D., Carlson, N., Carlson, R. W., Cobble, K., Dunham, J., Eisfeldt, D., Emilio, M., Jacques, C., Hinse, T. C., Kim, Y., Malacarne, M., Maley, P. D., Maury, A., Meza, E., Oliva, F., Orton, G. S., Pereira, C. L., Person, M., Plainaki, C., Sfair, R., Sindoni, G., Smith, M., Sussenbach, E., Stuart, P., Vrolijk, J., Winter, O. C.
Publikováno v:
The Astronomical Journal, Volume 163, Number 5, 2022
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:
http://arxiv.org/abs/2203.11711
Autor:
Fletcher, L. N., Oyafuso, F. A., Allison, M., Ingersoll, A., Li, L., Kaspi, Y., Galanti, E., Wong, M. H., Orton, G. S., Duer, K., Zhang, Z., Li, C., Guillot, T., Levin, S. M., Bolton, S.
Publikováno v:
Journal of Geophysical Research: Planets, 126, e2021JE006858
Juno Microwave Radiometer (MWR) observations of Jupiter's mid-latitudes reveal a strong correlation between brightness temperature contrasts and zonal winds, confirming that the banded structure extends throughout the troposphere. However, the microw
Externí odkaz:
http://arxiv.org/abs/2110.14620
Autor:
Galanti, E., Kaspi, Y., Duer, K., Fletcher, L., Ingersoll, A. P., Li, C., Orton, G. S., Guillot, T., Levin, S. M., Bolton, S. J.
Publikováno v:
Geophysical Research Letters, 2021
The observed zonal winds at Jupiter's cloud tops have been shown to be closely linked to the asymmetric part of the planet's measured gravity field. However, other measurements suggest that in some latitudinal regions the flow below the clouds might
Externí odkaz:
http://arxiv.org/abs/2102.10595
Autor:
Irwin, P. G. J., Dobinson, J., James, A., Toledo, D., Teanby, N. A., Fletcher, L. N., Orton, G. S., Pérez-Hoyos, S.
We present a reanalysis of visible/near-infrared (480-930 nm) observations of Neptune, made in 2018 with the MUSE instrument at the Very Large Telescope (VLT) in Narrow Field Adaptive Optics mode, reported by Irwin et al., Icarus, 311, 2019. We find
Externí odkaz:
http://arxiv.org/abs/2101.01063
Autor:
Fletcher, L. N., Orton, G. S., Greathouse, T. K., Rogers, J. H., Zhang, Z., Oyafuso, F. A., Eichstädt, G., Melin, H., Li, C., Levin, S. M., Bolton, S., Janssen, M., Mettig, H-J., Grassi, D., Mura, A., Adriani, A.
We present multi-wavelength measurements of the thermal, chemical, and cloud contrasts associated with the visibly dark formations (also known as 5-$\mu$m hot spots) and intervening bright plumes on the boundary between Jupiter's Equatorial Zone (EZ)
Externí odkaz:
http://arxiv.org/abs/2004.00072
Autor:
Iñurrigarro, P., Hueso, R., Legarreta, J., Sánchez-Lavega, A., Eichstädt, G., Rogers, J. H., Orton, G. S., Hansen, C. J., Pérez-Hoyos, S., Rojas, J. F., Gómez-Forrellad, J. M.
Moist convective storms in Jupiter develop frequently and can trigger atmospheric activity of different scales, from localized storms to planetary-scale disturbances including convective activity confined inside a larger meteorological system. In Feb
Externí odkaz:
http://arxiv.org/abs/1911.04437
Autor:
Cavalié, T., Hue, V., Hartogh, P., Moreno, R., Lellouch, E., Feuchtgruber, H., Jarchow, C., Cassidy, T., Fletcher, L. N., Billebaud, F., Dobrijevic, M., Rezac, L., Orton, G. S., Rengel, M., Fouchet, T., Guerlet, S.
Publikováno v:
A&A 630, A87 (2019)
Context. The origin of water in the stratospheres of Giant Planets has been an outstanding question ever since its first detection by ISO some 20 years ago. Water can originate from interplanetary dust particles, icy rings and satellites and large co
Externí odkaz:
http://arxiv.org/abs/1908.07399
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Akademický článek
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