Zobrazeno 1 - 10
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pro vyhledávání: '"Wong, M H"'
Autor:
Sánchez-Lavega, A., García-Melendo, E., Perez-Hoyos, S., Hueso, R., Wong, M. H., Simon, A., Sanz-Requena, J. F., Antuñano, A., Barrado-Izagirre, N., Garate-Lopez, I., Rojas, J. F., Gaztelurrutia, T. del Rio, Gómez-Forrellad, J. M., de Pater, I., Li, L., Barry, T., contributors, PVOL
Publikováno v:
Nature Communications, vol. 7, article number: 13626 (2016)
Saturn has an intense and broad eastward equatorial jet with a complex three-dimensional structure mixed with time variability. The equatorial region experiences strong seasonal insolation variations enhanced by ring shadowing and three of the six kn
Externí odkaz:
http://arxiv.org/abs/2401.17833
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:
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:
Hueso, R., Sánchez-Lavega, A., Rojas, J. F., Simon, A. A., Barry, T., del Río-Gaztelurrutia, T., Antuñano, A., Sayanagi, K. M., Delcroix, M., Fletcher, L. N., García-Melendo, E., Pérez-Hoyos, S., Blalock, J., Colas, F., Gómez-Forrellad, J. M., Gunnarson, J. L., Peach, D., Wong, M. H.
We examine Saturn's atmosphere with observations from ground-based telescopes and Hubble Space Telescope (HST). We present a detailed analysis of observations acquired during 2018. A system of polar storms that appeared in the planet in March 2018 an
Externí odkaz:
http://arxiv.org/abs/1909.13849
Publikováno v:
Icarus 2019, Volume 322, p. 168-191
We observed Jupiter four times over a full rotation (10 hrs) with the upgraded Karl G. Jansky Very Large Array (VLA) between December 2013 and December 2014. Preliminary results at 4-17 GHz were presented in de Pater et al. (2016); in the present pap
Externí odkaz:
http://arxiv.org/abs/1902.07294
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Autor:
Fletcher, L. N., Melin, H., Adriani, A., Simon, A. A., Sanchez-Lavega, A., Donnelly, P. T., Antunano, A., Orton, G. S., Hueso, R., Kraaikamp, E., Wong, M. H., Barnett, M., Moriconi, M. L., Altieri, F., Sindoni, G.
Publikováno v:
Astronomical Journal, 156:67 (13pp), 2018
We characterise the origin and evolution of a mesoscale wave pattern in Jupiter's North Equatorial Belt (NEB), detected for the first time at 5 $\mu$m using a 2016-17 campaign of `lucky imaging' from the VISIR instrument on the Very Large Telescope a
Externí odkaz:
http://arxiv.org/abs/1807.10484
Autor:
Hueso, R., de Pater, I., Simon, A., Sanchez-Lavega, A., Delcroix, M., Wong, M. H., Tollefson, J. W., Baranec, C., de Kleer, K., Luszcz-Cook, S. H., Orton, G. S., Hammel, H. B., Gomez-Forrellad, J. M., Ordonez-Etxeberria, I., Sromovsky, L., Fry, P., Colas, F., Rojas, J. F., Perez-Hoyos, S., Gorczynski, P., Guarro, J., Kivits, W., Miles, P., Millika, D., Nicholas, P., Sussenbach, J., Wesley, A., Sayanagi, K., Ammons, S. M., Gates, E. L., Gavel, D., Garcia, E. Victor, Law, N. M., Mendikoa, I., Riddle, R.
Publikováno v:
Hueso et al., Icarus 295, 89-109 (2017)
Since 2013, observations of Neptune with small telescopes have resulted in several detections of long-lived bright atmospheric features that have also been observed by large telescopes such as Keck II or Hubble. The combination of both types of image
Externí odkaz:
http://arxiv.org/abs/1709.08854
Autor:
Fletcher, L. N., Orton, G. S., Sinclair, J. A., Donnelly, P., Melin, H., Rogers, J. H., Greathouse, T. K., Kasaba, Y., Fujiyoshi, T., Sato, T. M., Fernandes, J., Irwin, P. G. J., Giles, R. S., Simon, A. A., Wong, M. H., Vedovato, M.
Publikováno v:
Geophys. Res. Lett., 44, 7140-7148 (2017)
The dark colors of Jupiter's North Equatorial Belt (NEB, $7-17^\circ$N) appeared to expand northward into the neighboring zone in 2015, consistent with a 3-5 year cycle of activity in the NEB. Inversions of thermal-IR imaging from the Very Large Tele
Externí odkaz:
http://arxiv.org/abs/1708.05179
Autor:
Fletcher, Leigh N., Orton, G. S., Rogers, J. H., Simon-Miller, A. A., de Pater, I., Wong, M. H., Mousis, O., Irwin, P. G. J., Jacquesson, M., Yanamandra-Fisher, P. A.
Publikováno v:
Icarus, Volume 213, Issue 2, June 2011, Pages 564-580
Mid-infrared 7-20 $\mu$m imaging of Jupiter demonstrates that the increased albedo of Jupiter's South Equatorial Belt (SEB) during the `fade' (whitening) event of 2009-2010 was correlated with changes to atmospheric temperature and aerosol opacity. T
Externí odkaz:
http://arxiv.org/abs/1701.00957