Zobrazeno 1 - 10
of 755
pro vyhledávání: '"de Pater, I"'
Autor:
Roth, L., Blöcker, A., de Kleer, K., Goldstein, D., Lellouch, E., Saur, J., Schmidt, C., Strobel, D. F., Tao, C., Tsuchiya, F., Dols, V., Huybrighs, H., Mura, A., Szalay, J. R., Badman, S. V., de Pater, I., Dott, A. -C., Kagitani, M., Klaiber, L., Koga, R., McEwen, A., Milby, Z., Retherford, K. D., Schlegel, S., Thomas, N., Tseng, W. L., Vorburger, A.
Since the Voyager mission flybys in 1979, we have known the moon Io to be extremely volcanically active as well as to be the main source of plasma in the vast magnetosphere of Jupiter. Material lost from Io forms neutral clouds, the Io plasma torus a
Externí odkaz:
http://arxiv.org/abs/2403.13970
Autor:
Hedman, M. M., Tiscareno, M. S., Showalter, M. R., Fletcher, L. N., King, O. R. T., Harkett, J., Roman, M. T., Rowe-Gurney, N., Hammel, H. B., Milam, S. N., Moutamid, M. El, Cartwright, R. J., de Pater, I., Molter, E.
JWST measured the infrared spectra of Saturn's rings and several of its small moons (Epimetheus, Pandora, Telesto and Pallene) as part of Guaranteed Time Observation program 1247. The NIRSpec instrument obtained near-infrared spectra of the small moo
Externí odkaz:
http://arxiv.org/abs/2402.15698
Subsurface Thermophysical Properties of Europa's Leading and Trailing Hemispheres as Revealed by ALM
We present best-fit values of porosity -- and the corresponding effective thermal inertiae -- determined from three different depths in Europa's near-subsurface (~1-20 cm). The porosity of the upper ~20 cm of Europa's subsurface varies between 75-50%
Externí odkaz:
http://arxiv.org/abs/2402.01952
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
Publikováno v:
Planetary Science Journal, 4 104 (2023)
The zeta ring is the innermost component of the Uranian ring system. It is of scientific interest because its morphology changed significantly between the Voyager 2 encounter in 1986 and subsequent Earth-based observations around 2007. It is also of
Externí odkaz:
http://arxiv.org/abs/2305.07190
Autor:
Cordiner, M. A., Villanueva, G. L., Wiesemeyer, H., Milam, S. N., de Pater, I., Moullet, A., Aladro, R., Nixon, C. A., Thelen, A. E., Charnley, S. B., Stutzki, J., Kofman, V., Faggi, S., Liuzzi, G., Cosentino, R., McGuire, B. A.
The presence of phosphine (PH$_3$) in the atmosphere of Venus was reported by Greaves et al. (2021a), based on observations of the J=1-0 transition at 267 GHz using ground-based, millimeter-wave spectroscopy. This unexpected discovery presents a chal
Externí odkaz:
http://arxiv.org/abs/2210.13519
Autor:
Brooks, Shawn M., Becker, Tracy M., Baillié, K., Becker, H. N., Bradley, E. T., Colwell, J. E., Cuzzi, J. N., de Pater, I., Eckert, S., Moutamid, M. El, Edgington, S. G., Estrada, P. R., Evans, M. W., Flandes, A., French, R. G., García, Á., Gordon, M. K., Hedman, M. M., Hsu, H. -W., Jerousek, R. G., Marouf, E. A., Meinke, B. K., Nicholson, P. D., Pilorz, S. H., Showalter, M. R., Spilker, L. J., Throop, H. B., Tiscareno, M. S.
We now know that the outer solar system is host to at least six diverse planetary ring systems, each of which is a scientifically compelling target with the potential to inform us about the evolution, history and even the internal structure of the bo
Externí odkaz:
http://arxiv.org/abs/2008.12418
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
Autor:
Price, D. C., Foster, G., Geyer, M., van Straten, W., Gajjar, V., Hellbourg, G., Karastergiou, A., Keane, E. F., Siemion, A. P. V., Arcavi, I., Bhat, R., Caleb, M., Chang, S-W., Croft, S., DeBoer, D., de Pater, I., Drew, J., Enriquez, J. E., Farah, W., Gizani, N., Green, J. A., Isaacson, H., Hickish, J., Jameson, A., Lebofsky, M., MacMahon, D. H. E., Möller, A., Onken, C. A., Petroff, E., Werthimer, D., Wolf, C., Worden, S. P., Zhang, Y. G.
Here, we report on the detection and verification of Fast Radio Burst FRB 180301, which occurred on UTC 2018 March 1 during the Breakthrough Listen observations with the Parkes telescope. Full-polarization voltage data of the detection were captured-
Externí odkaz:
http://arxiv.org/abs/1901.07412