Zobrazeno 1 - 10
of 3 650
pro vyhledávání: '"Wong, Michael A."'
Autor:
Harkett, Jake, Fletcher, Leigh N., King, Oliver R. T., Roman, Michael T., Melin, Henrik, Hammel, Heidi B., Hueso, Ricardo, Sánchez-Lavega, Agustín, Wong, Michael H., Milam, Stefanie N., Orton, Glenn S., de Kleer, Katherine, Irwin, Patrick G. J., de Pater, Imke, Fouchet, Thierry, Rodríguez-Ovalle, Pablo, Fry, Patrick M., Showalter, Mark R.
Publikováno v:
JGR:Planets, 129, e2024JE008415
Jupiter's Great Red Spot (GRS) was mapped by the James Webb Space Telescope (JWST)/Mid-Infrared Instrument (4.9-27.9 micron) in July and August 2022. These observations took place alongside a suite of visual and infrared observations from; Hubble, JW
Externí odkaz:
http://arxiv.org/abs/2410.02468
Autor:
Bockelée-Morvan, Dominique, Poch, Olivier, Leblanc, Françcois, Zakharov, Vladimir, Lellouch, Emmanuel, Quirico, Eric, de Pater, Imke, Fouchet, Thierry, Rodriguez-Ovalle, Pablo, Roth, Lorenz, Merlin, Frédéric, Duling, Stefan, Saur, Joachim, Masson, Adrien, Fry, Patrick, Trumbo, Samantha, Brown, Michael, Cartwright, Richard, Cazaux, Stéphanie, de Kleer, Katherine, Fletcher, Leigh N., Milby, Zachariah, Moingeon, Audrey, Mura, Alessandro, Orton, Glenn S., Schmitt, Bernard, Tosi, Federico, Wong, Michael H.
Publikováno v:
A&A 690, L11 (2024)
Jupiter's icy moon Ganymede has a tenuous exosphere produced by sputtering and possibly sublimation of water ice. To date, only atomic hydrogen and oxygen have been directly detected in this exosphere. Here, we present observations of Ganymede's CO$_
Externí odkaz:
http://arxiv.org/abs/2409.13364
Autor:
Rodríguez-Ovalle, Pablo, Fouchet, Thierry, Guerlet, Sandrine, Cavalié, Thibault, Hue, Vincent, López-Puertas, Manuel, Lellouch, Emmanuel, Sinclair, James A., de Pater, Imke, Fletcher, Leigh N., Wong, Michael H., Harkett, Jake, Orton, Glenn S., Hueso, Ricardo, Sánchez-Lavega, Agustín, Stallard, Tom S., Bockelee-Morvan, Dominique, King, Oliver, Roman, Michael T., Melin, Henrik
Jupiters south polar region was observed by JWST Mid Infrared Instrument in December 2022. We used the Medium Resolution Spectrometer mode to provide new information about Jupiters South Polar stratosphere. The southern auroral region was visible and
Externí odkaz:
http://arxiv.org/abs/2406.08133
Autor:
Li, Cheng, Allison, Michael, Atreya, Sushil, Brueshaber, Shawn, Fletcher, Leigh N., Guillot, Tristan, Li, Liming, Lunine, Jonathan, Miguel, Yamila, Orton, Glenn, Steffes, Paul, Waite, J. Hunter, Wong, Michael H., Levin, Steven, Bolton, Scott
The temperature structure of a giant planet was traditionally thought to be an adiabat assuming convective mixing homogenizes entropy. The only in-situ measurement made by the Galileo Probe detected a near-adiabatic temperature structure within one o
Externí odkaz:
http://arxiv.org/abs/2403.05363
Autor:
Schmider, François-Xavier, Gaulme, Patrick, Morales-Juberías, Raúl, Jackiewicz, Jason, Gonçalves, Ivan, Guillot, Tristan, Simon, Amy A., Wong, Michael H., Underwood, Thomas, Voelz, David, Sanchez, Cristo, DeColibus, Riley, Kovac, Sarah A., Sellers, Sean, Gilliam, Doug, Boumier, Patrick, Appourchaux, Thierry, Dejonghe, Julien, Rivet, Jean Pierre, Markham, Steve, Howard, Saburo, Abe, Lyu, Mekarnia, Djamel, Ikoma, Masahiro, Hanayama, Hidekazu, Sato, Bun'ei, Kunitomo, Masanobu, Izumiura, Hideyuki
Publikováno v:
Planet. Sci. J. 5 100 (2024)
We present three-dimensional (3D) maps of Jupiter's atmospheric circulation at cloud-top level from Doppler-imaging data obtained in the visible domain with JIVE, the second node of the JOVIAL network, which is mounted on the Dunn Solar Telescope at
Externí odkaz:
http://arxiv.org/abs/2312.16888
Autor:
Irwin, Patrick G. J., Dobinson, Jack, James, Arjuna, Wong, Michael H., Fletcher, Leigh N., Roman, Michael T., Teanby, Nicholas A., Toledo, Daniel, Orton, Glenn S., Perez-Hoyos, Santiago, Sanchez-Lavega, Agustin, Simon, Amy, Morales-Juberias, Raul, de Pater, Imke
Spectral observations of Neptune made in 2019 with the MUSE instrument at the Very Large Telescope in Chile have been analysed to determine the spatial variation of aerosol scattering properties and methane abundance in Neptune's atmosphere. The dark
Externí odkaz:
http://arxiv.org/abs/2310.13525
We investigated whether large language models (LLMs) can develop data validation tests. We considered 96 conditions each for both GPT-3.5 and GPT-4, examining different prompt scenarios, learning modes, temperature settings, and roles. The prompt sce
Externí odkaz:
http://arxiv.org/abs/2310.01402
Autor:
Chavez, Erandi, de Pater, Imke, Redwing, Erin, Molter, Edward M., Roman, Michael T., Zorzi, Andrea, Alvarez, Carlos, Campbell, Randy, de Kleer, Katherine, Hueso, Ricardo, Wong, Michael H., Lynam, Elinor Gates Paul David, Davies, Ashley G., Aycock, Joel, Mcilroy, Jason, Pelletier, John, Ridenour, Anthony, Stickel, Terry
Publikováno v:
Icarus Volume 404, 1 November 2023, 115667
Using archival near-infrared observations from the Keck and Lick Observatories and the Hubble Space Telescope, we document the evolution of Neptune's cloud activity from 1994 to 2022. We calculate the fraction of Neptune's disk that contained clouds,
Externí odkaz:
http://arxiv.org/abs/2307.08157
Autor:
Chavez, Erandi, Redwing, Erin, de Pater, Imke, Hueso, Ricardo, Molter, Edward M., Wong, Michael H., Alvarez, Carlos, Gates, Elinor, de Kleer, Katherine, Aycock, Joel, Mcilroy, Jason, Pelletier, John, Ridenour, Anthony, Sánchez-Lavega, Agustín, Rojas, Jose Félix, Stickel, Terry
Publikováno v:
Icarus Volume 401, 1 September 2023, Article 115604
Using near-infrared observations of Neptune from the Keck and Lick Observatories, and the Hubble Space Telescope in combination with amateur datasets, we calculated the drift rates of prominent infrared-bright cloud features on Neptune between 2018 a
Externí odkaz:
http://arxiv.org/abs/2307.06462
Autor:
Bhattacharya, Ananyo, Li, Cheng, Atreya, Sushil K., Steffes, Paul G., Levin, Steven M., Bolton, Scott J., Guillot, Tristan, Gupta, Pranika, Ingersoll, Andrew P., Lunine, Jonathan I., Orton, Glenn S., Oyafuso, Fabiano A., Waite, J. Hunter, Belloti, Amadeo, Wong, Michael H.
Water and ammonia vapors are known to be the major sources of spectral absorption at pressure levels observed by the microwave radiometer (MWR) on Juno. However, the brightness temperatures and limb darkening observed by the MWR at its longest wavele
Externí odkaz:
http://arxiv.org/abs/2306.12546