Search Publications

The CHEOPS view of the climate of WASP-3 b
DOI: 10.1051/0004-6361/202451049 Bibcode: 2024A&A...692A.129S

Alonso, R.; Deleuil, M.; Erikson, A. +83 more

Context. Hot Jupiters are giant planets subject to intense stellar radiation. The physical and chemical properties of their atmosphere make them the most amenable targets for atmospheric characterization. Aims. In this paper we analyze the photometry collected during the secondary eclipses of the hot Jupiter WASP-3 b by CHEOPS, TESS, and Spitzer. …

2024 Astronomy and Astrophysics
CHEOPS 0
Internal Structure of the Magnetic Funnel in the Polar Heliosphere
DOI: 10.1134/S003809462460104X Bibcode: 2024SoSyR..58S.105K

Kislov, R. A.

According to data obtained by the Ulysses spacecraft in 2017, high-latitude current sheets have been discovered in the polar heliosphere. They have been observed during solar activity minima in 1994 and 2007 at a distance of 2–3 AU above the south pole of the Sun. The discovered current sheets formed a conical surface rotating as a whole around th…

2024 Solar System Research
Ulysses 0
Interaction between a Coronal Mass Ejection and Comet 67P/Churyumov–Gerasimenko
DOI: 10.3847/1538-4357/ad3c42 Bibcode: 2024ApJ...967...43H

Gombosi, Tamas I.; Combi, Michael R.; Altwegg, Kathrin +6 more

The interaction between a coronal mass ejection (CME) and a comet has been observed several times by in situ observations from the Rosetta Plasma Consortium, which is designed to investigate the cometary magnetosphere of comet 67P/Churyumov–Gerasimenko (CG). Goetz et al. reported a magnetic field of up to 300 nT measured in the inner coma, which i…

2024 The Astrophysical Journal
Rosetta 0
Repeated and Long-Lasting Fault Activation on Amazonian Mars as Demonstrated by Tectonically Induced Landslides
DOI: 10.1029/2023GL107757 Bibcode: 2024GeoRL..5107757W

Fawdon, P.; Balme, M. R.; Rothery, D. A. +1 more

We identify and analyze a large shortening structure (surface expression of a thrust fault) in western Arabia Terra, Mars, exhibiting recent, repeated, and long-lasting tectonic activity. Where the fault system deforms Marsabit crater rim, four landslides with differing degradation states extend onto the crater floor. We propose these were trigger…

2024 Geophysical Research Letters
ExoMars-16 0
JCMT 850 µm Continuum Observations of Density Structures in the G35 Molecular Complex
DOI: 10.3847/1538-4357/ad6a5f Bibcode: 2024ApJ...974..239S

Tsai, Chao-Wei; Sanhueza, Patricio; Tej, Anandmayee +32 more

Filaments are believed to play a key role in high-mass star formation. We present a systematic study of the filaments and their hosting clumps in the G35 molecular complex using James Clerk Maxwell Telescope SCUBA-2 850 µm continuum data. We identified five clouds in the complex and 91 filaments within them, some of which form 10 hub–filamen…

2024 The Astrophysical Journal
Herschel 0
Mapping "Brain Terrain" Regions on Mars Using Deep Learning
DOI: 10.3847/PSJ/ad5673 Bibcode: 2024PSJ.....5..167P

Zhao, Daniel; Noe, Eldar; Morgan, Alexander M. +2 more

One of the main objectives of the Mars Exploration Program is to search for evidence of past or current life on the planet. To achieve this, Mars exploration has been focusing on regions that may have liquid or frozen water. A set of critical areas may have seen cycles of ice thawing in the relatively recent past in response to periodic changes in…

2024 The Planetary Science Journal
MEx 0
Martian paleolake outlet canyons - Evidence for controls on valley network formation
DOI: 10.1016/j.icarus.2023.115835 Bibcode: 2024Icar..40815835D

Sefton-Nash, Elliot; Miguel, Yamila; Diamant, Sharon J. M. +1 more

Martian valley networks (VNs) have been viewed as one of the most compelling pieces of evidence for ancient fluvial activity during the Late Noachian and Early Hesperian periods (3.7-3.5 Ga), likely as a result of precipitation (snowfall/rainfall). During this period, paleolakes also formed, predominantly due to water accumulation within impact cr…

2024 Icarus
MEx 0
Investigation of X-band and Ka-band amplitude scintillation based on measurement data collected during ESA's BepiColombo superior solar conjunction campaign
DOI: 10.1007/s12567-023-00491-2 Bibcode: 2024CEAS...16...87C

Chen, Shun-Ping; Lanucara, Marco; Villalvilla, Jose

Solar phase scintillation and solar amplitude scintillation are fundamentally important in deep space mission operations for designing a communication system capable of transmitting signals when the signal path is close to the Sun. The ESA's BepiColombo measurement data were analyzed in a previous paper in terms of the power spectral density of th…

2024 CEAS Space Journal
BepiColombo 0
Characterizing High-Energy Solar Proton Events with Energies Below and Above 100 MeV
DOI: 10.1007/s11207-024-02378-9 Bibcode: 2024SoPh..299..133A

Vainio, Rami; Valtonen, Eino; Al-Sawad, Amjad +1 more

We analyzed 58 high-energy proton events that occurred during the years 1996 – 2022. In 32 out of the 58 (55%) events, the proton energies extended up to 68 MeV but did not reach 100 MeV. In the remaining 26 events, the proton energies exceeded 100 M…

2024 Solar Physics
SOHO 0
FAST Observations of Four Comets to Search for the Molecular Line Emissions between 1.0 and 1.5 GHz Frequencies
DOI: 10.1088/1674-4527/ad7823 Bibcode: 2024RAA....24j5008C

Tsai, Chao-Wei; Duan, Yan; Li, Di +11 more

We used the Five-hundred-meter Aperture Spherical radio Telescope (FAST) to search for the molecular emissions in the L-band between 1.0 and 1.5 GHz toward four comets, C/2020 F3 (NEOWISE), C/2020 R4 (ATLAS), C/2021 A1 (Leonard), and 67P/Churyumov-Gerasimenko during or after their perihelion passages. Thousands of molecular transition lines fall i…

2024 Research in Astronomy and Astrophysics
Rosetta 0