From the 5 of 255 papers with an AI index.
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- The University of TokyoJP63 papers
- Kyoto UniversityJP44 papers
- Nagoya UniversityJP22 papers
- Centre National de la Recherche ScientifiqueFR19 papers
- Tokyo University of ScienceJP18 papers
- Czech Academy of Sciences, Astronomical InstituteCZ17 papers
- The University of OsakaJP17 papers
- Institute of Science Tokyo16 papers
- National Astronomical Observatory of JapanJP16 papers
- The Graduate University for Advanced Studies, SOKENDAIJP16 papers
- University of GenevaCH15 papers
- High Energy Accelerator Research OrganizationJP14 papers
5 papers · 1 filter
Oxygen isotope fractionation in the Martian atmosphere induced by CO photolysis and O formation
Tatsuya Yoshida, Shohei Aoki, Hiromu Nakagawa +8
The paper presents a 1D photochemical model of the Martian atmosphere that quantifies oxygen isotope fractionation caused by CO₂ photolysis and ozone formation, matching observed i…
Interpreting ALMA Multiwavelength Continuum Observations of PDS 70 c: An Optically Thick Dust Ring in the Circumplanetary Disk
Yuhito Shibaike, Satoshi Okuzumi, Takahiro Ueda +2
Giant planets form small gas disks, called circumplanetary disks (CPDs), during gas accretion. The CPD of PDS 70 c has been detected by the Atacama Large Millimeter/submillimeter A…
exoALMA XXI: The Morphology and Dynamics of Vertical Flows
Myriam Benisty, Andres F. Izquierdo, Jochen Stadler +33
Vertical gas flows, such as winds and meridional circulations, are natural outcomes of protoplanetary disk processes and play a critical role in the earliest stages of planet forma…
Characteristics of natural remanence records in fine-grained particles returned from asteroid Ryugu
Masahiko Sato, Yuki Kimura, Tadahiro Hatakeyama +25
Particles collected from the asteroid Ryugu by the Hayabusa2 spacecraft offer a unique opportunity to investigate the magnetic record of the primitive solar system, as any terrestr…
Comparison of General Circulation Models of the Venus upper atmosphere
Antoine Martinez, Hiroki Karyu, Amanda Brecht +7
In the context of future Venusian missions, it is crucial to improve our understanding of Venus upper atmosphere through 3D modeling, notably for spacecraft orbit computation. This…