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Caillon, N.; Jouzel, J.; Severinghaus, J.P.; Chappellaz, J.; Blunier, T. (2003). A novel method to study the phase relationship between Antarctic and Greenland climate. Geophysical research letters, 30.
Keywords: 3344 Meteorology and Atmospheric Dynamics: Paleoclimatology; 4267 Oceanography: General: Paleoceanography; 1827 Hydrology: Glaciology; 4870 Oceanography: Biological and Chemical: Stable isotopes; 1620 Global Change: Climate dynamics
Programme: 902
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Florenchie P., Le Provost C., Blayo E. & Verron J. (1995). A numerical model of the South Atlantic Ocean with assimilation of Topex-Poseidon data: predictions of the ACC frontal structures. (Vol. 115).
Abstract: IOC Workshop Report on 'Sea Level variability and Southern Ocean Dynamics'
Programme: 688
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Parish T.R., Pettre P. & Wendler G. (1993). A numerical study of the diurnal variation of the Adelie Land katabatic wind regime. J. Geophys. Res., 98(d7), 12933–12947.
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. (2022). A pair of sub-Neptunes transiting the bright K-dwarf TOI-1064 characterized with CHEOPS (Vol. 511).
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. (2023). A peat core Hg stable isotope reconstruction of Holocene atmospheric Hg deposition at Amsterdam Island (37.8oS) (Vol. 341).
Keywords: Hg deposition Hg stable isotopes Peat Rain Southern Hemisphere
Programme: 1028
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Marx J.C., Blaise V., Collins T., D'Amico S., Delille D., Gratia E., Hoyoux A., Huston A.ML., Sonan G., Feller G. & Gerday C. (2004). A perspective on cold enzymes: current knowledge and frequently asked questions. Cellular and molecular biology, 50, 643–655.
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. (2000). Antarct. Sci., 12(1), 52–63.
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. (2022). A Possible Alignment Between the Orbits of Planetary Systems and their Visual Binary Companions (Vol. 163).
Abstract: Astronomers do not have a complete picture of the effects of wide-binary companions (semimajor axes greater than 100 au) on the formation and evolution of exoplanets. We investigate these effects using new data from Gaia Early Data Release 3 and the Transiting Exoplanet Survey Satellite mission to characterize wide-binary systems with transiting exoplanets. We identify a sample of 67 systems of transiting exoplanet candidates (with well-determined, edge-on orbital inclinations) that reside in wide visual binary systems. We derive limits on orbital parameters for the wide-binary systems and measure the minimum difference in orbital inclination between the binary and planet orbits. We determine that there is statistically significant difference in the inclination distribution of wide-binary systems with transiting planets compared to a control sample, with the probability that the two distributions are the same being 0.0037. This implies that there is an overabundance of planets in binary systems whose orbits are aligned with those of the binary. The overabundance of aligned systems appears to primarily have semimajor axes less than 700 au. We investigate some effects that could cause the alignment and conclude that a torque caused by a misaligned binary companion on the protoplanetary disk is the most promising explanation.
Programme: 1066
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. (2011). A possible teleconnection between East Antarctic sea ice and ENSO during the Holocene..
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Thiebot JB, Arnould J, Gómez-Laich A, Ito K, Kato A, Mattern T, Mitamura H, Noda T, Poupart T, Quintana F, Raclot T, Ropert-Coudert Y, Sala JE, Sutton G, Yoda K, Takahashi . (2016). A Predator-borne videos emphasize the ecosystem role of jellyfish across southern oceans.
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