Zobrazeno 1 - 10
of 86
pro vyhledávání: '"Attilio Rivoldini"'
Autor:
Mélanie Drilleau, Henri Samuel, Raphaël F. Garcia, Attilio Rivoldini, Clément Perrin, Mark Wieczorek, Philippe Lognonné, William B. Banerdt
Publikováno v:
Geophysical Research Letters, Vol 51, Iss 4, Pp n/a-n/a (2024)
Abstract Using body wave arrival times from 31 seismic events recorded on Mars by the InSight mission, combined with topography and gravity field modeling, we constrained lateral variations of crustal thickness through a Bayesian inversion approach.
Externí odkaz:
https://doaj.org/article/cb888cd622eb4c988d132c40f2fe31de
Autor:
Chi Yan, Ankit Barik, Sabine Stanley, Jason S.-Y. Leung, Anna Mittelholz, Catherine L. Johnson, Ana-Catalina Plesa, Attilio Rivoldini
Publikováno v:
The Planetary Science Journal, Vol 4, Iss 1, p 11 (2023)
Magnetic field observations from the MGS, MAVEN, and InSight missions reveal that a dynamo was active in Mars’s early history. One unique feature of Mars’s magnetic crustal field is its hemispheric dichotomy, where magnetic fields in the southern
Externí odkaz:
https://doaj.org/article/f4762010f0fb412aa9e0512b60f7e7e3
Autor:
Mélanie Drilleau, Éric Beucler, Philippe Lognonné, Mark P. Panning, Brigitte Knapmeyer‐Endrun, W. Bruce Banerdt, Caroline Beghein, Savas Ceylan, Martin vanDriel, Rakshit Joshi, Taichi Kawamura, Amir Khan, Sabrina Menina, Attilio Rivoldini, Henri Samuel, Simon Stähler, Haotian Xu, Mickaël Bonnin, John Clinton, Domenico Giardini, Balthasar Kenda, Vedran Lekic, Antoine Mocquet, Naomi Murdoch, Martin Schimmel, Suzanne E. Smrekar, Éléonore Stutzmann, Benoit Tauzin, Saikiran Tharimena
Publikováno v:
Earth and Space Science, Vol 7, Iss 12, Pp n/a-n/a (2020)
Abstract SEIS, the seismometer of the InSight mission, which landed on Mars on 26 November 2018, is monitoring the seismic activity of the planet. The goal of the Mars Structure Service (MSS) is to provide, as a mission product, the first average 1
Externí odkaz:
https://doaj.org/article/44c55f60f73149c3be76f9a1f5b97d80
Publikováno v:
Geodesy and Geodynamics, Vol 8, Iss 6, Pp 427-432 (2017)
The global Very Long Baseline Interferometry observation for measuring the Earth rotation's parameters was launched around 1970s. Since then the precision of the measurements is continuously improving by taking into account various instrumental and e
Externí odkaz:
https://doaj.org/article/ab09e2913dbe4b5d84bbcd7228727afa
Autor:
Véronique Dehant, Raphael Laguerre, Jérémy Rekier, Attilio Rivoldini, Santiago Andres Triana, Antony Trinh, Tim Van Hoolst, Ping Zhu
Publikováno v:
Geodesy and Geodynamics, Vol 8, Iss 6, Pp 389-395 (2017)
In this review paper, we examine the changes in the Earth orientation in space and focus on the nutation (shorter-term periodic variations), which is superimposed on precession (long-term trend on a timescale of years). We review the nutation modelli
Externí odkaz:
https://doaj.org/article/2d0da575eae44e9aad5f4ba02466f4a5
Publikováno v:
Advances in Physics: X, Vol 4, Iss 1 (2019)
More than 1000 exoplanets with a radius smaller than twice that of the Earth are currently known, mainly thanks to space missions dedicated to the search of exoplanets. Mass and radius estimates, which are only available for a fraction ($$ \sim $$ 10
Externí odkaz:
https://doaj.org/article/7c8099d41342478299a5ff021f21b6b9
Autor:
Taichi Kawamura, Matthias Grott, Raphael Garcia, Mark Wieczorek, Sébastien de Raucourt, Philippe Lognonné, Felix Bernauer, Doris Breuer, John Clinton, Pierre Delage, Mélanie Drilleau, Luigi Ferraioli, Nobuaki Fuji, Anna Horleston, Günther Kletetschka, Martin Knapmeyer, Brigitte Knapmeyer-Endrun, Sebastiano Padovan, Ana-Catalina Plesa, Attilio Rivoldini, Johan Robertsson, Sebastien Rodriguez, Simon C. Stähler, Eleonore Stutzmann, Nicholas A. Teanby, Nicola Tosi, Christos Vrettos, Bruce Banerdt, Wenzhe Fa, Qian Huang, Jessica Irving, Yoshiaki Ishihara, Katarina Miljković, Anna Mittelholz, Seiichi Nagihara, Clive Neal, Shaobo Qu, Nicholas Schmerr, Takeshi Tsuji
Publikováno v:
Experimental Astronomy. 54:617-640
Geophysical observations will provide key information about the inner structure of the planets and satellites and understanding the internal structure is a strong constraint on the bulk composition and thermal evolution of these bodies. Thus, geophys
Autor:
Jessica C. E. Irving, Vedran Lekić, Cecilia Durán, Mélanie Drilleau, Doyeon Kim, Attilio Rivoldini, Amir Khan, Henri Samuel, Daniele Antonangeli, William Bruce Banerdt, Caroline Beghein, Ebru Bozdağ, Savas Ceylan, Constantinos Charalambous, John Clinton, Paul Davis, Raphaël Garcia, null Domenico Giardini, Anna Catherine Horleston, Quancheng Huang, Kenneth J. Hurst, Taichi Kawamura, Scott D. King, Martin Knapmeyer, Jiaqi Li, Philippe Lognonné, Ross Maguire, Mark P. Panning, Ana-Catalina Plesa, Martin Schimmel, Nicholas C. Schmerr, Simon C. Stähler, Eleonore Stutzmann, Zongbo Xu
Publikováno v:
Proceedings of the National Academy of Sciences of the United States of America
Proceedings of the National Academy of Sciences of the United States of America, 2023, ⟨10.1073/pnas.2217090120⟩
Proceedings of the National Academy of Sciences of the United States of America, vol 120, iss 18
Proceedings of the National Academy of Sciences of the United States of America, 120 (18)
Proceedings of the National Academy of Sciences of the United States of America, 2023, ⟨10.1073/pnas.2217090120⟩
Proceedings of the National Academy of Sciences of the United States of America, vol 120, iss 18
Proceedings of the National Academy of Sciences of the United States of America, 120 (18)
We present the first observations of seismic waves propagating through the core of Mars. These observations, made using seismic data collected by the InSight geophysical mission, have allowed us to construct the first seismically constrained models f
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::95185c4d4ac2ea963394d0c8b4235f11
Autor:
Quancheng Huang, Nicholas C. Schmerr, Scott D. King, Doyeon Kim, Attilio Rivoldini, Ana-Catalina Plesa, Henri Samuel, Ross R. Maguire, Foivos Karakostas, Vedran Lekić, Constantinos Charalambous, Max Collinet, Robert Myhill, Daniele Antonangeli, Mélanie Drilleau, Misha Bystricky, Caroline Bollinger, Chloé Michaut, Tamara Gudkova, Jessica C. E. Irving, Anna Horleston, Benjamin Fernando, Kuangdai Leng, Tarje Nissen-Meyer, Frederic Bejina, Ebru Bozdağ, Caroline Beghein, Lauren Waszek, Nicki C. Siersch, John-Robert Scholz, Paul M. Davis, Philippe Lognonné, Baptiste Pinot, Rudolf Widmer-Schnidrig, Mark P. Panning, Suzanne E. Smrekar, Tilman Spohn, William T. Pike, Domenico Giardini, W. Bruce Banerdt
Publikováno v:
Proceedings of the National Academy of Sciences of the United States of America
Proceedings of the National Academy of Sciences of the United States of America, 2022, 119 (42), ⟨10.1073/pnas.2204474119⟩
Proceedings of the National Academy of Science
Proceedings of the National Academy of Sciences of the United States of America, 119 (42)
Huang, Q, Schmerr, N, Horleston, A C, Irving, J C E, Myhill, R C, Giardini, D & et, A 2022, ' Seismic detection of a deep mantle discontinuity within Mars by InSight ', Proceedings of the National Academy of Sciences of the United States of America, vol. 119, no. 42, e2204474119 . https://doi.org/10.1073/pnas.2204474119
Proceedings of the National Academy of Sciences of the United States of America, 2022, 119 (42), ⟨10.1073/pnas.2204474119⟩
Proceedings of the National Academy of Science
Proceedings of the National Academy of Sciences of the United States of America, 119 (42)
Huang, Q, Schmerr, N, Horleston, A C, Irving, J C E, Myhill, R C, Giardini, D & et, A 2022, ' Seismic detection of a deep mantle discontinuity within Mars by InSight ', Proceedings of the National Academy of Sciences of the United States of America, vol. 119, no. 42, e2204474119 . https://doi.org/10.1073/pnas.2204474119
Constraining the thermal and compositional state of the mantle is crucial for deciphering the formation and evolution of Mars. Mineral physics predicts that Mars' deep mantle is demarcated by a seismic discontinuity arising from the pressure-induced
Since being first visited by the spacecraft Cassini in 2005, the Saturnian moon Enceladus has attracted far more attention than could be guessed from its modest size and lack of atmosphere, compared to its giant neighbour Titan. The reason for this s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::47a7772cbc786d5e66107523fa9362d4
https://doi.org/10.5194/epsc2022-1042
https://doi.org/10.5194/epsc2022-1042