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Baptiste Cecconi

Researcher at University of Paris

Publications -  268
Citations -  5427

Baptiste Cecconi is an academic researcher from University of Paris. The author has contributed to research in topics: Magnetosphere of Saturn & Magnetosphere. The author has an hindex of 38, co-authored 252 publications receiving 4784 citations. Previous affiliations of Baptiste Cecconi include Janssen Pharmaceutica & University of Toulouse.

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Description, accessibility and usage of SOIR/Venus Express atmospheric profiles of Venus distributed in VESPA (Virtual European Solar and Planetary Access)

TL;DR: Venus Express SOIR profiles of pressure, temperature and number densities of different constituents of the mesosphere and lower thermosphere of Venus are the only experimental data covering the 60 km to 220 km range of altitudes at the terminator of Venus as mentioned in this paper.

Planetary GIS and EuroPlanet-RI H2020

TL;DR: In this paper, a workshop on Planetary GIS in broad sense and with particular reference to ESA data archives has been organized, which is strongly supported by ESA and the broad planetary community, both directly and through its official channel for Planetary Science archive science access and exploitation-related needs, the PSA User Group.

Wind/WAVES Observations of Auroral Kilometric Radiation: Automated Burst Detection and Terrestrial Solar Wind ‐ Magnetosphere Coupling Effects

TL;DR: Auroral Kilometric radiation (AKR) is the strongest terrestrial radio emission, and emanates from the same electron acceleration regions from which particles precipitate into the ionosphere, exciting the aurorae and other phenomena as mentioned in this paper .
Proceedings ArticleDOI

Saturn Kilometric Radiation Near a Source Center on Day 73, 2008

TL;DR: The radio and plasma wave instrument, RPWS, observed intense SKR in the extraordinary (X) mode as discussed by the authors, and the electron low-energy spectrometer (ELS) obtained a phase space distribution of sufficient energy and pitch angle resolution to allow growth rate calculations for the observed wave emissions.