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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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Magnetospheric period magnetic field oscillations at Saturn: Equatorial phase “jitter” produced by superposition of southern and northern period oscillations

TL;DR: In this article, the authors investigated magnetic field oscillations near the planetary rotation period in Saturn's magnetosphere observed during the initial near-equatorial phase of the Cassini mission.
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An auroral oval at the footprint of Saturn's kilometric radio sources, colocated with the UV aurorae

TL;DR: In this article, the authors present resolved SKR maps derived from the Cassini Radio and Plasma Wave Science (RPWS) experiment using goniopolarimetric techniques, which imply that the SKR and atmospheric aurorae are triggered by the same populations of energetic electron beams.
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Modeling of Io‐Jupiter decameter arcs, emission beaming and energy source

TL;DR: In this article, a good fit of arcs t-f location and shape is obtained for loss-cone driven (oblique) emission beamed in a hollow cone of half-angle ≥ 80° around the source magnetic field, closing at high frequencies, and of cone thickness ≤ 1°.
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On the character and distribution of lower-frequency radio emissions at Saturn and their relationship to substorm-like events

TL;DR: In this paper, a survey of low-frequency extensions during the equatorial orbits of the Cassini spacecraft at Saturn was conducted and three examples in each of which the SKR spectrum extends to lower frequencies than usual were presented.
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Variation of Saturn's UV aurora with SKR phase

TL;DR: In this article, the authors used an empirical SKR phase determined from Cassini observations to order the ‘quiet time’ total emitted UV auroral power as observed by the Hubble Space Telescope in programs during the interval 2005-2009.