Statistics – Applications
Scientist
Statistics
Applications
Scientist
Lunar and Planetary Institute, 3600 Bay Area Boulevard, Houston, Texas 77058, USA; LANL, Space Science and Applications, ISR-1, Mail Stop D-466, Los Alamos, New Mexico 87545, USA
Aeronomie IPSL and LPG
Service d'aeronomie / IPSL, France
Service d'aeronomie, France
Lunar and Planetary Institute, Houston, Texas, USA
Lunar and Planetary Institute, 3600 Bay Area Boulevard, Houston, TX 77058, United States; Los Alamos National Laboratory, Los Alamos, NM 87545, United States
Universite Pierre et Marie Curie-Paris6; Service d'aeronomie-IPSL-CNRS UMR 7620 Univ Paris 06, UMR 7620, Aéronomie CNRS-IPSL, BP 3, F-91371 Verrières, France
Service d'aéronomie-IPSL-CNRS, UMR 7620, Route des Gâtines, BP 3, 91371 Verrières-le-Buisson, France Alamos National Laboratory, Los Alamos, NM, USA; Los Alamos, NM, USA; Los Alamos, NM, USA; Space Science and Applications, ISR-1, Mail Stop D-466, Los Alamos, NM 87545, USA; Lunar and Planetary Institute, 3600 Bay Area Blvd., Houston, TX 77058, USA
Université de Paris, France
Université de Paris VI / Aéronomie
Université Paris 6, Service d'Aéronomie
CNRS Service aeronomie, France
UPMC Paris, Aeronomie, France
Lunar and Planetary Institute, Houston, USA
Lunar and Planetary Institute, Houston, TX USA
Lunar and Planetary Institute, Houston, 77058 TX, USA
University of Paris, Service d'Aéronomie CNRS, BP3 - Route des Gatines, F-91371 Verrieres, France
Université Pierre et Marie Curie-Paris6, Aéronomie CNRS-IPSL, BP 3, 91371 Verrières, France
LPI
Laboratoire de Planétologie de Grenoble, France
LPI, Houston, USA
LANL, Los Alamos, NM, USA
LPI, Houston, TX, USA Univ. Paris 06, UMR 7620, LATMOS / IPSL, BP 3, F-91371 Verrières Cedex, France; Lunar and Planetary Institute, 3600 Bay Area Blvd., Houston, TX 77058,
A 3-dimensional Thermal Model For Icy Bodies In The Solar System.
Aggregates model to describe light scattering by cometary dust
Appearance of layered structures in numerical simulations of polydisperse bodies accretion: Application to cometary nuclei
Approaching Interplanetary Dust Physical Properties from Light Scattering and Thermal Observations and Simulations
Approaching Interplanetary Dust Physical Properties, from Light Scattering and Thermal Observations and Simulations
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