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Quantitation of circulating viral RNAs as a new biomaker of Hepatitis B functional cure
Le RHU CirB-RNA a pour objectif de valider les ARN circulants du virus de l’hépatite B (VHB) comme biomarqueur d’une guérison fonctionnelle de l’hépatite B chronique. Les projets menés visent à *caractériser d’un point de vue biologique les compartiments et les différentes espèces d’ARNs circulants
Compact circulator operating in Ku band – CirCKu
This 30 months duration project concerns the development of compact circulators for applications in the Ku band, a frequency band in which new systems for defense and space telecommunications are developed. These components, essential in transmitter/receiver (T/R) modules, are today the main shortco
Signature de trois conventions territoriales entre la région Pays de la Loire et l’ANR, l’ANRT et le CNRS pour soutenir la recherche et l’innovation
Téléchargez le communiqué de presse La coopération entre les opérateurs de recherche nationaux et les collectivités territoriales est indispensable pour accompagner les équipes de recherche au plus près de leurs besoins, notamment de financement et permettre ainsi la prise d’initiative au profit
Chemical and optical evolution of TITAn's aerosols under high-energy RADiation – TITARAD
The 13-year (2004-2017) exploration of the Saturnian system by the Cassini-Huygens mission has revealed that Titan's atmospheric chemistry is by far the most complex of any observed in the solar system. In the upper atmosphere, Cassini's mass spectrometers (INMS and CAPS) detected the presence of po
Analysis of Photometric Observations for the Study of Titan Climate – APOSTIC
The scope of this project is to understand Titan climate system with the use of a couple 3D General Circulation Model, and with a meteorological record of different observable fields from recent observations. Since the arrival of Cassini in 2004 and Huygens in 2005, our knowledge of this planetary
Modélisation des climats de Titan et Vénus – EXOCLIMATS
Today, as space missions exploring planetary atmospheres are highly successful, with scientific teams now collecting a large amount of data, the study of the detailed aspects of all the mechanisms controling these complex atmospheric systems becomes possible. However, the interpretation of Cassini-H
