CLASP (Chromospheric Lyman Alpha Spectro Polarimeter, NASA) is another rocket-borne instrument which objective is the measure of the polarisation of chromospheric Ly alpha radiation in order to measure the chromospheric magnetic field.
Contact: F. Auchère
REMi (Reflectance d'Échantillons Microscopiques), spectroscopy device for microscopic samples in the visible and near infrared in a clean room.
Contacts : Zahia Djouadi, Cateline Lantz, Rosario Brunetto
The sample under the microscope is illuminated (via a fiber) by a halogen lamp, it reflects part of the light which is collected by a second fiber and routed to a spectrometer with a spectral range [0.45, 1.0] µm.
PRONEXT (PROcessus NEbulaires à la surface des grains EXTraterrestres), is a commercial cell (from SPECAC) operating at different temperatures [300, 1000 K] and high pressures up to ~69 bar. It fits in the sample compartment of a Bruker VERTEX 70 FTIR spectrometer.
The system is associated with a mixing line and a pumping system. This makes it possible to control the composition of the initial gas mixture sent into the reactor and maintained at low pressure. The plasma that forms in the reactor is induced and maintained by a microwave discharge coupled with an Evenson cavity. The device is such that part of the solid organic matter produced is deposited in the form of a thin film directly on an ad hoc support, facilitating subsequent characterizations, particularly by infrared.
Contact : Donia Baklouti
INGMAR (IrradiatioN de Glaces et Météorites Analysées par Réflectance VIS-IR
Euclid is an ESA mission that will map the geometry of the Dark Universe. The mission will investigate the distance-redshift relationship and the evolution of cosmic structures by measuring shapes and redshifts of galaxies and clusters of galaxies out to redshifts ~2, or equivalently to a look-back time of 10 billion years. In this way, Euclid will cover the entire period over which Dark Energy played a significant role in accelerating the expansion of the Universe.
Contact IAS: Nabila Aghanim & Hervé Dole
The Sun and its corona as seen by HECOR and HEIT: preliminary results.
Launched on September 14, 2009 from White Sands Missile Range (New Mexico), the Herschel sounding rocket was carrying two experiments with strong IAS participation: HECOR and HEIT.
IRIS (Interface Region Imaging Spectrograph, NASA, launched in 2013) combines imagers and a spectrograph. The solar group gets interest in this mission for its diagnosis capacities of the solar plasma based on these two technics.
Contact: J-C Vial
The BepiColombo mission was launched on October 19, 2018 for an arrival at Mercury in 2026. This ambitious mission will study all aspects of the closest planet to the sun, from interior to surface to magnetosphere. More details on the launch here.
Contacts : Yves Langevin, François Poulet, Mathieu Vincendon
OSIRIS-REx (for Origins, Spectral Interpretation, Resource Identification, Security, Regolith Explorer) is a NASA space mission which aims to bring back to Earth at the end of 2023 samples of the carbonaceous near-Earth asteroid Bennu.
The probe was launched in September 2016 and arrived near Bennu in December 2018. Since then, it has been in orbit mapping the entire surface of the asteroid in order to choose the best place to collect samples. The collection at the Nightingale site was a success in autumn 2020.
