Exoplanet & Planetary Atmosphere Modeling
One of the main focus area of the Exoplanets and Planetary Atmospheres research group at NISER
is to develop forward and inverse models to plan and interpret the observations
of exoplanets. SANSAR (Suite of Adaptable plaNetary atmoSphere model And Retrieval) a state of the art
adaptable planetary atmosphere model is being developed in this group.
Exoplanet Observations Planning & Data Reduction
Transiting exoplanet observations from space telescopes like TESS, HST and JWST
are also reduced by our group members to characterize these far away worlds. Atmosphere
models are also used to generate simulated observations for planning observations.
Shukrayaan - ISRO's Venus Mission
Our research group members are involved in developing spectro-polarimetric models for planning observations
from Venus Atmospheric SpectroPolarimeter (VASP) instrument onboard
Shukrayaan (Venus Orbiter Mission) scheduled to launch in 2028 and later after the launch to interpret these observations.
Earth's Atmosphere & Remote Sensing
We also develop retrieval algorithms to constrain various properties of the Earth's atmosphere,
ocean and surfaces, focusing on Indian sub-continent and surrounding region. Various aspects of SANSAR model are benchmarked with Earth based observations and models.