Using Earth-based Observations to Bootstrap Expected Signatures of Exoplanets

While multi-dimensional physical-chemical models of the upper atmospheres of Earth, Venus and Mars have been developed, they suffer from the many approximations that are related to the pure knowledge of network reaction and reaction rates ignited due to energetic particle precipitation. The major objective of the proposed research is to conduct a comprehensive and inter-disciplinary theory guided experimental study of Earth’s atmospheric chemistry irradiated by the energetic electrons and protons from flares from the Sun (simulated van der Graff Accelerator facility, a part of Radiation Laboratory at GSFC) with future applications to other planets in the Solar system and beyond.

This effort will address the problems of fundamental importance for Heliophysics and Planetary divisions with the major goal to improve the performance of multi-dimensional computer tools and provide a new capability to predict the state of Eartth’s upper atmosphere during extreme space weather events. Specifically, it will provide important interdisciplinary science input in support to a number of Heliophysics, Astrophysics and Planetary NASA mission. Specifically it will help inform measurements from GDC, DAVINCI, and MAVEN.

This is early/mid-stage (TRL 3) — the most realistic path in is NASA SBIR/STTR, which funds small businesses and research institutions to develop technology aligned with NASA's needs (equity-free, phased funding). Check whether a current SBIR/STTR solicitation topic overlaps with this project's technology area, or contact the project directly (above) to ask.

None of these are guaranteed paths for this specific project — TechPort itself doesn't have an "apply" button. Reaching out to the contact(s) above with a specific question is usually the fastest way to find out what's actually open.