The Student Thermal Energetic Activity Module (STEAM) is a collaboration with the Southwest AV名湿 Institute (SwRI) to search for X-ray signatures of coronal heating mechanisms. STEAM is a supplementary experiment to .聽STEAM's CAD can be seen below, with dimensions.
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STEAM will house two Amptek off-the-shelf X-ray spectrometers and all associated electronics. The exterior structure will be composed of Aluminum 7075 to allow for low mass structural integrity that can withstand the forces of launch, while also shielding against ionizing radiation in orbit. The spectrometer configuration will allow for the separation of the pre-amplifiers and detector heads from the main electronics to reduce volume. To minimize signal from the cosmic background radiation, exterior aluminum baffles will constrain the field of view of the detectors. Experimental calibration of both spectrometers will be done before and after integration, through calibrated X-ray emitting radioactive isotope source measurements as well as instrument response matrix implementation.
By exploring the signatures of low First Ionization Potential (FIP) elements in solar flares and active regions, STEAM will infer the origin of plasma through comparing enhancement factors in the corona over chromospheric abundances. STEAM will be doing data analysis using emission database modeling, and will derive the temperature and abundances from observables. There is potential for STEAM to use machine learning for further analysis. This data will contribute to efforts towards better understanding how magnetic reconnection-based solar events and quiescent active regions contribute to the heating of the corona.