Description: Development of compact telescopes and spectrometers flown on high-altitude aircraft and stratospheric balloons to observe the solar corona in the EUV and infrared with sensitivity to coronal magnetic fields.
Samra develops telescopes and spectrometers flown on aircraft and balloons to observe the solar corona at EUV and infrared wavelengths, including solar magnetometry, optical design, and modeling — a borderline but included astronomy-instrumentation case given its magnetometric sensing goal, though the platform is a classical (non-quantum) spectropolarimeter.