J. M. Sunshine

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About

J. M. Sunshine is a leading figure in lunar photometry and planetary spectroscopy, whose work has fundamentally shaped how scientists calibrate remote sensing instruments using the Moon as a standard source. Her key research areas include lunar surface composition, visible and infrared spectrophotometry, and photometric correction techniques for planetary bodies. Sunshine’s most impactful contribution is the development of a wavelength-dependent photometric function for the Moon, derived from the USGS’s Robotic Lunar Observatory (ROLO) project. This empirical model, published in 2011 (49 citations), provides a critical calibration standard across 0.347–2.39 μm and solar phase angles from 1.55° to 97°, enabling consistent cross-instrument comparisons for Earth-observing satellites. Her follow-up work, “One Moon, many measurements 2: Photometric corrections” (2013, 41 citations), further refined these corrections, addressing variability in lunar observations from multiple platforms. Sunshine’s research has been instrumental in advancing lunar remote sensing, supporting NASA’s planetary missions, and improving the accuracy of global Earth observation data. Her meticulous empirical approach and dedication to calibration standards have made her a trusted authority in the field, with her ROLO-based models now widely adopted by the planetary science community.