2 min read<\/p>\n
Preparations for Next Moonwalk Simulations Underway (and Underwater)<\/h1>\n<\/div>\n<\/div>\n<\/div>\n\n\n\n![\"A](\"https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/06\/asfmastercalibration-loiacono-04242025-2.jpg?w=2048\")
<\/a><\/figure>\nElectrical engineer Nikolas Gibson performs calibration tests on the MODIS\/ASTER Airborne Simulator (MASTER) spectrometer, co-developed by NASA\u2019s Ames Research Center and NASA\u2019s Jet Propulsion Laboratory. Gibson works at the Airborne Sensor Facility at Ames, which builds, maintains, miniaturizes, and calibrates instruments.<\/div>\nNASA\/Milan Loiacono<\/div>\n<\/figcaption><\/div>\n<\/div>\n<\/div>\nNASA\u2019s Ames Research Center in Silicon Valley houses a unique laboratory: the Airborne Sensor Facility (ASF). The engineers at the ASF are responsible for building, maintaining, and operating numerous instruments that get deployed on research aircraft, but one of their most important roles is instrument calibration.<\/p>\n<\/p>\n
Think of calibration like tuning a piano between performances: A musician uses a tuner to set the standard pitch for each string, ensuring that the piano remains on pitch for every concert.<\/p>\n<\/p>\n
The \u201ctuners\u201d at ASF include lasers, mirrors, and a light source called an integrating sphere \u2013 a hollow sphere about 36 inches in diameter that emits a set amount of light from a hole in the top. By checking an instrument against this baseline between each mission, engineers ensure that the instrument sensors provide accurate, reliable data every time.<\/p>\n<\/p>\n
In the photo above, electrical engineer Nikolas Gibson performs calibration tests on the MODIS\/ASTER Airborne Simulator (MASTER) spectrometer, co-developed by NASA Ames and NASA\u2019s Jet Propulsion Laboratory in Southern California.<\/p>\n<\/p>\n
A spectrometer separates light into individual wavelengths, providing researchers with information about the properties of whatever is creating or interacting with that light. The MASTER instrument measures about 50 individual spectral channels, providing data on wavelengths from the visible spectrum through the infrared.<\/p>\n<\/p>\n
When it comes to calibration, each of these channels functions like a specific key on a piano and needs to be individually checked against the \u201ctuner.\u201d By pointing the instrument\u2019s sensor at a known quantity of light coming from the integrating sphere, the team checks the accuracy of MASTER\u2019s data output and repairs or adjusts the sensor as needed.<\/p>\n<\/p>\n
In this image, MASTER had returned from an April 2025 scientific campaign observing \u00a0prescribed fires in Alabama and Georgia with NASA\u2019s FireSense<\/a> project. It was recalibrated before heading back into the field for the Geological Earth Mapping Experiment, or GEMx, \u00a0mission in late May 2025, which will use the instrument to help map critical minerals across the southwestern United States.<\/p>\n\n\n\nAbout the Author<\/h3>\n<\/div>\n<\/div>\n\n\n\n![\"Milan](\"https:\/\/www.nasa.gov\/wp-content\/uploads\/2023\/07\/cropped-img-4375-300x300.jpg\")
<\/div>\n\n\nMilan Loiacono<\/h2>\n<\/div>\nScience Communication Specialist<\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n\nMilan Loiacono is a science communication specialist for the Earth Science Division at NASA Ames Research Center.<\/p>\n<\/div>\n<\/div>\n<\/div>\n
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![\"A](\"https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/06\/asfmastercalibration-loiacono-04242025-2.jpg\")
<\/a><\/figure>NASA\u2019s Ames Research Center in Silicon Valley houses a unique laboratory: the Airborne Sensor Facility (ASF). The engineers at the ASF are responsible for building, maintaining, and operating numerous instruments that get deployed on research aircraft, but one of their most important roles is instrument calibration.<\/p>\n<\/p>\n
Think of calibration like tuning a piano between performances: A musician uses a tuner to set the standard pitch for each string, ensuring that the piano remains on pitch for every concert.<\/p>\n<\/p>\n
The \u201ctuners\u201d at ASF include lasers, mirrors, and a light source called an integrating sphere \u2013 a hollow sphere about 36 inches in diameter that emits a set amount of light from a hole in the top. By checking an instrument against this baseline between each mission, engineers ensure that the instrument sensors provide accurate, reliable data every time.<\/p>\n<\/p>\n
In the photo above, electrical engineer Nikolas Gibson performs calibration tests on the MODIS\/ASTER Airborne Simulator (MASTER) spectrometer, co-developed by NASA Ames and NASA\u2019s Jet Propulsion Laboratory in Southern California.<\/p>\n<\/p>\n
A spectrometer separates light into individual wavelengths, providing researchers with information about the properties of whatever is creating or interacting with that light. The MASTER instrument measures about 50 individual spectral channels, providing data on wavelengths from the visible spectrum through the infrared.<\/p>\n<\/p>\n
When it comes to calibration, each of these channels functions like a specific key on a piano and needs to be individually checked against the \u201ctuner.\u201d By pointing the instrument\u2019s sensor at a known quantity of light coming from the integrating sphere, the team checks the accuracy of MASTER\u2019s data output and repairs or adjusts the sensor as needed.<\/p>\n<\/p>\n
In this image, MASTER had returned from an April 2025 scientific campaign observing \u00a0prescribed fires in Alabama and Georgia with NASA\u2019s FireSense<\/a> project. It was recalibrated before heading back into the field for the Geological Earth Mapping Experiment, or GEMx, \u00a0mission in late May 2025, which will use the instrument to help map critical minerals across the southwestern United States.<\/p>\n Milan Loiacono is a science communication specialist for the Earth Science Division at NASA Ames Research Center.<\/p>\n<\/div>\n<\/div>\n<\/div>\nAbout the Author<\/h3>\n<\/div>\n<\/div>\n
<\/div>\nMilan Loiacono<\/h2>\n<\/div>\n
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