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The International Space Station was orbiting on a northeast track 261 miles above the Pacific Ocean when this photograph captured the first rays of an orbital sunrise illuminating Earth's atmosphere.
Okorn installing an INSTEP monitor on a rooftop at NASA Ames

Atmospheric Composition and Dynamics Instruments at Ames

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Charles Gatebe

Cloud Absorption Radiometer (CAR)

CAR is a multispectral scanner, designed to operate on various aircraft, such as NASA’s P-3B. It was originally designed for making scattered solar radiation measurements deep within a cloud layer over a wide angular range (190°) for determining the spectral absorption of solar radiation by clouds. It has been used most extensively since 1991 for measuring the bidirectional reflectance-distribution function (BRDF) of a wide variety of terrestrial surfaces as well as clouds and smoke embedded in the atmosphere. CAR’s unique measurement geometry allows a comparison of measurements acquired from different satellite instruments with various geometrical configurations, none of which are capable of obtaining such a complete and nearly instantaneous BRDF. The instrument supported the 2022 SaSa (Student Airborne Science Activation) field campaign aboard the NASA P-3B.

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CAR mounted on nose of J-31. It looks to be cylinder shaped with a head at the end while a red plane is in the background
CAR is a multi-wavelength scanning radiometer for determining albedo of clouds in the visible and near-infrared and measuring the angular distribution of scattered radiation and bidirectional reflectance of various surface types. It acquires imagery of cloud and Earth surface features.

Meteorological Measurement System (MMS)

Named for American rocketry pioneer Dr. Robert H. Goddard, the center was established May 1, 1959, as NASA's first space flight complex.

MMS is a state-of-the-art instrument system that is operated on various NASA aircraft for measuring accurate, high resolution in-situ airborne state parameters (pressure, temperature, turbulence index, and the 3-dimensional wind vector). The MMS system has been used for over 100 publications, and that number continues to grow. This is indicative of the essential contribution of high-quality meteorological information for analyses of aircraft observations.

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Image of the Meteorological Measurement System (MMS) for planes. This is a still from an ESPO video
The Meteorological Measurement System (MMS) is a state-of-the-art instrument for measuring accurate, high resolution in situ airborne state parameters (pressure, temperature, turbulence index, and the 3-dimensional wind vector). These key measurements enable our understanding of atmospheric dynamics, chemistry and microphysical processes. The MMS is used to investigate atmospheric mesoscale (gravity and mountain lee waves) and microscale (turbulence) phenomena.

Inexpensive Network Sensor Technology for Exploring Pollution (INSTEP)

INSTEP is a network of low-cost gas sensors based on a design from the Hannigan Lab at the University of Colorado Boulder. The INSTEP monitors measure a variety of trace gases (CH4, HCHO, CO, CO2, NO2, O3) and have been placed around the San Francisco Bay and Los Angeles areas for satellite, ground-based remote sensing, and airborne measurement validation.

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The INSTEP monitors measure a variety of trace gases (CH4, HCHO, CO, CO2, NO2, O3) and will be placed around the San Francisco Bay and Los Angeles areas. Red markers refer to a monitor placed on its own; blue dots indicate monitors co-located with remote sensing instruments for validation purposes.

Carbon monOxide Measurement from Ames (COMA)

COMA is an Off-Axis Integrated Cavity Output Spectroscopy (OA-ICOS) instrument developed by Los Gatos Research (now ABB Ltd.) and extensively modified for high-altitude airborne in-situ measurements of carbon monoxide (CO) and nitrous oxide (N2O). The instrument supported the 2022 ACCLIP (Asian Summer Monsoon Chemical and CLimate Impact Project) mission aboard the NASA WB-57F.

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Image of JSC Aircraft Ops WB-57 Science Campaign
JSC Aircraft Ops WB-57 Science Campaign – Asian Summer Monsoon Chemical and Climate Impact Project (ACCLIP). Photo Date: August 17, 2021. Location: Ellington Field – Hangar 990 & 994.
Robert Markowitz

Spectrometer for Sky-Scanning, Sun-Tracking Atmospheric Research (4STAR)

4STAR is an airborne sun-sky spectrophotometer measuring direct solar beam transmittance at various spectral channels between 350 nm and 1650 nm. It is used to quantify properties of various atmospheric constituents such as the spectral aerosol optical depth (AOD), and aerosol intensive properties such as single scattering albedo (SSA), asymmetry parameter, scattering phase function, absorption angstrom exponent, size distribution, and index of refraction.

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4STAR Instrument Installed in DC-8: SEAC4RS Mission
Scientists installed components of the Spectrometer for Sky-Scanning, Sun-Tracking Atmospheric Research (4STAR) instrument into NASA’s DC-8 flying laboratory for data collection during a complex mission to study how air pollution and natural emissions affect climate change.

Rapid Ozone Experiment (ROZE)

ROZE is an in-situ instrument capable of measuring ozone (O3) throughout the troposphere and lower stratosphere and more sensitive (500 X) than any commercially available ozone photometer. It can be operated in a range of field environments, including low- and high-altitude research aircraft, and is particularly suited to O3 vertical-flux measurements using the eddy covariance technique.

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Photo of wires of the NASA Rapid OZone Experiment (ROZE) is an in situ instrument capable of measuring ozone (O3) throughout the troposphere and lower stratosphere on airborne platforms. The instrument uses cavity-enhanced absorption to measure the amount of ozone in a sampled volume flowing through an optical cell.
The NASA Rapid OZone Experiment (ROZE) is an in situ instrument capable of measuring ozone (O3) throughout the troposphere and lower stratosphere on airborne platforms. The instrument uses cavity-enhanced absorption to measure the amount of ozone in a sampled volume flowing through an optical cell.