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Merge pull request #6328 from nasa-gibs/release
Release to Main v4.82.0
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LICENSE.md

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This code was originally developed at NASA/Goddard Space Flight Center for
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the Earth Science Data and Information System (ESDIS) project.
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Copyright © 2013 - 2025 United States Government as represented by the
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Copyright © 2013 - 2026 United States Government as represented by the
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Administrator of the National Aeronautics and Space Administration.
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All Rights Reserved.
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## [NASA OPEN SOURCE AGREEMENT VERSION 1.3](https://opensource.gsfc.nasa.gov/nosa.php)
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## [NASA OPEN SOURCE AGREEMENT VERSION 1.3](https://opensource.org/license/nasa1-3-php)
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THIS OPEN SOURCE AGREEMENT ("AGREEMENT") DEFINES THE RIGHTS OF USE,
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REPRODUCTION, DISTRIBUTION, MODIFICATION AND REDISTRIBUTION OF CERTAIN
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**B.** Each Recipient must ensure that the following copyright notice appears
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prominently in the Subject Software:
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Copyright © 2012-2025 United States Government
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Copyright © 2012-2026 United States Government
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as represented by the Administrator of the
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National Aeronautics and Space Administration.
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All Rights Reserved.

config/default/common/brand/about/license.md

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<h2>License</h2>
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<p>Copyright © 2013 - 2025 United States Government as represented by the Administrator of the National Aeronautics
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<p>Copyright © 2013 - 2026 United States Government as represented by the Administrator of the National Aeronautics
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and Space Administration. All Rights Reserved. This software is licensed under the <a
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href="https://opensource.org/license/nasa1-3-php" target="_blank" rel="noopener noreferrer">NASA Open Source
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Software Agreement, Version 1.3</a>. Source code is available on the <a

config/default/common/colormaps/dcotss/DCOTSS_ER-2_ROZE_Ozone.xml

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config/default/common/colormaps/dcotss/DCOTSS_ER-2_UCATS_Ozone.xml

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The Dynamics and Chemistry to the Summer Stratosphere (DCOTSS) ER-2 Flight Tracks and Rapid Ozone Experiment (ROZE) Ozone data provide the location of where the NASA ER-2 aircraft collected data to support the campaign. These data include measurements of trace gas species, including Ozone. Ozone data featured in this layer were collected by the ROZE instrument, which is a broadband cavity-enhanced ultraviolet (UT) absorption instrument for the detection of in situ ozone.
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Each summer the North American Monsoon Anticyclone (NAMA) dominates the circulation of the North-Western Hemisphere and acts to partially confine and isolate air from the surrounding atmosphere. Strong convective storms in the NAMA regularly reach altitudes deep into the lower stratosphere, with some ascending above 20 km. These storms carry water and pollutants from the troposphere into the otherwise very dry stratosphere, where they can have a significant impact on radiative and chemical processes, potentially including destruction of stratospheric ozone. The Dynamics and Chemistry of the Summer Stratosphere (DCOTSS) field campaign was a NASA Earth Venture Suborbital research project aimed at investigating these thunderstorms. DCOTSS utilized NASA’s ER-2 aircraft and conducted two ~8-week science deployments based out of Salina, KS spanning early to late summer.
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References: DCOTSS at the ASDC, [doi:10.5067/ASDC/SUBORBITAL/DCOTSS/DATA001](https://asdc.larc.nasa.gov/project/DCOTSS); [DCOTSS Overview Publication](https://journals.ametsoc.org/view/journals/bams/aop/BAMS-D-24-0177.1/BAMS-D-24-0177.1.xml); [ROZE Overview](https://amt.copernicus.org/articles/13/6877/2020/amt-13-6877-2020.pdf)
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The Dynamics and Chemistry to the Summer Stratosphere (DCOTSS) ER-2 Flight Tracks and UAS Chromatograph for Atmospheric Trace Species (UCATS) Ozone data provide the location of where the NASA ER-2 aircraft collected data to support the campaign. These data include measurements of trace gas species, including Ozone. Ozone data featured in this layer were collected by the UCATS instrument, which uses gas chromatography to separate atmospheric traces along a narrow heated column, followed by precise and accurate detection with electron capture detectors.
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Each summer the North American Monsoon Anticyclone (NAMA) dominates the circulation of the North-Western Hemisphere and acts to partially confine and isolate air from the surrounding atmosphere. Strong convective storms in the NAMA regularly reach altitudes deep into the lower stratosphere, with some ascending above 20 km. These storms carry water and pollutants from the troposphere into the otherwise very dry stratosphere, where they can have a significant impact on radiative and chemical processes, potentially including destruction of stratospheric ozone. The Dynamics and Chemistry of the Summer Stratosphere (DCOTSS) field campaign was a NASA Earth Venture Suborbital research project aimed at investigating these thunderstorms. DCOTSS utilized NASA’s ER-2 aircraft and conducted two ~8-week science deployments based out of Salina, KS spanning early to late summer.
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References: DCOTSS at the ASDC, [doi:10.5067/ASDC/SUBORBITAL/DCOTSS/DATA001](https://asdc.larc.nasa.gov/project/DCOTSS); [DCOTSS Overview Publication](https://journals.ametsoc.org/view/journals/bams/aop/BAMS-D-24-0177.1/BAMS-D-24-0177.1.xml); [UCATS Overview](https://amt.copernicus.org/articles/14/6795/2021/)
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The OCO-2 Carbon Dioxide (Difference from Global Mean) is a layer that combines OCO-2 XCO<sub>2</sub> (column-averaged dry-air mole fraction) and an estimated daily global trend XCO<sub>2</sub> value that is produced by the National Oceanic and Atmospheric Administration Earth System Research Laboratory Global Monitoring Division (NOAA ESRL GMD). It is calculated from daily averaged CO<sub>2</sub> data from four surface stations and is subtracted from the OCO-2 XCO<sub>2</sub> in order to provide a product that visualizes smaller variations in XCO<sub>2</sub> than the raw XCO<sub>2</sub> product. This is done because increasing atmospheric CO<sub>2</sub> concentrations has resulted in a large range of XCO<sub>2</sub> values over the OCO-2 record.
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References: OCO2_L2_Lite_FP [doi:10.5067/5Q8JLZL1VD4A](https://doi.org/10.5067/5Q8JLZL1VD4A); [NOAA - What is the Global Greenhouse Gas Reference Network?](https://gml.noaa.gov/ccgg/about.html); [Ed Dlugokencky and Pieter Tans, NOAA/ESRL](https://esrl.noaa.gov/gmd/ccgg/trends/); [OCO-2 Carbon Dioxide in GIBS/Worldview](https://github.com/hcronk/oco2_worldview/blob/jpl/code/oco2_ref_co2_trend_gl.txt)
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References: OCO2_L2_Lite_FP [doi:10.5067/70K2B2W8MNGY](https://doi.org/10.5067/70K2B2W8MNGY); [NOAA - What is the Global Greenhouse Gas Reference Network?](https://gml.noaa.gov/ccgg/about.html); [Ed Dlugokencky and Pieter Tans, NOAA/ESRL](https://esrl.noaa.gov/gmd/ccgg/trends/); [OCO-2 Carbon Dioxide in GIBS/Worldview](https://github.com/hcronk/oco2_worldview/blob/jpl/code/oco2_ref_co2_trend_gl.txt)
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The OCO-2 Carbon Dioxide (Total Column Average) layer displays the column-averaged dry-air mole fraction of carbon dioxide (XCO<sub>2</sub>) in the vertical column of the atmosphere (i.e. from Earth’s surface to the top of the atmosphere) and is measured in parts per million (ppm).
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References: OCO2_L2_Lite_FP [doi:10.5067/5Q8JLZL1VD4A](https://doi.org/10.5067/5Q8JLZL1VD4A); Crisp et al. The ACOS CO2 Retrieval Algorithm - Part 2: Global XCO2 data Characterization Atmos. Meas. Tech., 5, 687-707, 2012; [GES DISC - OCO-2 Documents](https://disc.gsfc.nasa.gov/information/documents?title=OCO-2%20Documents); [OCO-2 Data Collections](https://disc.gsfc.nasa.gov/datasets?project=OCO)
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References: OCO2_L2_Lite_FP [doi:10.5067/70K2B2W8MNGY](https://doi.org/10.5067/70K2B2W8MNGY); Crisp et al. The ACOS CO2 Retrieval Algorithm - Part 2: Global XCO2 data Characterization Atmos. Meas. Tech., 5, 687-707, 2012; [GES DISC - OCO-2 Documents](https://disc.gsfc.nasa.gov/information/documents?title=OCO-2%20Documents); [OCO-2 Data Collections](https://disc.gsfc.nasa.gov/datasets?project=OCO)

config/default/common/config/metadata/layers/oco2/OCO-2_Solar_Induced_Florescence_757nm.md

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One of the OCO-2 channels, the O<sub>2</sub> A-band, contains multiple Fraunhofer lines and thus allows for the retrieval of SIF. The absorption at 771 nm is about 1.5 times smaller than at 757 nm, but both values are made available for analysis. However, the blended SIF is the recommended product. The OCO-2 Solar Induced Chlorophyll Fluorescence 771 nm parameter is taken from the OCO-2 Level 2 Lite SIF product. OCO-2 makes eight simultaneous, adjacent measurements, each with a spatial resolution of 2.25 km x 1.29 km. These measurements are then mapped onto a 500 m<sup>2</sup> grid. The repeat cycle for OCO-2 is every 16 days.
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References: OCO2_L2_Lite_SIF [doi:10.5067/OTRE7KQS8AU8](https://doi.org/10.5067/OTRE7KQS8AU8)
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References: OCO2_L2_Lite_SIF [doi:10.5067/8XXUQU7HBGBL](https://doi.org/10.5067/8XXUQU7HBGBL)
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Frankenberg et al. Prospects for chlorophyll fluorescence remote sensing from the Orbiting Carbon Observatory-2, Remote Sensing of Environment, Vol 147, 5 May. 2014, Pgs 1-12, [doi:10.1016/j.rse.2014.02.007](https://doi.org/10.1016/j.rse.2014.02.007)

config/default/common/config/metadata/layers/oco2/OCO-2_Solar_Induced_Florescence_771nm.md

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One of the OCO-2 channels, the O<sub>2</sub> A-band, contains multiple Fraunhofer lines and thus allows for the retrieval of SIF. The absorption at 771 nm is about 1.5 times smaller than at 757 nm, but both values are made available for analysis. However, the blended SIF is the recommended product. The OCO-2 Solar Induced Chlorophyll Fluorescence 771 nm parameter is taken from the OCO-2 Level 2 Lite SIF product. OCO-2 makes eight simultaneous, adjacent measurements, each with a spatial resolution of 2.25 km x 1.29 km. These measurements are then mapped onto a 500 m<sup>2</sup> grid. The repeat cycle for OCO-2 is every 16 days.
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References: OCO2_L2_Lite_SIF [doi:10.5067/OTRE7KQS8AU8](https://doi.org/10.5067/OTRE7KQS8AU8)
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References: OCO2_L2_Lite_SIF [doi:10.5067/8XXUQU7HBGBL](https://doi.org/10.5067/8XXUQU7HBGBL)
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Frankenberg et al. Prospects for chlorophyll fluorescence remote sensing from the Orbiting Carbon Observatory-2, Remote Sensing of Environment, Vol 147, 5 May. 2014, Pgs 1-12, [doi:10.1016/j.rse.2014.02.007](https://doi.org/10.1016/j.rse.2014.02.007)

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