Update to v4.41.1 upstream

Dockerfile

@@ -19,7 +19,7 @@ RUN dnf install -y epel-release && \
     xz
 RUN mkdir -p /usr/local/nvm
 ENV NVM_DIR=/usr/local/nvm
-ENV NODE_VERSION=20.11.0
+ENV NODE_VERSION=20.12.2
 RUN curl -o- https://raw.githubusercontent.com/nvm-sh/nvm/v0.39.3/install.sh | bash && \
     . "$NVM_DIR/nvm.sh" && \
     nvm install v${NODE_VERSION} && \

config/active/common/colormaps/orbits/OrbitTracks_Sentinel-3A_Ascending.xml

@@ -0,0 +1,12 @@
+<?xml version="1.0" encoding="utf-8"?>
+<ColorMaps xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
+           xsi:noNamespaceSchemaLocation="http://gibs.earthdata.nasa.gov/schemas/ColorMap_v1.3.xsd">
+  <ColorMap title="Sentinel-3A Orbital Track">
+    <Entries>
+      <ColorMapEntry rgb="3,17,252" sourceValue="200" transparent="false" ref="1" />
+    </Entries>
+    <Legend type="classification">
+      <LegendEntry rgb="3,17,252" id="1" tooltip="Acquisition Time (UTC)" label="Acquisition Time (UTC)" showLabel="true" />
+    </Legend>
+  </ColorMap>
+</ColorMaps>

config/active/common/colormaps/orbits/OrbitTracks_Sentinel-3A_Descending.xml

@@ -0,0 +1,12 @@
+<?xml version="1.0" encoding="utf-8"?>
+<ColorMaps xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
+           xsi:noNamespaceSchemaLocation="http://gibs.earthdata.nasa.gov/schemas/ColorMap_v1.3.xsd">
+  <ColorMap title="Sentinel-3A Orbital Track">
+    <Entries>
+      <ColorMapEntry rgb="3,17,252" sourceValue="200" transparent="false" ref="1" />
+    </Entries>
+    <Legend type="classification">
+      <LegendEntry rgb="3,17,252" id="1" tooltip="Acquisition Time (UTC)" label="Acquisition Time (UTC)" showLabel="true" />
+    </Legend>
+  </ColorMap>
+</ColorMaps>

config/active/common/colormaps/orbits/OrbitTracks_Sentinel-3B_Ascending.xml

@@ -0,0 +1,12 @@
+<?xml version="1.0" encoding="utf-8"?>
+<ColorMaps xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
+           xsi:noNamespaceSchemaLocation="http://gibs.earthdata.nasa.gov/schemas/ColorMap_v1.3.xsd">
+  <ColorMap title="Sentinel-3B Orbital Track">
+    <Entries>
+      <ColorMapEntry rgb="245,66,138" sourceValue="200" transparent="false" ref="1" />
+    </Entries>
+    <Legend type="classification">
+      <LegendEntry rgb="245,66,138" id="1" tooltip="Acquisition Time (UTC)" label="Acquisition Time (UTC)" showLabel="true" />
+    </Legend>
+  </ColorMap>
+</ColorMaps>

config/active/common/colormaps/orbits/OrbitTracks_Sentinel-3B_Descending.xml

@@ -0,0 +1,12 @@
+<?xml version="1.0" encoding="utf-8"?>
+<ColorMaps xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
+           xsi:noNamespaceSchemaLocation="http://gibs.earthdata.nasa.gov/schemas/ColorMap_v1.3.xsd">
+  <ColorMap title="Sentinel-3B Orbital Track">
+    <Entries>
+      <ColorMapEntry rgb="245,66,138" sourceValue="200" transparent="false" ref="1" />
+    </Entries>
+    <Legend type="classification">
+      <LegendEntry rgb="245,66,138" id="1" tooltip="Acquisition Time (UTC)" label="Acquisition Time (UTC)" showLabel="true" />
+    </Legend>
+  </ColorMap>
+</ColorMaps>

config/active/common/config/metadata/layers/aeronet/AERONET_ANGSTROM_440-870NM.md

@@ -0,0 +1,9 @@
+The AERONET Angstrom Parameter 440-870nm (Near Real-Time) layer provides the Angstrom parameter from the Level 1.5 data for AERONET ground-based remote sensing aerosol network sites. The angstrom parameter provides additional information related to the aerosol particle size (larger the value, the smaller the particle size). Values < 1 suggest optical dominance of coarse particles (e.g. dust) and values > 1 suggest optical dominance of fine particles (e.g. smoke).
+
+The angstrom parameter is calculated for all available wavelengths within the Angstrom parameter range. For example, the Angstrom 870-440nm includes the 870, 670, 500 and 440 nm AOD data. A special case for a polarized instrument is Angstrom 870-440nm which only includes 870, 670 and 440 nm AOD data (polarized instruments do not have 500nm channel). Level 1.5 is automatically cloud cleared but may not have final calibration applied. These data are NOT quality assured.
+
+Each AERONET ground-based remote sensing aerosol network site consist of a sun photometer and satellite transmission system. Sun photometer measurements of the direct (collimated) solar radiation provide information to calculate the columnar aerosol optical depth (AOD). AOD can be used to compute columnar water vapor (Precipitable Water) and estimate the aerosol size using the Angstrom parameter relationship.
+
+The Near Real-Time layer displays the reading from the last one hour, ranging from < 0.0 to >= 2.5. Inactive sites are denoted in grey. Data for this layer is provided by the The AErosol RObotic NETwork ([AERONET](https://aeronet.gsfc.nasa.gov/)) program.
+
+References: [AERONET Aerosol Optical Depth](https://aeronet.gsfc.nasa.gov/new_web/aerosols.html)

config/active/common/config/metadata/layers/aeronet/AERONET_AOD_500NM.md

@@ -0,0 +1,9 @@
+The Aerosol Optical Depth 500nm (Near Real-Time) layer shows aerosol optical depth at 500 nanometers (nm) from the Level 1.5 data for AERONET ground-based remote sensing aerosol network sites. Level 1.5 is automatically cloud cleared but may not have final calibration applied. These data are NOT quality assured.
+
+Aerosol Optical Depth (AOD) (or Aerosol Optical Thickness) indicates the level at which particles in the air (aerosols) prevent light from traveling through the atmosphere. Aerosols scatter and absorb incoming sunlight, which reduces visibility. From an observer on the ground, an AOD of less than 0.1 is “clean” - characteristic of clear blue sky, bright sun and maximum visibility. As AOD increases to 0.5, 1.0, and greater than 3.0, aerosols become so dense that sun is obscured. Sources of aerosols include pollution from factories, smoke from fires, dust from dust storms, sea salt, and volcanic ash and smog. Aerosols compromise human health when inhaled by people, particularly those with asthma or other respiratory illnesses. Aerosols also have an effect on the weather and climate by cooling or warming the Earth, helping or preventing clouds from forming.
+
+Each AERONET ground-based remote sensing aerosol network site consist of a sun photometer and satellite transmission system. Sun photometer measurements of the direct (collimated) solar radiation provide information to calculate the columnar aerosol optical depth (AOD). AOD can be used to compute columnar water vapor (Precipitable Water) and estimate the aerosol size using the Angstrom parameter relationship.
+
+The Near Real-Time layer displays the reading from the last one hour, ranging from < 0.0 to 5.0. Inactive sites are denoted in grey. Data for this layer is provided by the The AErosol RObotic NETwork ([AERONET](https://aeronet.gsfc.nasa.gov/)) program.
+
+References: [AERONET Aerosol Optical Depth](https://aeronet.gsfc.nasa.gov/new_web/aerosols.html)

config/active/common/config/metadata/layers/aeronet/DAILY_AERONET_ANGSTROM_440-870NM.md

@@ -0,0 +1,10 @@
+The AERONET Angstrom Parameter 440-870nm (Daily) layer provides the Angstrom parameter from the Level 1.5 data for AERONET ground-based remote sensing aerosol network sites. The angstrom parameter provides additional information related to the aerosol particle size (larger the value, the smaller the particle size). Values < 1 suggest optical dominance of coarse particles (e.g. dust) and values > 1 suggest optical dominance of fine particles (e.g. smoke).
+
+The angstrom parameter is calculated for all available wavelengths within the Angstrom parameter range. For example, the Angstrom 870-440nm includes the 870, 670, 500 and 440 nm AOD data. A special case for a polarized instrument is Angstrom 870-440nm which only includes 870, 670 and 440 nm AOD data (polarized instruments do not have 500nm channel). Level 1.5 is automatically cloud cleared but may not have final calibration applied. These data are NOT quality assured.
+
+Each AERONET ground-based remote sensing aerosol network site consist of a sun photometer and satellite transmission system. Sun photometer measurements of the direct (collimated) solar radiation provide information to calculate the columnar aerosol optical depth (AOD). AOD can be used to compute columnar water vapor (Precipitable Water) and estimate the aerosol size using the Angstrom parameter relationship.
+
+The Daily layer displays the daily average based on the UTC solar day, ranging from < 0.0 to >= 2.5. Inactive sites are denoted in grey. Data for this layer is provided by the The AErosol RObotic NETwork ([AERONET](https://aeronet.gsfc.nasa.gov/)) program.
+
+References: [AERONET Aerosol Optical Depth](https://aeronet.gsfc.nasa.gov/new_web/aerosols.html)
+

config/active/common/config/metadata/layers/aeronet/DAILY_AERONET_AOD_500NM.md

@@ -0,0 +1,9 @@
+The Aerosol Optical Depth 500nm (Daily) layer shows aerosol optical depth at 500 nanometers (nm) from the Level 1.5 data for AERONET ground-based remote sensing aerosol network sites. Level 1.5 is automatically cloud cleared but may not have final calibration applied. These data are NOT quality assured.
+
+Aerosol Optical Depth (AOD) (or Aerosol Optical Thickness) indicates the level at which particles in the air (aerosols) prevent light from traveling through the atmosphere. Aerosols scatter and absorb incoming sunlight, which reduces visibility. From an observer on the ground, an AOD of less than 0.1 is “clean” - characteristic of clear blue sky, bright sun and maximum visibility. As AOD increases to 0.5, 1.0, and greater than 3.0, aerosols become so dense that sun is obscured. Sources of aerosols include pollution from factories, smoke from fires, dust from dust storms, sea salt, and volcanic ash and smog. Aerosols compromise human health when inhaled by people, particularly those with asthma or other respiratory illnesses. Aerosols also have an effect on the weather and climate by cooling or warming the Earth, helping or preventing clouds from forming.
+
+Each AERONET ground-based remote sensing aerosol network site consist of a sun photometer and satellite transmission system. Sun photometer measurements of the direct (collimated) solar radiation provide information to calculate the columnar aerosol optical depth (AOD). AOD can be used to compute columnar water vapor (Precipitable Water) and estimate the aerosol size using the Angstrom parameter relationship.
+
+The Daily layer displays the daily average based on the UTC solar day, ranging from < 0.0 to 5.0. Inactive sites are denoted in grey. Data for this layer is provided by the The AErosol RObotic NETwork ([AERONET](https://aeronet.gsfc.nasa.gov/)) program.
+
+References: [AERONET Aerosol Optical Depth](https://aeronet.gsfc.nasa.gov/new_web/aerosols.html)

config/active/common/config/metadata/layers/aeronet/aeronet.md

@@ -0,0 +1,4 @@
+### About AERONET
+The [AERONET](https://aeronet.gsfc.nasa.gov/new_web/index.html) (AErosol RObotic NETwork) program is a federation of ground-based remote sensing aerosol networks established by [NASA](https://www.nasa.gov/) and [PHOTONS](https://www-loa.univ-lille1.fr/photons) (PHOtométrie pour le Traitement Opérationnel de Normalisation Satellitaire; [Univ. of Lille 1](http://www.univ-lille1.fr/), [CNES](http://www.cnes.fr/), and [CNRS-INSU](http://www.cnrs.fr/)) and is greatly expanded by networks (e.g., [RIMA](https://www.caelis.uva.es/rima/), [AeroSpan](https://research.csiro.au/acc/capabilities/aerospan/), [AEROCAN](http://www.aerocanonline.com/), [AEROSPAIN](https://aerospain.aemet.es/), [NEON](https://www.neonscience.org/), [NCU](https://www.ncu.edu.tw/en/index.html), and CARSNET) and [collaborators](https://aeronet.gsfc.nasa.gov/new_web/collaborators.html) from national agencies, institutes, universities, individual scientists, and partners. For more than 25 years, the project has provided long-term, continuous, and readily accessible public domain database of aerosol optical, microphysical and radiative properties for aerosol research and characterization, validation of satellite retrievals, and synergism with other databases. The network imposes standardization of [instruments](https://aeronet.gsfc.nasa.gov/new_web/system_descriptions_instrument.html), [calibration](https://aeronet.gsfc.nasa.gov/new_web/system_descriptions_calibration.html), [processing](https://aeronet.gsfc.nasa.gov/new_web/system_descriptions_processing.html) and [distribution](https://aeronet.gsfc.nasa.gov/new_web/system_descriptions_distribution.html).
+
+AERONET collaboration provides globally distributed observations of spectral aerosol optical depth (AOD), inversion products, and precipitable water in diverse aerosol regimes. Version 3 AOD data are computed for three data quality levels: Level 1.0 (unscreened), Level 1.5 (cloud-screened and quality-controlled), and Level 2.0 (quality-assured). Inversions, precipitable water, and other AOD-dependent products are derived from these levels and may implement additional quality checks.

config/active/common/config/metadata/layers/modis/aqua/MODIS_Aqua_Brightness_Temp_Band31_Day.md

@@ -1,4 +1,4 @@
-The MODIS Brightness Temperature (Band 31, Day) layer is the brightness temperature, measured in Kelvin (K), calculated from the top-of-the-atmosphere radiances. It does not provide an accurate temperature of either clouds nor the land surface, but it does show relative temperature differences which can be used to distinguish features both in clouds and over clear land.  It can be used to distinguish land, sea ice, and open water over the polar regions during winter (in cloudless areas).
+The MODIS Brightness Temperature (Band 31, Day) layer is the brightness temperature, measured in Kelvin (K), calculated from the top-of-the-atmosphere radiances. It does not provide an accurate temperature of either clouds or the land surface, but it does show relative temperature differences which can be used to distinguish features both in clouds and over clear land.  It can be used to distinguish land, sea ice, and open water over the polar regions during winter (in cloudless areas).
 
 The MODIS Brightness Temperature layer is calculated from MODIS Calibrated Radiances and is available from both the Terra (MOD02) and Aqua (MYD02) satellites. The sensor and imagery resolution is 1 km, and the temporal resolution is daily.
 

config/active/common/config/metadata/layers/modis/aqua/MODIS_Aqua_Brightness_Temp_Band31_Night.md

@@ -1,4 +1,4 @@
-The MODIS Brightness Temperature (Band 31, Night) layer is the brightness temperature, measured in Kelvin (K), calculated from the top-of-the-atmosphere radiances. It does not provide an accurate temperature of either clouds nor the land surface, but it does show relative temperature differences which can be used to distinguish features both in clouds and over clear land.  It can be used to distinguish land, sea ice, and open water over the polar regions during winter (in cloudless areas).
+The MODIS Brightness Temperature (Band 31, Night) layer is the brightness temperature, measured in Kelvin (K), calculated from the top-of-the-atmosphere radiances. It does not provide an accurate temperature of either clouds or the land surface, but it does show relative temperature differences which can be used to distinguish features both in clouds and over clear land.  It can be used to distinguish land, sea ice, and open water over the polar regions during winter (in cloudless areas).
 
 The MODIS Brightness Temperature layer is calculated from MODIS Calibrated Radiances and is available from both the Terra (MOD02) and Aqua (MYD02) satellites. The sensor and imagery resolution is 1 km, and the temporal resolution is daily.
 

config/active/common/config/metadata/layers/modis/terra/MODIS_Terra_Brightness_Temp_Band31_Day.md

@@ -1,4 +1,4 @@
-The MODIS Brightness Temperature (Band 31, Day) layer is the brightness temperature, measured in Kelvin (K), calculated from the top-of-the-atmosphere radiances. It does not provide an accurate temperature of either clouds nor the land surface, but it does show relative temperature differences which can be used to distinguish features both in clouds and over clear land.  It can be used to distinguish land, sea ice, and open water over the polar regions during winter (in cloudless areas).
+The MODIS Brightness Temperature (Band 31, Day) layer is the brightness temperature, measured in Kelvin (K), calculated from the top-of-the-atmosphere radiances. It does not provide an accurate temperature of either clouds or the land surface, but it does show relative temperature differences which can be used to distinguish features both in clouds and over clear land.  It can be used to distinguish land, sea ice, and open water over the polar regions during winter (in cloudless areas).
 
 The MODIS Brightness Temperature layer is calculated from MODIS Calibrated Radiances and is available from both the Terra (MOD02) and Aqua (MYD02) satellites. The sensor and imagery resolution is 1 km, and the temporal resolution is daily.
 

config/active/common/config/metadata/layers/modis/terra/MODIS_Terra_Brightness_Temp_Band31_Night.md

@@ -1,4 +1,4 @@
-The MODIS Brightness Temperature (Band 31, Night) layer is the brightness temperature, measured in Kelvin (K), calculated from the top-of-the-atmosphere radiances. It does not provide an accurate temperature of either clouds nor the land surface, but it does show relative temperature differences which can be used to distinguish features both in clouds and over clear land.  It can be used to distinguish land, sea ice, and open water over the polar regions during winter (in cloudless areas).
+The MODIS Brightness Temperature (Band 31, Night) layer is the brightness temperature, measured in Kelvin (K), calculated from the top-of-the-atmosphere radiances. It does not provide an accurate temperature of either clouds or the land surface, but it does show relative temperature differences which can be used to distinguish features both in clouds and over clear land.  It can be used to distinguish land, sea ice, and open water over the polar regions during winter (in cloudless areas).
 
 The MODIS Brightness Temperature layer is calculated from MODIS Calibrated Radiances and is available from both the Terra (MOD02) and Aqua (MYD02) satellites. The sensor and imagery resolution is 1 km, and the temporal resolution is daily.
 

config/active/common/config/metadata/layers/multi-mission/opera/OPERA_L3_DIST-ALERT-HLS_Color_Index.md

@@ -0,0 +1,5 @@
+The OPERA Land Surface Disturbance (DIST-ALERT) imagery layer is a Level-3 (L3) product that maps per pixel vegetation disturbance (specifically, vegetation cover loss). Vegetation disturbance is mapped when there is an indicated decrease in vegetation cover within an HLS pixel. The spatial resolution is 30 m and the displayed layer describes vegetation disturbance status based on confidence, magnitude of loss, and whether it is ongoing. There are three confidence levels: "first detection" which is loss detected in only the most recent observation, "provisional" upon a second detection of vegetation loss, and "confirmed" once there are sufficient loss detections to reach high confidence of disturbance. These are reported for both disturbances with <50% vegetation cover loss and those with ≥50% loss, whether diffuse across an entire pixel or just a portion of it. These labels persist as long as the anomalies continue to be detected. Once a location no longer has low vegetation cover, confirmed alerts are labeled as "finished" and the others are reset to no disturbance. This status is iteratively updated with each subsequent granule.
+
+The input dataset for generating each product is the Harmonized Landsat Sentinel-2 (HLS) dataset. The OPERA Land Surface Disturbance (L3) imagery layer is available through the Observational Products for End-Users from Remote Sensing Analysis (OPERA) project.
+
+References: OPERA_L3_DIST-ALERT-HLS_V1 [doi:10.5067/SNWG/OPERA_L3_DIST-ALERT-HLS_V1.001](https://doi.org/10.5067/SNWG/OPERA_L3_DIST-ALERT-HLS_V1.001)

config/active/common/config/metadata/layers/oci/OCI_PACE_Chlorophyll_a.md

@@ -0,0 +1,5 @@
+The Chlorophyll a layer provides the near-surface concentration of chlorophyll a in milligrams of chlorophyll pigment per cubic meter (mg/m<sup>3</sup>) in the ocean.
+
+The Chlorophyll a product is available from the Ocean Color Instrument (OCI) aboard the PACE satellite. The sensor resolution is 1.2 km, imagery resolution is 1 km, and the temporal resolution is daily.
+
+References: [PACE_OCI_L2_BGC_NRT](https://cmr.earthdata.nasa.gov/search/concepts/C2910373790-OB_CLOUD.html); PACE_OCI_L2_BGC [doi:10.5067/PACE/OCI/L2/OC_BGC/V1](https://doi.org/10.5067/PACE/OCI/L2/OC_BGC/V1)

config/active/common/config/metadata/layers/oci/OCI_PACE_True_Color.md

@@ -0,0 +1,5 @@
+These images are called true-color or natural color because this combination of wavelengths is similar to what the human eye would see. The images are natural-looking images of land surface, oceanic and atmospheric features. The downside of this set of bands is that they tend to produce a hazy image.
+
+The sensor resolution is 1.2 km, imagery resolution is 1 km, and the temporal resolution is daily.
+
+References: [PACE_OCI_L2_SFREFL_NRT](https://cmr.earthdata.nasa.gov/search/concepts/C2910373807-OB_CLOUD.html);  PACE_OCI_L2_SFREFL [doi:10.5067/PACE/OCI/L2/SFREFL/V1](https://doi.org/10.5067/PACE/OCI/L2/SFREFL/V1)