Trace gases at altitude, measured by moonlight (native format)
What it measures. Vertical profiles of gases and particles high in the atmosphere, including ozone, nitrogen dioxide, and water vapor, for a single observation made using moonlight. Each file covers one lunar event.
How it's made. Produced by the SAGE III instrument on the International Space Station, which watches moonlight pass through the edge of Earth's atmosphere; this is the same data as the HDF5 version but stored in the instrument's native file format.
How & where you'd use it. Supports long-term monitoring of the ozone layer and atmospheric chemistry, feeding into international assessments of ozone depletion.
What's measured
Coverage & cadence
- Time span2017-05-31 → 2024-11-24
- Measured byISS (SAGE III)
- Processing levelLevel 2
- FormatsBinary
- StatusCOMPLETE
What you can do with it
- Map air pollutants — NO₂, aerosols, ozone
- Track greenhouse gases and Earth's energy budget
- Feed weather and air-quality analysis
Official description
g3blspb_53 is the Stratospheric Aerosol and Gas Experiment III (SAGE III) on the International Space Station (ISS) (SAGE III/ISS) Level 2 Lunar Event Species Profiles (Native) V053 data product. It contains all the species products for a single lunar event. Launched on February 19, 2017 on a SpaceX Falcon 9 from Kennedy Space Center, the Stratospheric Aerosol and Gas Experiment III on the International Space Station (SAGE III/ISS), the second instrument from the SAGE III project, is externally mounted on the International Space Station (ISS). This ISS-based instrument uses a technique known as occultation, which involves looking at the light from the Sun or Moon as it passes through Earth’s atmosphere at the edge, or limb, of the planet to provide long-term monitoring of ozone vertical profiles of the stratosphere and mesosphere. The data provided by SAGE III/ISS includes other key components of atmospheric composition and their long-term variability, focusing on the study of aerosols, nitrogen dioxide, nitrogen trioxide, and water vapor. SAGE data has historically been used by the World Meteorological Organization to inform their periodic assessments of ozone depletion. These new observations from the International Space Station will continue the SAGE team's contributions to ongoing scientific understanding of the Earth's atmosphere. Several improvements predominately the ozone, nitrogen dioxide and aerosol products are realized in the version 6.0 data product and cause it to be recommended over version 5.3. These improvements include: filling transmission gaps (caused mainly by sunspots) leading to several hundred more events, additional term in L1 uncertainty, updated ozone absorption cross-section database, more robust covariance computation of aerosol uncertainty. Version 6.0 also has incorporated aerosol flags and particle size distribution information which were previously available in separate files. Further details can be found in the version 6.0 release notes.
Get the data
import earthaccess
earthaccess.login(strategy="netrc") # free Earthdata Login
results = earthaccess.search_data(
short_name="g3blspb",
version="53",
bounding_box=(-122.5, 37.2, -121.8, 37.9), # your area (W,S,E,N)
temporal=("2024-01-01", "2024-12-31"), # your dates
)
files = earthaccess.open(results) # stream straight from LARC_CLOUD Browsing CMR needs no login. Downloading or streaming bytes needs a free Earthdata Login + the earthaccess package. Official links
- NASA Open Source Agreement for Computer Software VIEW RELATED INFORMATION
- SAGE III/ISS Version 5.30 DPUG (Data Product User's Guide) VIEW RELATED INFORMATION
- SAGE III/ISS Version 5.30 Release Notes VIEW RELATED INFORMATION
- Earthdata Search for g3blspb_53 (NASA Application to search, discover, visualize, refine, and access NASA Earth Observation data) GET DATA
- ASDC Direct Data Download for g3blspb_53 GET DATA
- OPeNDAP data access for g3blspb_53 USE SERVICE API
- Virtual Directory for g3blspb_53 GET DATA
- SAGE III Algorithm Theoretical Basis Document (ATBD) Solar and Lunar Algorithm VIEW RELATED INFORMATION