Raw calibrated light spectra used to find CO2 (OCO-2)
What it measures. Calibrated light spectra, that is, how much near-infrared sunlight and oxygen-band light the instrument recorded, with precise location stamped on every measurement.
How it's made. Produced by NASA's OCO-2 satellite, which uses three spectrometers; this is the Level-1B stage that turns the raw instrument counts into calibrated light readings.
How & where you'd use it. A building-block input used to work out atmospheric carbon dioxide in higher-level products; most people use those CO2 results rather than these raw spectra directly.
What's measured
Coverage & cadence
- Time span2019-11-30 → ongoing
- Measured byOCO-2 (OCO-2)
- Processing levelLevel 1B
- Spatial extent-180, -90, 180, 90
- StatusACTIVE
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
Version 11.2r is the current version of the data set. Older versions will no longer be available and are superseded by Version 11.2r. The Orbiting Carbon Observatory is the first NASA mission designed to collect space-based measurements of atmospheric carbon dioxide with the precision, resolution, and coverage needed to characterize the processes controlling its buildup in the atmosphere. The OCO-2 project uses the LEOStar-2 spacecraft that carries a single instrument. It incorporates three high-resolution spectrometers that make coincident measurements of reflected sunlight in the near-infrared CO2 near 1.61 and 2.06 micrometers and in molecular oxygen (O2) A-Band at 0.76 micrometers. The three spectrometers have different characteristics and are calibrated independently. Their raw data numbers (DN) are delivered correlated in time to the Level 1B process as Level 1A products. Each band has 1016 spectral elements, although some are masked out in the L2 retrieval.This product is the output from the Level 1B process. It converts the raw instrument data numbers into calibrated radiances. This conversion is based upon files of instrument characteristics and algorithm parameters that may vary over time. In addition to calibrated radiances, the Level 1B output products have geolocation information recorded for each measurement for use in higher-level processes.
Get the data
import earthaccess
earthaccess.login(strategy="netrc") # free Earthdata Login
results = earthaccess.search_data(
short_name="OCO2_L1B_Science",
version="11.2r",
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 GES_DISC Browsing CMR needs no login. Downloading or streaming bytes needs a free Earthdata Login + the earthaccess package. Official links
- Use the Earthdata Search to find and retrieve data sets across multiple data centers. GET DATA
- Access the data via the OPeNDAP protocol. USE SERVICE API
- Access the data via HTTP. GET DATA
- Level 1B Algorithm Theoretical Basis (ATBD) VIEW RELATED INFORMATION
- README document. VIEW RELATED INFORMATION
- Data Quality document VIEW RELATED INFORMATION
- Subset recipe using OPeNDAP VIEW RELATED INFORMATION
- Level 1B Software Interface Specification containing description of all data objects in data files VIEW RELATED INFORMATION