20251229 10365800 1.0 TRUE 150000000 5000 ItemDescription AVIRIS-3 dNBR for the Southern California Wildfires January 2025 <div style='text-align:Left;'><div><div>Date of Image(s):Pre-event: 9/5/24Post-event: 1/16/25Summary:The normalized burn ratio difference (dNBR) are generated from the NASA AVIRIS-3 (Airborne Visible/Infrared Imaging Spectrometer -3). They are generated from differencing images from September 5, 2024 (pre-event) and January 16, 2025 (post-event) over Palisades and Eaton. NBR is defined mathematically as (NIR – SWIR)/(NIR + SWIR) where NIR is near-infrared and SWIR is short-wave infrared. dNBR is computed by the difference between the pre-fire NBR and the post-fire NBR. More information on dNBR can be found here: https://un-spider.org/advisory-support/recommended-practices/recommended-practice-burn-severity/in-detail/normalized-burn-ratio.Suggested Usage:NBR is commonly used as a proxy to indicate areas which have charred vegetation. Darker areas (more negative values) in the NBR image more strongly represent the presence of burned vegetation. Since the dNBR considers the condition of the scene before the fire occurred, the resulting value has been used as a proxy for burn severity. Higher dNBR values represent a proxy for greater burn severity. Negative dNBR values may represent a re-greening of or growth of vegetation in between pre and post imagery.The use of this dNBR product as a quantitative metric of burn severity at the time of posting this dataset should be strongly caveated. This is due to several dNBR limitations:<ul><li>The spectral band selections used for dNBR calculations, and the implication of changes observed following fire in those wavelengths, primarily pertain to how vegetation spectral signatures change in NIR and SWIR wavelengths following charring. Because of this, dNBR may not accurately describe burned surfaces that are not vegetation (e.g. human built infrastructure).</li><li>This dataset has not been validated by independent burn severity assessments.</li><li>The degree to which dNBR is accurately determined depends on careful selection of pre and post event imagery. An effort was made to use the highest quality imagery (i.e. cloud free) with representative conditions for each scene; however, it is unknown at the time of this posting how selection of different pre/post image pairs could affect the derived dNBR values.</li></ul>Sensor:Airborne Visible/Infrared Imaging Spectrometer 3rd-Generation (AVIRIS-3)The AVIRIS-3 wavelengths are 866nm and 2198nm.Credits:Rob Green (JPL), Phil Brodrick (JPL), David Thompson (JPL), John Chapman (JPL), Michael Eastwood (JPL), and Adam Chlus (JPL).</div></div></div> Rob Green (JPL), Phil Brodrick (JPL), David Thompson (JPL), John Chapman (JPL), Adam Chlus (JPL), Michael Eastwood (JPL) AVIRIS_DNBR AVIRIS-3 AVIRIS dNBR California Wildfires <div style='text-align:Left;'><div><div>NASA data and products are freely available to federal, state, public, non-profit and commercial users. This information can be experimental- or research-grade data products and may not be appropriate for operational use. These NASA data products, services, and the Disasters Mapping Portal are intended to aid decision makers and enhance situational awareness, but these data are not guaranteed to be consistently available or routinely updated.</div></div></div> 20251229