Skip to content

To bring about breakthroughs in international space research

  • Home
  • Onderzoeksvragen
  • Pijlers
  • Missies
  • Over ons
  • Contact
Home
    Home

    SRON | Wetenschappelijk ruimteonderzoek Nederland

    To bring about breakthroughs in international space research

    Home
    • Onderzoeksvragen
    • Pijlers
      • Wetenschap
      • Technologie
      • Instrumentatie
      • Onze mensen
      • Impact
    • Missies
    • Over ons
    • Actueel
    • Contact
    • SRON Academy
    • Werken bij
    • Bezoek aan SRON
    Home
      • Onderzoeksvragen
        • Hoe ontrafelen we de fysica achter zwarte gaten?
        • Hoe kunnen we de zwakste exoplaneten waarnemen?
        • Waar worden broeikasgassen uitgestoten?
        • Hoe speciaal is de aarde in de context van het heelal?
        • Hoe ontstaan en groeien zwarte gaten?
        • Hoe beïnvloeden aerosolen het klimaat?
        • Hoe ontstaan sterren en planeten?
        • Hoe beïnvloedt klimaatverandering het leven op aarde?
      • Pijlers
        • Wetenschap
          • Aardobservatie
            • Methaan
            • Aerosolen en Wolken
            • CO2
            • Koolmonoxide
          • Astrofysica
            • Lage energie
            • Hoge energie
            • Exoplaneten
        • Technologie
        • Instrumentatie
          • Nanotechnologie
          • Cryogenica
          • Optica
          • Electronica
          • PA/QA kwaliteit
          • Mechanica / Realisatie
        • Onze mensen
        • Impact
      • Missies
        • Actief
          • ALMA
          • GUSTO
          • PACE
          • Sentinel-5p
          • SPEX airborne
          • XRISM
        • In ontwikkeling
          • ARIEL
          • LISA
          • Metop-SG A
        • Legacy
          • BeppoSAX
          • STO2
      • Over ons
        • Faciliteiten
        • Geschiedenis
      • Actueel
      • Contact
      • SRON Academy
      • Werken bij
      • Bezoek aan SRON
      • Privacy policy
      01/09/2017

      Global fire emissions estimates during 1997-2016

      Climate, land use, and other anthropogenic and natural drivers have the potential to influence fire dynamics in many regions. To develop a mechanistic understanding of the changing role of these drivers and their impact on atmospheric composition, long-term fire records are needed that fuse information from different satellite and in situ data streams. Here we describe the fourth version of the Global Fire Emissions Database (GFED) and quantify global fire emissions patterns during 1997-2016. The modeling system, based on the Carnegie-Ames-Stanford Approach (CASA) biogeochemical model, has several modifications from the previous version and uses higher quality input datasets. Significant upgrades include (1) new burned area estimates with contributions from small fires, (2) a revised fuel consumption parameterization optimized using field observations, (3) modifications that improve the representation of fuel consumption in frequently burning landscapes, and (4) fire severity estimates that better represent continental differences in burning processes across boreal regions of North America and Eurasia. The new version has a higher spatial resolution (0.25°) and uses a different set of emission factors that separately resolves trace gas and aerosol emissions from temperate and boreal forest ecosystems. Global mean carbon emissions using the burned area dataset with small fires (GFED4s) were 2.2 × 1015 grams of carbon per year (Pg C yr-1) during 1997-2016, with a maximum in 1997 (3.0 Pg C yr-1) and minimum in 2013 (1.8 Pg C yr-1). These estimates were 11 % higher than our previous estimates (GFED3) during 1997-2011, when the two datasets overlapped. This net increase was the result of a substantial increase in burned area (37 %), mostly due to the inclusion of small fires, and a modest decrease in mean fuel consumption (-19 %) to better match estimates from field studies, primarily in savannas and grasslands. For trace gas and aerosol emissions, differences between GFED4s and GFED3 were often larger due to the use of revised emission factors. If small fire burned area was excluded (GFED4 without the <q>s</q> for small fires), average emissions were 1.5 Pg C yr-1. The addition of small fires had the largest impact on emissions in temperate North America, Central America, Europe, and temperate Asia. This small fire layer carries substantial uncertainties; improving these estimates will require use of new burned area products derived from high-resolution satellite imagery. Our revised dataset provides an internally consistent set of burned area and emissions that may contribute to a better understanding of multi-decadal changes in fire dynamics and their impact on the Earth system. GFED data are available from <a href=”http://www.globalfiredata.org” title=”” class=”ref”>http://www.globalfiredata.org</a>.

      SRON Leiden

      Leiden

      Niels Bohrweg 4
      2333 CA Leiden
      The Netherlands
      +31 (0)88 777 56 00

      SRON Groningen

      Groningen

      Landleven 12
      9747 AD Groningen
      The Netherlands
      +31 (0)50 363 40 74

      • Onderzoeksvragen
      • Pijlers
        • Wetenschap
        • Technologie
        • Instrumentatie
        • Onze mensen
        • Impact
      • Missies
      • Over ons
      • Actueel
      • Contact
      SRON on bluesky SRON on Instagram SRON on LinkedIn

      Niels Bohrweg 4
      2333 CA Leiden
      The Netherlands
      +31 (0)88 777 56 00

      Landleven 12
      9747 AD Groningen
      The Netherlands
      +31 (0)50 363 40 74

      NWO-I

      SRON is onderdeel van de institutenorganisatie van NWO-I

      • Privacy policy
      Home

      What happens up there, starts down here.