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HALO 2020 – Cloud effects on solar actinic radiation: Evaluation of satellite-aided radiative transfer model calculations with HALO measurements

HALO 2020 – Cloud effects on solar actinic radiation: Evaluation of satellite-aided radiative transfer model calculations with HALO measurements
HALO 2020 â 云对太阳光化辐射的影响:利用 HALO 测量评估卫星辅助辐射传输模型计算
批准号:
442647232
负责人:
Dr. Birger Bohn
金额:
$0.0万
依托单位:
依托单位国家:
德国
项目类别:
Infrastructure Priority Programmes
财政年份:
--
资助国家:
德国
项目状态:
未结题
起止时间:

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中文摘要
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英文摘要
In this project UV/VIS spectral actinic flux density measurements of six HALO missions will be used for an evaluation of radiative transfer model calculations based on operational satellite cloud retrievals. Five of the HALO missions have already been completed: TECHNO (2010), NARVAL-I (2014), OMO (2015), EMERGE (2017/2018), and CAFE-Africa (2018) with a total of around 75 research flights. In addition, data of CAFE-Brazil (2020) will be included. The main purpose of the spectral actinic flux density measurements is to derive photolysis frequencies that are important for photochemical research. The HALO measurements provide a rare opportunity for an evaluation of satellite derived photolysis frequencies because they provide high resolution spot samples that cover different altitudes and mission areas globally. Moreover, during TECHNO, NARVAL and OMO also nadir spectral radiance measurements were performed on HALO by a mission partner. These measurements cover the complete solar spectral range and provide independent, local information on cloud properties below the aircraft. That will help to interpret and correctly apply the satellite data. The main question addressed in this project is whether or not radiative transfer modelled and measured data can be brought into reasonable agreement by taking into account available satellite cloud information and if consistent results are obtained for different mission areas and altitude ranges. If this approach is successful, predictions of evaluated, user-defined 3D fields of photolysis frequencies and their error estimates can be produced based on satellite cloud information. These photolysis frequency fields can be used to test chemistry transport model predictions or they can serve directly as an input for such models in future studies. A corresponding case study is intended within this project. From these applications also future HALO missions and their scientific analyses could benefit.
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Solar Radiation Measurements on HALO
  • 批准号:
    178612691
  • 项目类别:
    Infrastructure Priority Programmes
  • 资助金额:
    $0.0万
  • 财政年份:
    2010
  • 负责人:
    Dr. Birger Bohn
  • 依托单位:
ATMOCHEM - Novel Approaches in the Understanding of Aromatic Compound Degradation in the Atmosphere: From Theoretical Studies to Simulation Chamber Experiments
  • 批准号:
    83127611
  • 项目类别:
    Research Grants
  • 资助金额:
    $0.0万
  • 财政年份:
    2008
  • 负责人:
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  • 资助金额:
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  • 批准年份:
    2025
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    2024
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  • 项目类别:
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  • 资助金额:
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  • 批准年份:
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  • 负责人:
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