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Radiative flux measurements in the troposphere
F P Valero1, W J Gore, L P Giver
1NASA, Ames Research Center, Moffett Field, California 94035, USA.
Applied Optics
|April 8, 2010
Summary
Accurate atmospheric radiative flux measurements were made using a specialized aircraft radiometer. This study quantifies heating rates in hazy and foggy conditions, validating the instrument by calculating the solar constant.
Area of Science:
- Atmospheric Science
- Radiative Transfer
- Aerosol Science
Background:
- Accurate measurement of radiative flux density in the troposphere is crucial for understanding atmospheric processes.
- Previous methods may have limitations in precision and scope.
Purpose of the Study:
- To report results from radiative flux-density measurements in the troposphere using a novel aircraft-mounted radiometer.
- To calculate heating rates for atmospheric gases and aerosols.
- To verify instrument performance by determining the solar constant.
Main Methods:
- Utilized a specially designed radiometer mounted on a Cessna 402B aircraft for in-situ measurements.
- Calculated atmospheric heating rates using measured radiative flux densities and radiosonde data.
- Verified instrument accuracy by calculating the solar constant from tropospheric flux density data.
Main Results:
- Determined total atmospheric heating rates of 0.175 K h⁻¹ for hazy and 0.377 K h⁻¹ for foggy conditions.
- Deduced aerosol heating rates of 0.065 K h⁻¹ (hazy) and 0.235 K h⁻¹ (foggy).
- Derived a solar constant of 1387 ± 21 W m⁻², agreeing within 4% of the standard value.
Conclusions:
- The specialized radiometer provides highly accurate atmospheric radiative flux determinations.
- The study quantifies significant aerosol contributions to atmospheric heating.
- Instrument performance is validated, demonstrating its capability for precise solar constant calculation.
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