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Updated: Jun 16, 2026
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Simultaneous Measurement of Turbulence and Particle Kinematics Using Flow Imaging Techniques
Published on: March 12, 2019
Comparison of vertical profile turbulence structure with stellar observations
Applied Optics
|February 4, 2010
Summary
Balloon flights successfully measured microthermal turbulence structure up to 25 km. This data, combined with meteorological and stellar scintillation data, accurately predicted stellar irradiance spectra.
Area of Science:
- Atmospheric physics
- Optical astronomy
Background:
- Understanding atmospheric turbulence is crucial for astronomical observations.
- Microthermal turbulence affects signal propagation.
Purpose of the Study:
- To measure vertical profiles of microthermal turbulence.
- To compare turbulence data with meteorological and scintillation data.
- To predict stellar irradiance spectra using turbulence and wind data.
Main Methods:
- Balloon flights to altitudes near 25 km.
- Acquisition of microthermal turbulence structure data.
- Simultaneous collection of meteorological and stellar scintillation data.
- Computation of integrals over turbulence structure.
- Analysis of turbulence and wind velocity data.
Main Results:
- Successful comparison between observed turbulence structure and meteorological/scintillation data.
- Accurate prediction of stellar irradiance spectra using turbulence and wind velocity data.
Conclusions:
- Vertical turbulence profiles can be accurately measured using balloon flights.
- Measured turbulence data can successfully predict stellar irradiance spectra.
- The study validates theoretical models linking turbulence to optical phenomena.
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