Correlation between the phase and the log-amplitude of a wave through the vertical atmospheric propagation

Abstract

Expressions of the correlation between the log-amplitude and the phase of a wavefront propagating through the atmospheric turbulence are presented. These expressions are useful to evaluate the feasibility of proposed methods to increase the confidence level of the detection of faint transient astronomical objects. The properties of the derived angular correlation functions are discussed using usual synthetic turbulence profiles. The close formulation between the phase and the log-amplitude allows an analytic formulation in the Rytov approximation. Equations contain the product of an arbitrary number of hypergeometric functions that are evaluated using the Mellin transforms integration method.

23 pages, 5 figures, version 2, accepted to JOSAA

References in corpus (3)

• Measuring the Abundance of sub-kilometer sized Kuiper Belt Objects using Stellar Occultations
• Transformation of Zernike coefficients: A Fourier based method for scaled, translated and rotated wavefront apertures
• The Multiplexed Imaging Method: High-Resolution Wide Field Imaging Using Physically Small Detectors