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Based on an expansion with hypergeometric functions, MARINI and MURRAY
[Marini and Murray (1973)] obtained the following integrals for the atmospheric
refraction correction
:
![\begin{displaymath}
\begin{array}{rcl}
\Delta R & = & \frac{1}{\sin(\theta_0)} ...
...r_1} (N(r)N_{Gr}(r) - \frac{1}{2}N(r)^2) dr \right]
\end{array}\end{displaymath}](img2.png) |
(1) |
The phase and group refractive indexes are defined by
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|
|
(2) |
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|
|
(3) |
By expanding the apparent angle of elevation
in terms of the true
angle of elevation
and retaining only the first term, the
third integral in equation 1 is cancelled.
The remaining three integrals were recomputed in order to treat the correction
terms for dry air and water vapour separately and to visualize the physical
constants involved.
![\begin{displaymath}
10^{-6} \int\limits_{r_0}^{\infty} N_{Gr}(h)dh = \frac{1}{g(\phi,H)}\left [ f_{Gr}(\lambda)g_1 + g_3 \right ]
\end{displaymath}](img7.png) |
(4) |
 |
(5) |
where we have defined the following terms:
![\begin{displaymath}
g_1 = 80.343 \times 10^{-6} \left[ \frac{\cal{R}}{M_d \bar{g...
...{M_w}{M_d}\right) \frac{\cal{R}}{4 M_d \bar{g}} P_w(0) \right]
\end{displaymath}](img9.png) |
(6) |
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(7) |
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(8) |
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(9) |
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(10) |
The following table explains the input values:
The refraction correction is now reduced to the simple formula
![\begin{displaymath}
\Delta R = \frac{f_{Gr}(\lambda)}{g(\phi,H)} \left [\frac{g_1 + g_3}{\sin(\theta_w)}+\frac{g_2}{\sin(\theta_w)^3} \right ]
\end{displaymath}](img15.png) |
(11) |
where the dispersion of water vapour was set equal to the dispersion of dry
air. This reduces the validity of equation 11 to
wavelengths in the vincinity of
, since the dispersion function
is normalized to this wavelength.
To ensure a better convergence of equation 11 it
expanded into a continued fraction:
 |
(12) |
The empirical term
was obatined by comparing the reduction formula to
values obtained by raytracing of radiosonde profiles, which served also as
validation of the refduction formula.
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Previous: Introduction
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