(ALLEGEDLY
SPHEROIDAL)
EARTH
CURVATURE
EQUATION
W/ ELEVATED
OBSERVER
Introduction to the (Allegedly Spheroidal) Earth Curvature Equation w/ Elevated Observer
On the (allegedly spheroidal) surface of the earth (see Figure 1), note the mean sea level (MSL) geographic position P_1(φ_1,λ_1) of an observer or detector (henceforth referred to as P_1), where the Greek letters φ (phi) and λ (lambda) refer to the position’s latitude and longitude respectively. But whereas the observer or detector is at some elevation or orthometric height (H_1)1 above MSL, then note also the orthographic height position P_1(φ_1,λ_1, H_1) of the observer or detector, henceforth referred to as P_1(H_1). In relation to position P_1(H_1), consider a distant subject at (MSL) geographic position P_2(φ_2,λ_2), henceforth referred to as P_2. The (alleged) distance d_n is represented by the line from P_2 below and normal to the observer or detector’s horizon line of sight, i.e., the ray fom the observer or detector that is tangent to the observer or detector’s horizon and coplanar with P_2, said line intersecting said ray at point α. The curvature equation w/ elevated observer — in terms of the extent to which P_2 is (allegedly) hidden from P_1(H_1) by the (alleged) curvature of the earth — is essentially the equation for determining the (alleged) magnitude of d_n.
From Figure 1, it is obvious that for a given distance between the observer or detector and the subject of observation or detection, the magnitude of d_n decreases with increasing orthometric height H_1.
Figure 1. Analysis of the curvature (w/ elevated observer) of the (allegedly spheroidal) earth.
The (Alleged) Linear (i.e., Line of Sight) Distance d_h to the (Allegedly Spheroidal) Earth Horizon
In Figure 1, angle \displaystyle{(∠)}\,\displaystyle{P_1(H_1)P_{horizon}O} is a right angle \displaystyle{(∟)} since line segment P_1(H_1)P_{horizon} (the magnitude of which is represented by d_h) is tangent to radial line OP_{horizon}. Hence, triangle \displaystyle{(Δ)}\,P_1(H_1)P_{horizon}O is a right triangle \displaystyle{(◿)}.
Therefore, by Pythagoras’ theorem,
[P_1(H_1)P_{horizon}]^2+[OP_{horizon}]^2
=[OP_1(H_1)]^2,
and hence,
P_1(H_1)P_{horizon}=
\sqrt{[OP_1(H_1)]^2-[OP_{horizon}]^2}.
Whereas from Figure 1, P_1(H_1)P_{horizon}=d_h, OP_1(H_1)=R_1+H_1, and OP_{horizon}=R_1, where R_1 is the (alleged) mean radius of the (allegedly spheroidal) earth, then
d_h=\sqrt{(R_1+H_1)^2-R_1^2},
and hence,
d_h=\sqrt{2R_1H_1+H_1^2}.
The (Alleged and Allegedly) Curvilinear (i.e., Surface) Distance s_h to the (Allegedly Spheroidal) Earth Horizon
It is well known that arc length is equal to the radius times the angle (in radians) subtended by the arc. Hence, from Figure 1,
s_h=R_1𝜓,
where 𝜓=\displaystyle{∠}\,\displaystyle{P_1(H_1)OP_{horizon}}.
Whereas (from above) triangle \displaystyle{(Δ)}\,P_1(H_1)P_{horizon}O is a right triangle \displaystyle{(◿)}, then
\textrm{cos}\,𝜓=\left(\frac{R_1}{R_1+H_1}\right).
Hence,s_{h}=
R_1 \bigg\{{\left[\textrm{cos}\,^{-1}\left(\frac{R_1}{R_1+H_1}\right)\right]\textrm{rad}\bigg\}}.
Note:The respective magnitudes of d_h and s_h are almost the same for the elevations or altitudes considered in the debate over the large-scale structure of the earth’s surface. Hence, on the web pages under the CALCULATORS folder, the calculated values for d_h and s_h are expressed to eight decimal places to indicate the minor but actual differences in their respective magnitudes.
Derivation of the (Allegedly Spheroidal) Earth Curvature Equation W/ Elevated Observer
To repeat the concluding statement from the Introduction above: “From Figure 1, it is obvious that for a given distance between the observer or detector [i.e., P_1(φ_1,λ_1, H_1)] or simply P_1(H_1)] and the subject of observation or detection [i.e., P_2(φ_2,λ_2) or simply P_2], the magnitude of d_n decreases with increasing orthometric height H_1.” In other words, the greater the observer or detector’s orthometric height H_1, the closer the observer or detector’s horizon point (P_{horizon}) is to the subject of observation or detection (P_2). Whereas the observer or detector at P_1(H_1) has a direct line of sight to the observer or detector’s horizon point (P_{horizon}), the effective amount of (alleged) curvature of the (allegedly spheroidal) earth between the observer or detector and the subject of observation or detection is therefore represented by the (allegedly curvilinear) distance or arc (⌒) s-s_h, i.e., arc (⌒) P_{horizon}P_2.
The (alleged) distance d_n is proportional to the amount of (alleged) curvature of the (allegedly spheroidal) earth between the observer or detector’s horizon point (P_{horizon}) and the subject of observation or detection as represented by the (allegedly curvilinear) distance arc (⌒) s-s_h, i.e., arc (⌒) P_{horizon}P_2. Expressed in terms of angular measurement — for this derivation, radians (rad) — the amount of curvature (on any spheroid) is directionally dependent and inversely proportional to a function of its three semi-axes; in the case of the (allegedly spheroidal) earth, the amount of curvature is inversely proportional to R_1, where R_1 is the (alleged) mean radius of the earth, specifically, the (alleged) Mean Radius of the Three Semi-axes of the (allegedly spheroidal) earth.2 Hence, the (allegedly curvilinear) distance s-s_h subtends the angle θ-𝜓, the magnitude of which is,
θ-𝜓=\frac{s-s_h}{R_1}\textrm{rad}.
Referring again to Figure 1, if O is the center of the (allegedly) spheroidal earth, and P_1(H_1) is (again) the orthometric height position of the observer or detector — at a distance R_1+H_1 from O, whereby R_1 is represented by lines OP_1 and OP_{horizon}, and if P_2 is again the position of the subject of observation or detection, whereby R_1 is also represented by line OP_2, then the angle (\scriptstyle{∠}) θ-𝜓 subtended by ⌒s-s_h, i.e., ⌒P_{horizon}P_2, can also be expresed as, θ-𝜓=\;\scriptstyle{∠}\,\displaystyle{P_{horizon}OP_2.}
Hence,
\;\scriptstyle{∠}\,\displaystyle{P_{horizon}OP_2=\frac{s-s_h}{R_1}\textrm{rad}.}
Referring once again to Figure 1, and as indicated previously, α is the intersection of the line from the subject’s position P_2 with (and normal to) the observer or detector’s horizon line of sight. Hence, the two components of ⌒P_{horizon}P_2 are represented by line P_{horizon}α (collinear with the observer or detector’s horizon line of sight) and line P_2α (normal to the observer or detector’s horizon line of sight). In rectangle (▭) P_{horizon}αP_2β, the line from the subject’s position P_2 with (and perpendicular to) line OP_{horizon} intersects line OP_{horizon} at β, lines P_{horizon}β and P_2β being equal and parallel to (⋕) lines P_2α and P_{horizon}α respectively; hence, triangle P_2βO is a right triangle (◿).
In ◿P_2βO,
\textrm{cos}\,\scriptstyle{∠}\,\displaystyle βOP_2\,\textrm{[or cos}\,(θ-𝜓)]=
\dfrac{Oβ}{OP_2}\,\left(\textrm{or}\;\dfrac{Oβ}{R_1}\right).
Hence,
R_1=\frac{Oβ}{\textrm{cos}\,(θ-𝜓)},
and therefore,
Oβ=R_1\textrm{cos}\,(θ-𝜓).
But R_1 is also equal to OP_{horizon}\,\textrm{(or}\,Oβ+P_{horizon}β), and whereas P_{horizon}β⋕P_2α\,\textrm{(or}\,d_n), then d_n=R_1-Oβ.
Hence,
d_n=R_1-R_1\textrm{cos}\,(θ-𝜓),
or,
d_n=R_1[(1-\textrm{cos}\,(θ-𝜓)].
And whereas,
θ=\frac{s}{R_1}\textrm{rad},
and
𝜓=\textrm{cos}^{-1}\left(\frac{R_1}{R_1+H_1}\right)\textrm{rad},
then, for an observer or detector at orthographic height position P_1(H_1), the curvature equation in terms of the distance d_n from P_2 normal to the observer or detector’s horizon line of sight, is:
d_{n}=
R_1\bigg\{{1- \textrm{cos}\,\left[\left(\frac{s}{R_1}\textrm{rad}\right)-\\\textrm{cos}\,^{-1}\left(\frac{R_1}{R_1+H_1}\right)\textrm{rad}\,\right]\bigg\}.}
— FINIS —
The curvature equation w/ elevated observer is further developed to include the orthometric height of the subject of observation or detection on our web page titled, (Allegedly Spheroidal) Earth Curvature Equation W/ Elevated Observer and Subject.
For a description of orthometric (or geoidal) height, see our web page titled, (Allegedly Spheroidal) Earth Mensuration.↩️
See our web page titled, (Allegedly Spheroidal) Earth Mensuration.↩️
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REVISION | 0 | 1 |
DATE | 2022-JUN-06 | 2023-NOV-09 |