apparent altitude to observed altitude

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Calculation: The conversion from apparent altitude (Ha) to observed altitude (Ho) of the sun requires correction for atmospheric refraction and compensation for the varying diameters and distances of both the Sun and the Earth throughout the year.

corrections from sextant apparent altitude to observed altitude using images

Sextant Corrections at a Glance:

Page 1: Hs to Ha – THEORY

Page 2: Hs to Ha – CALCULATION

Page 3: Ha to Ho – THEORY

Page 4: Ha to Ho – CALCULATION “ON THIS PAGE”

Moreover, these adjustments collectively result in the final observed altitude, measured from the center of the Earth to the center of the Sun.

This page contributes to the primary objective of offering guidance and interactivity on the calculation and understanding of the Line of Position (LOP) using only a sextant and the sun, and then tracing this line on a plotting sheet. See recommendations.

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Example of calculation apparent altitude to observed altitude (Ha to Ho)

sextant apparent to observed altitude, errors due to external factors and period of the year
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sextant apparent to observed altitude:

Three entries:

1)Ha = 32°14′.5 (Apparent altitude.)

In fact, this apparent altitude was obtained in the blue section (Hs to Ha)

2) Date: Observation somewhere in JULY

3) lower limb of the sun

sextant apparent to observed altitude image upper and lower limb
description lower limb and upper limb

Tables for eye height up to 12 meters and measurement of the Sun’s lower limb only.

In fact, App altitude is about 32°, the observation between is April and September and we took the lower limb → altitude correction = 14′.4

Sextant apparent to observed altitude: solution example

Hs …………………. = _ _° _ _’. _

index error…….. = _ _° _ _’. _

Dip………………… = _ _° _ _’. _

 _________________________ +

Ha………………….. = 32° 14′.5

sun correct LL …= 00° 14′.4

__________________________ +

Ho…………………….= 32° 28′.9

After all necessary corrections, a sextant reading taken on deck provides the geocentric altitude, that is, the angle measured from the Earth’s center to the Sun’s center.

This distinction is important, because the trigonometric formulas used to compute the calculated altitude are likewise derived from the centers of the celestial bodies.

sextant apparent to observed altitude, image observed altitude from center earth

Observed altitude = 32° 29′,0

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