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Analysis Code for High Altitude Balloons - FedOA - Università degli ...

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ACHAB: <strong>Analysis</strong> <strong>Code</strong> <strong>for</strong> <strong>High</strong> <strong>Altitude</strong> <strong>Balloons</strong> Chapter 3<br />

• Compute Local Hour Angle ( LHA ).<br />

The Local Hour Angle is then:<br />

LHA = θ −<br />

• Convert Local Hour Angle and declination to horizon coordinates.<br />

Now it is possible to compute the local solar elevation angle (ELV) and<br />

RA<br />

azimuth angle using the following relationships:<br />

( Lat)<br />

sinδ<br />

+ cos(<br />

Lat)<br />

cos ( LHA)<br />

sin ELV = sin<br />

δ cos<br />

tan AZ = −<br />

cos<br />

where Lat is the balloon actual latitude.<br />

sin(<br />

LHA)<br />

( Lat)<br />

tanδ<br />

− sin(<br />

Lat)<br />

cos(<br />

LHA)<br />

Using this algorithm it is possible to simulate the day and night cycle.<br />

Twilight.<br />

Be<strong>for</strong>e sunrise and again after sunset there are time intervals during which there is<br />

natural light provided by the upper atmosphere, which does receive direct sunlight<br />

and reflects part of it toward the Earth's surface. This kind of illumination is referred<br />

to as twilight.<br />

There are several definitions <strong>for</strong> twilight according to application. The present model<br />

considers civil twilight, which is defined to begin (in the morning), and to end (in the<br />

evening) when the center of the Sun is geometrically 6 degrees below the horizon 31 .<br />

3.2.3.2 – Atmospheric Transmissivity<br />

Irradiance of both the solar radiation and the longwave radiation is obviously<br />

influenced by the presence of the atmosphere. The transmissivity of a solar beam and<br />

the attenuation of the ground thermal radiation, follow an exponential decay 9 based<br />

on Beer’s Law. All of the following equations are based on those from Ref. 9 and<br />

Ref. 20.<br />

33

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