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