Editing Passive solar building design (section)

==The solar path in passive design==

[[File:Solar altitude.svg|thumb|300px|Solar altitude over a year; latitude based on [[New York City|New York]], [[New York (state)|New York]]]]

{{Main|Sun path|Position of the Sun}}

The ability to achieve these goals simultaneously is fundamentally dependent on the seasonal variations in the sun's path throughout the day.

This occurs as a result of the [[inclination]] of the Earth's axis of rotation in relation to its [[orbit]]. The [[sun path]] is unique for any given latitude.

In Northern Hemisphere non-tropical latitudes farther than 23.5 degrees from the equator:

* The sun will reach its [[noon|highest point]] toward the south (in the direction of the equator)
* As winter [[solstice]] approaches, the [[azimuth|angle]] at which the sun [[sunrise|rises]] and [[sunset|sets]] progressively moves further toward the south and the daylight hours will become shorter
* The opposite is noted in summer where the sun will rise and set further toward the north and the daylight hours will lengthen<ref>{{cite web |url=http://www.srrb.noaa.gov/highlights/sunrise/fig5_40n.gif |access-date=20 April 2023 |website=noaa.gov |title=Solar path image, 40N latitude}}</ref>

The converse is observed in the Southern Hemisphere, but the sun rises to the east and sets toward the west regardless of which hemisphere you are in.

In equatorial regions at less than 23.5 degrees, the position of the sun at [[noon|solar noon]] will oscillate from north to south and back again during the year.<ref>{{cite web |url=http://www.srrb.noaa.gov/highlights/sunrise/fig5_0n.gif |access-date=20 April 2023 |website=noaa.gov |title=Solar path image, 0N latitude}}</ref>

In regions closer than 23.5 degrees from either north-or-south pole, during summer the sun will trace a complete circle in the sky without setting whilst it will never appear above the horizon six months later, during the height of winter.<ref>{{cite web |url=http://www.srrb.noaa.gov/highlights/sunrise/fig5_90n.gif |access-date=20 April 2023 |website=noaa.gov |title=Solar path image, 90N latitude}}</ref>

[[File:Seasonal Insulation Effects of a Pergola.svg|thumb|Seasonal insulation effects of a [[pergola]]]]

The 47-degree difference in the altitude of the sun at [[solar noon]] between winter and summer forms the basis of passive solar design. This information is combined with local climatic data ([[degree day]]) heating and cooling requirements to determine at what time of the year solar gain will be beneficial for [[thermal comfort]], and when it should be blocked with shading. By strategic placement of items such as glazing and shading devices, the percentage of solar gain entering a building can be controlled throughout the year.

One passive solar sun path design problem is that although the sun is in the same relative position six weeks before, and six weeks after, the solstice, due to "thermal lag" from the [[thermal mass]] of the Earth, the temperature and solar gain requirements are quite different before and after the summer or winter solstice. Movable shutters, shades, shade screens, or window quilts can accommodate day-to-day and hour-to-hour solar gain and insulation requirements.

Careful arrangement of rooms completes the passive solar design. A common recommendation for residential dwellings is to place living areas facing solar noon and sleeping quarters on the opposite side.<ref name="autogenerated2">{{cite web|url=http://www.yourhome.gov.au/technical/fs43.html|title=Your Home Technical Manual - 4.3 Orientation - Part 1|date=9 November 2012|archive-url=https://web.archive.org/web/20121109095540/http://www.yourhome.gov.au/technical/fs43.html|archive-date=2012-11-09}}</ref> A [[heliodon]] is a traditional movable light device used by architects and designers to help model sun path effects. In modern times, 3D computer graphics can visually simulate this data, and calculate performance predictions.<ref name="fs110"/>