Global radiation has its maximum in the direction of the
respective position of the sun. Solar energy use in its simplest
form is thus based on the optimal exposure of those surfaces
foreseen or oriented for use in energy conversion, as well as
their freedom from shadow.
The VDI-GUIDELINE 3789, Sheet 2 (1994) contains the
foundations and significant working aids for the calculation of
radiation.
Exposure
The orientation of surfaces according to direction and angle
of inclination leads to various amounts of absorbed radiation.
Daily and yearly variations in the position of the sun must also
be taken into account. (In fact, the noontime solar zenith
varies by 47 degrees between the summer and winter solstices.)
Maximum solar radiation thus shifts to more southerly oriented
surfaces during winter because of the lower position of the sun.
A simple aid for the assessment of surface orientation in
regards to usage of the annual solar radiation is depicted in Figure
3/6 from BIASIN and DIETRICH (1992).
This diagram assumes an average annual radiation of 982 kWh/m2
on a horizontal surface. In the case of a southerly-oriented
surface angled at 30°, a maximum annual radiation of 1,055
kWh/m2 is possible.
In relation to this 100% theoretical maximum value, all other
orientations in direction and angles of incline yield lower
potential radiation values. When one considers the case of a
building wall (angle of inclination 90°), one can ascertain a
comparatively small change for orientations in the semi-circle
from east through south to west in relation to the decreasing
solar elevations in the east and west. That is, the annual solar
radiation remains in the area of 60% to 68% of the maximum value.
Admittedly, this denotes a much smaller amount of radiation than
in the case of a horizontal surface, which is shown at 93% in
the radiation diagram. Only the exposure area contained by the
93% curve signifies a radiation efficiency exceeding that of a
horizontal surface.
The importance of vertical walls requires a differentiated
consideration of the data for walls: Figures 3/7 and
Figures 3/8
depict annual variations in global radiation (including for
northerly wall orientations), distinguishing between average
conditions (Figure 3/7) and almost cloudless days (Figure 3/8).
Figures 3/7
and
Figures 3/8
lead to the following summarizing
conclusions in relation to vertical exterior surfaces (walls):
Greater global radiation on nearly cloudless days implies
lesser proportions of diffuse celestial radiation. The latter’s
proportion on sunny days amounts to between 27% (in the case of
a south wall) and 81% (north wall). On average (that is, under
consideration of average cloud conditions), however, the
comparable values for the proportion of diffuse radiation are
51% (south wall) and 94% (north wall).
The proportion of diffuse radiation under average conditions
produces a certain equalization in global radiation at various
orientations. The global radiation for east and west walls
amounts on average (Figures 3/7) to 81% of that of the
respective south wall, or only 73% on sunny days. The comparison
values for the relationship of north wall to south wall amount
to 48% on average, or 26% on sunny days.
During the months of June, July, and August, westerly and
easterly oriented walls provide larger daily totals of global
radiation than the south wall. This is especially true on sunny
days with correspondingly large proportions of direct sunlight.
The energy-related advantage of a southerly orientation comes
into play during the heating season. Above all during the months
of November, December, and January, southward-facing surfaces
show considerable deficits in radiation. In relation to the
heating season, northern walls prove significantly less
efficient in comparison to the year-round average.
A further point pertains to the southerly orientation of
building walls as well as large window surfaces: The environment
of the city with its close proximity of structures produces an
artificial heightening of the horizon at low positions of the
sun (mornings and evenings, especially in winter months), which
results in later sunrises and earlier sunsets. Thus there exists
a greater chance of freedom from shading for the southern sky,
which provides additional importance to southward-facing
surfaces. An orientation of building windows exclusively towards
the south reduces energy use by about 10%.
The positive effect of a southerly orientation for individual
rooms depends strongly on the proportion of window surface and
the quality of the window materials. A more completely described
model space in DUETZ and MAERTIN (1982) yielded the following
conditions for the annual hours of full use of the heating
system in the presence of double-glazed windows and a 50%
proportion of window surfaces dependent on the orientation:
North: 100%, South: 83%, West: 94%, East: 93%,
Shading
Shading signifies a reduction in the astronomically possible
sunlight through heightening of the horizon, e.g. from mountains
or surrounding buildings. Primarily in the case of valleys and
northerly-exposed surfaces, but also in areas of dense urban
development, restrictions arise in the duration of sunshine.
Due to shading at low positions of the sun, northerly slopes
with inclines up to 10° receive 10% to 30% less global
radiation in winter than southerly-oriented faces. Development
on northerly slopes should thus be avoided as much as possible,
since these microclimatic disadvantages can only be
insufficiently compensated through other built measures (DUETZ
and MAERTIN, 1982).
Helpful for the
planning are calculated solar maps which illustrate these
relations. The figure
3/9a shows the direct sun radiation as a annual mean for
the area of Stuttgart. In the figure
3/9b the global radiation is illustrated. The great
differences in radiation in dependence of the different
slopes can be seen clearly.
Figure 3/9 reproduces the result of a computer model showing
the distribution of solar energy for an area of development
planned on a slope facing west to southwest (GORETZKI, 1990).
Although at first glance one would expect good conditions for
passive solar energy use because of the ideal exposure, the
simulation shows a reduction up to 30% in radiation owing to the
slope shading (as a consequence of the topography).
With the help of the polar coordinate diagram in Figure
3/10, the astronomically possible duration of sunshine for a
location and its limitations due to horizon heightening and
shading can be calculated from the various sun curves for
particular times of the year. The diagram is strictly valid for
the coordinates 49° 46" N, 9° 11" E, and thus in
this form can be used with sufficient accuracy in the state of
Baden-Württemberg. At this geographic latitude, the extreme
values of the sun’s position at 12:00 local time (not Central
European Time!) are:
64.5° (June 21, Summer Solstice)
17.6° (December 21, Winter Solstice)
The position of the sun for other dates and times can also be
read from Figure
3/10.
Solar tracks for other locations and arbitrary dates can be
requested at the internet address:
http://www.stadtklima-stuttgart.de/index.php?klima_sonnenstand
The dashed lines give the time in Central European Time. The
concentric circles are supplied with a scale in degrees for the
elevation of the sun. The respective position of the sun is
calculated from the intersection of a crosswise date curve with
an upright time curve. At the intersection, one can read the
angle of the solar elevation (concentric circles) as well as the
solar azimuth (direction towards the sun in the sky), the latter
of which comes from connecting the intersection with the middle
point of the diagram and reading the resultant direction from
the compass.
If one inserts into such a diagram a picture of the local
topography or built environment from the perspective of a
location to be examined, the portion of the solar track not
obscured by heightening of the horizon shows the remaining
potential for sunlight. Thereby the shading produced by existing
or planned buildings in the southern part of the hemisphere can
be assessed. This method is described in detail in TONNE (1954)
(compare with Chapter 3.2.3).
The picture must be inserted into the diagram in a polar
projection, similar to the reflected image on a mirrored
half-sphere at the level of the horizon. The middle point of the
diagram corresponds to the zenith, from which all vertical
building lines emanate. The outer circle of the diagram
corresponds to the horizon. Spatial lines running parallel to
the horizon and horizontal building lines are transposed to
concentric circles relative to their height.
It must be kept in mind
that the roof edge of a long, straight building appears to the
viewer at large side angles to have a smaller angle of height,
so that the building picture cuts the concentric circles in
accordance with the variation of the elevation angle.