|
|
|
Reasons for
TestingIn the autumn of 2005, Navitron took the decision to
have a range of solar panels tested for
the BS EN 12975 standard. Unfortunately, we were forced to choose a European company
from the 'approved testing house' list. Having spoken to a
number of testing houses, we opted to use SPF in Switzerland, a
Solar Keymark Company, due to their extensive industry
experience, and the level of their professionalism and help in
dealing with our enquiry. The European standard is mainly about
documenting the performance of a panel - hence even flat plate
collectors are able to achieve the standard - although political
decision-makers assume that the standard indicates a 'quality'
product, and therefore it is frequently specified as a
requirement to qualify for certain grants, subsidies or for
inclusion on various 'approved product' lists. Hence our
decision to have our panels tested.
No CE label for solar collectors
The CE mark
normally used as a quality indicator for goods sold in Europe
should not be used for solar hot water systems, as it falls
outside the requirements of the CE standards.
According to the
European
Pressure Equipment Directive (Directive 97/23/EG), solar
collectors for domestic hot water and space heating may not
be labelled with the CE label. Hence, our choice to adopt
the voluntary standard EN BS12975
Weather
Unfortunately, the Swiss climate
does not permit suitable sunlight conditions for testing during
the winter months, so the tests had to be called off until April
at which point solar irradiation levels are sufficient to
continue testing. The tests are exhaustive, and therefore take
some time to complete. Due to the reliance on weather
conditions, it is impossible for SPF to provide an accurate date
for completion of the tests, but we are anticipating that
testing should be complete by mid-summer.
About
SPF
The Institut für
Solartechnik SPF is part of the Hochschule für Technik
Rapperswil HSR. The Institute has been engaged in applied
research and development on thermal solar technology since 1981.
Around 20 members of staff (engineers, physicists and
technicians) are occupied in the following areas:
-
Materials and components (absorber coatings, substrates,
covers, pumps, compensators)
-
Collectors (flat-plate and tubular collectors, liquid
and gaseous heat transfer media, concentrating
configurations)
- Systems
(solar domestic hot water systems, combined systems for
space heating and hot water, solar cooling)
-
Information technology (Software ""Polysun"" to
calculate and optimize collector systems)
SPF is involved
in technology transfer between research and development centres
on the one hand, and trade and industry on the other. In doing
so, SPF acts as a link between users, investors, educational
institutions, manufacturers and installation tradespeople.
- SPF's expertise is officially
confirmed by accreditation (Schweizer Akkreditierungsstelle
(SAS))
- SPF test reports are
recognized internationally without restrictions
- Outdoor testing guarantees
realistic results
- SPF have 25 years of
experience
- All existing standards will be
taken into account if required
- Navitron test results will be
published on SPF's CD-ROM and on their Internet
- Navitron data will be included
in the Polysun collector data base
SPF Performance test
- Measurement of the efficiency
curves with and without wind
- Measurement of the incidence
angle modifier
- Calculation of the thermal
capacity
THE BS EN
TESTING FACILITIES:
Optical Measurements
|
|
Several
instruments are available to determine the various
optical properties that are important in the thermal use
of solar energy. These include an FTIR spectrometer
with integrating spheres and a spectral range from
UV to MIR, an IAM measurement stand to determine
the angle-dependent transmittance and a
spectroradiometer to measure the spectral
radiation.These instruments can be used for many
different measurement tasks. Some measurement procedures
and tests have been standardized, so that the most
relevant materials properties for the thermal use of
solar energy can be determined as inexpensively and
quickly as possible: |
 |
Absorber
The
absorptance and emittance of absorbers is determined on
the basis of a spectral, direct/hemispherical
reflectance measurement. The sample is irradiated with a
parallel ray (Ø 25 mm) with an incidence angle of 10°
relative to the sample normal. The hemispherically
reflected radiation is measured using an integrating
sphere. The solar absorptance is calculated from these
measured data by integration, with the AM1.5 spectrum
(ISO 9845-1) as the weighting spectrum. The thermal
emittance is obtained from weighted integration with the
spectrum of a blackbody at a temperature of 100 °C
(373K). If desired, other weighting functions (for
instance, the blackbody spectrum for another temperature
than 100 °C (373K)) can be used to calculate the
integrated values. Further, the standard measurement
spectral range (0.3 µm - 18 µm) can be extended or
restricted. |
- Spectral measurement
of the specular/hemispherical reflectance in the
range from 0.3 µm to 18 µm.
- Calculation of the
solar absorptance a (AM1.5) (other spectra
possible).
- Calculation of the
emittance e (373K) (other temperatures possible)
|

Fig.2:
Result of an spectral reflection measurement
|
Cover glazing
The
transmittance of a sample is determined with a
direct/hemispherical spectral measurement. The sample is
irradiated with a parallel ray (Ø 25 mm) with an
incidence angle of 10° relative to the sample normal.
The hemispherically transmitted radiation is measured
using an integrating sphere. The solar transmittance is
calculated from these measured data by integration, with
the AM1.5 spectrum (ISO 9845-1) as the weighting
spectrum. The visible transmittance is obtained from
weighted integration with the product of the radiation
function for the standard light source D65 and the
photopic spectral response of the human eye (DIN 67
607). If desired, other weighting functions can be used
to calculate the integrated values. Further, the
standard measurement spectral range (0.29 µm - 2.5 µm)
can be extended or restricted. The latter can be an
interesting option, if measurements in the UV and or NIR
are not required. |
- Spectral measurement
of the direct/hemispherical transmittance in the
range from 0.29 µm to 2.5 µm.
- Calculation of the
solar transmittance t(AM1.5). (other spectra
possible)
- Calculation of the
visible transmittance t(D65). (other spectra
possible)
- Sample dimensions at
least 5 cm x 5 cm.
|
Fig.3:
Result of an spectral transmission measurement
|
Incident angle modifier
The sun is
not always located perpendicular to the collector plane;
the incidence angle generally changes both during the
course of a day and throughout the year. The
transmittance of the cover glazing for the collector
changes with the incidence angle. The relationship
between the incident angle and the transmittance can be
calculated for materials with smooth surfaces.However,
usually at least one surface of the cover used for a
solar collector is structured, which means that the
angle-dependent transmittance can no longer be easily
calculated. For this reason, we have set up a special
test stand to determine this quantity.To be precise, the
angle-dependent transmittance is not determined
absolutely with this test stand, but its variation with
respect to that at normal incidence. This is the
definition of the incident angle modifier (IAM) for
transmittance. However, an additional transmittance
measurement for normally incident radiation can be made.
From the measurement technology, this does not achieve
the same absolute accuracy as a measurement with the
Fourier spectrometer (see above), but it is usually
adequate for comparison purposes. |
- Determination of the IAM in the range
between 30° and 70° in 10° steps (measurement
geometry depending on the sample)
- Spectral measurement
of the direct/hemispherical transmittance in the
range from 0.3 µm to 1.7 µm and calculation of the
transmittance (basic glazing package II)
- Sample size up to
collector dimensions.
|

Fig.4:
Result of an incident angle modifier measurement |
Durability
of Materials for Solar Systems
|
Absorber coatings
The optical
properties of the selective coating are decisive in
determining the efficiency of the collector and thus the
system yield. These should not decrease with time due to
degradation of the absorber coating. In order to
guarantee this, in principle a newly developed absorber
coating would have to withstand 25 years of use without
damage, before marketing could begin. Clearly, this
condition cannot be met. Thus, we have co-operated
internationally with other institutes to establish a
method which allows the aging performance of such
coatings to be determined in the laboratory within a
short time. |

Fig.1:
Condensation test of new absorbers |

Fig.2: Test of the fin - tube bond |
Climatic chambers
Many
materials tests demand that the testing climate be
accurately specified and controlled. To achieve this, we
use climatic chambers, in which the air humidity and
temperature can be exactly controlled within wide
ranges. In addition, the sample can be subjected to
simulated solar radiation or UV-enhanced radiation. A
precisely controlled, circulating-air oven can be used
for higher temperatures. If the surrounding atmosphere
is disturbing, the high temperatures can also be applied
under vacuum. |
|