DR20 Class A Pyrheliometer

DR20-A1 is a high-accuracy direct (normal incidence) solar radiation sensor, or pyrheliometer. DR20 pyrheliometer complies with the Class A specifications of the ISO 9060 standard. It has a better temperature response than DR15-A1, which is a spectrally flat Class B pyrheliometer. These instruments are used in tracker-mounted operation, and offer analogue millivolt outputs. DR-series pyrheliometers have superior window heating that leads to high data availability.

  • ISO 9060 spectrally flat Class A
  • Heating at low offsets for high data availability
  • Low power consumption
  • Analogue millivolt output
  • Supplied with test report for the individual instrument, including temperature response

Description

Specifications

Measurand Direct solar radiation
ISO classification Spectrally flat Class A
Calibration uncertainty < 1.2 % (k = 2)
Heating Included
Heater 1 W at 12 VDC
Response time (95 %) 4 s
Full field of view angle 5 °
Slope angle 1 °
Zero offset < ± 1 W/m²
Calibration traceability to WRR
Spectral range 200 to 4000 x 10⁻⁹ m
Rated operating temperature range -40 to +80 °C
Temperature response < ± 0.4 % (-30 to +50 °C) with correction in data processing
Calibration certificate Included
Temperature response test of individual instrument Report included
Standard cable length 5 m (16.4 ft)

Overview

DR20 DR15 1A webv1901

Hukseflux model DR20 pyrheliometer is an ISO 9060 spectrally flat Class A instrument. Together with DR15 pyrheliometer, it replaces the models DR01, DR02 and DR03. DR20 has a better temperature response than DR15. Both instruments offer the highest accuracy and highest data availability, featuring window heating at low offsets. At the same heating power, the heating has been improved with a factor 4, at a 4 times lower offset!

DR20 DR15 02 webv1901

DR20 pyrheliometer is applied in high-accuracy measurement of the solar radiation received by a plane surface from a 5 ° full field of view angle. This quantity, expressed in W/m², is called “direct” solar radiation or DNI (direct normal irradiance). It is necessary to keep the instrument pointed at the sun by using a two-axis tracker.

hfluxman DR15 DR20 52 mediumprint bannerv1901

A pyrheliometer is used in tracker-mounted operation. DR20-A1 can be connected directly to commonly used data logging systems. It offers analogue output in the millivolt range. The pyrheliometer features a precision ground and polished quartz window, a compact sized collimated tube and a thermopile sensor with black coated surface. High data availability is attained by heating of the front window. This suppresses dew and frost deposition at a very low power consumption: DR20 needs only 1 W to keep its window free from dew and frost.

DR30 5 window assembly heater webv1802Using DR20 / DR15 pyrheliometers offer significant benefits over the use of competing models. The pyrheliometers offer the highest accuracy and highest data availability, featuring heating at low offsets. The advantages of having a heater are demonstrated in graphs in the DR20 brochure (PDF)

DR20 DR15 3B webv1901As required by ISO 9060 for Class A classification, each DR20 is supplied with test results for the individual instrument:

sensitivity
response time
temperature response

 

Suggested Use

  • Solar energy surveys
  • Solar resource assessments
  • Meteorological networks
  • Sites with dew and frost problems

Areas of Application

Meteorology / surface energy flux measurement
Solar energy / PV system performance monitoring

Frequently asked questions

How does a pyranometer work?

A pyranometer measures the solar radiation received by a plane surface from a 180 ° field of view angle. This quantity, expressed in W/m², is called “hemispherical” solar radiation. The solar radiation spectrum extends roughly from 285 to 3000 x 10⁻⁹ m. By definition a pyranometer should cover that spectral range with a spectral selectivity that is as “flat” as possible.

In an irradiance measurement by definition the response to “beam” radiation varies with the cosine of the angle of incidence; i.e. it should have full response when the solar radiation hits the sensor perpendicularly (normal to the surface, sun at zenith, 0 ° angle of incidence), zero response when the sun is at the horizon (90 ° angle of incidence, 90 ° zenith angle), and 50 % of full response at 60 ° angle of incidence. A pyranometer should have a so-called “directional response” (older documents mention “cosine response”) that is as close as possible to the ideal cosine characteristic.

In order to attain the proper directional and spectral characteristics, a pyranometer’s main components are:

•    a thermal sensor with black coating. It has a flat spectrum covering the 200 to 50000 x 10⁻⁹ m range, and has a near-perfect directional response. The coating absorbs all solar radiation and, at the moment of absorption, converts it to heat. The heat flows through the sensor to the sensor body. The thermopile sensor generates a voltage output signal that is proportional to the solar irradiance.

•    a glass dome. This dome limits the spectral range from 285 to 3000 x 10⁻⁹ m (cutting off the part above 3000 x 10⁻⁹ m), while preserving the 180 ° field of view angle. Another function of the dome is that it shields the thermopile sensor from the environment (convection, rain).

•    a second (inner) glass dome: For secondary standard and first class pyranometers, two domes are used, and not one single dome. This construction provides an additional “radiation shield”, resulting in a better thermal equilibrium between the sensor and inner dome, compared to using a single dome. The effect of having a second dome is a strong reduction of instrument offsets.

•    a heater: in order to reduce the effect of dew deposition and frost on the outer dome surface, most advanced pyranometers have a built-in heater. The heater is coupled to the sensor body. Heating a pyranometer can generate additional irradiance offset signals, therefore it is recommended to activate the heater only during night-time. Combining a heater with external ventilation makes these heating offsets very low.

Why use a pyranometer?

There are good reasons why pyranometers are the standard for solar radiation measurement in outdoor PV system performance monitoring.

The purpose of outdoor PV testing is to compare the available resource to system output and thus to determine efficiency. The efficiency estimate serves as an indication of overall performance and stability. It also serves as a reference for remote diagnostics and need for servicing.

The irradiance measurement for outdoor PV performance monitoring is usually carried out with pyranometers. Some standards suggest using PV reference cells. Reference cells are (with some minor exceptions) unsuitable for proof in bankability and in proof of PV system efficiency. Pyranometers are and will remain the standard for outdoor solar energy monitoring.

From a fundamental point of view:

  • Pyranometers measure truly available solar irradiance (so the amount of available resource). This is the parameter you need to have for a true efficiency calculation.
  • Reference cells measure only that part of solar radiation that can be used by cells of identical material and identical packaging (flat window), so the yield of a certain PV cell type. This is not a measurement that can be used in an efficiency calculation and in fact leads to several percentage points error in efficiency estimates.

The International Energy Agency (IEA) and ASTM standards for PV monitoring recommend pyranometers for outdoor PV monitoring. PV reference cells do not meet IEC 61724-1 class A requirements for irradiance measurement uncertainty: their directional response makes them systematically overestimate daily radiant exposure in J/m2 (or W·hr/m2 ) by more than 2 %, larger on hourly basis.

How do I choose a pyranometer?

Choosing the right pyranometer for your application is not an easy task. We can offer assistance. But first, you should ask yourself the following questions:

  • are there standards for my application?
  • what level of accuracy do I need?
  • what will be the instrument maintenance level?
  • what are the interfacing possibilities?

When discussing with Hukseflux, our recommendation for the best suited pyranometer will be based on:

  • recommended pyranometer class
  • recommended maintenance level
  • estimate of the measurement accuracy
  • recommended calibration policy
  • recommended interface

Pyranometers can be manufactured to different specifications and with different levels of verification and characterisation during production. The ISO 9060 – 1990 standard, “Solar energy – specification and classification of instruments for measuring hemispherical solar and direct solar radiation”, distinguishes between 3 classes; secondary standard (highest accuracy), first class (second highest accuracy) and second class (third highest accuracy). From second class to first class and from first class to secondary standard, the achievable accuracy improves by a factor 2.

The ISO 9060 – 1990 standard is up for revision. The new 2018 version of the standard will be slightly different from the 1990 version. The new version of ISO 9060 includes three instrument accuracy classes A, B and C, and a special extension of every class “Spectrally Flat”, which is recommended for Plane of Array (POA), albedo, and reflected solar measurements.

Our pyranometer selection guide offers practical guidelines for choosing a pyranometer. The application of pyranometers in PV system performance monitoring according to IEC 61724-1 is highlighted as an example. Sensors specific for diffuse radiation and meteorological networks are also addressed in this selection guide.

What is the difference between a pyrheliometer and a pyranometer?

A pyranometer measures hemispherical solar radiation. When measuring in the horizontal plane this is called Global Horizontal Irradiance (GHI). When measuring in “plane of array”, next to PV panels, this is called plane of array POA irradiance.

A pyrheliometer is used to measure Direct Normal Irradiance (DNI). DNI is defined as the solar radiant flux collected by a plane unit surface normal to the axis pointing towards the centre of the sun, within an optical angular aperture. DNI is composed of the solar irradiance within the extent of the solar disk (half-angle 0.266 ° ± 1.7 %) plus some circumsolar radiation.