RA01

RA01 is a market leading 2-component radiometer, used in scientific-grade energy balance and surface flux studies. It offers 2 separate measurements of solar and longwave radiation. Product features include a modular design, low weight, and easy levelling, and low solar offsets in the longwave measurement. The unique capability to heat the pyrgeometer reduces measurement errors caused by dew deposition. When combined with estimates of solar albedo and of local surface temperature, this instrument can also be used for estimation of net radiation. The advantages of this approach are cost reduction and independence from local surface properties.

  • Modular design, low weight and easy levelling
  • Low solar offsets in the longwave measurement
  • Unique capability to heat the pyrgeometer reducing measurement errors caused by dew

Description

Specifications

Measurand downward longwave radiation*global solar radiation
Optional measurand sky temperature*solar duration
Included sensors 1 x ISO 9060 second class pyranometer 1 x pyrgeometer with 150 ° field of view angle
Calibration traceability solar to WRR
Spectral range solar 285 to 3000 x 10⁻⁹ m
Calibration traceability longwave to WISG
Spectral range longwave 4.5 to 40 x 10⁻⁶ m
Required readout 2 x DC voltage 1x Pt100
Rated operating temperature range -40 to +80 °C
Temperature sensor Pt100
Measurand Pt100 instrument body temperature
Heater on pyrgeometer 1.5 W at 12 VDC
Levelling 2-axis levelling assembly (included)
Mounting on a 1 inch NPS tube; RA01 delivery includes a shim for easy alternative mounting on a ¾ inch tube (tubes not included)
Standard cable length 2 x 5 m (16.4 ft) (see options)
* Required measurand instrument body temperature
Options • Longer cable, in multiples of 5 m, cable lengths above 20 m in multiples of 10 m
• Upgrade to NR01 net radiometer

Overview

RA01 radiometers 1webv1201RA01 2-Component Radiometer
RA01 radiometer measures 2 separate components of the surface radiation balance: solar and longwave radiation. The solar radiation sensor is called pyranometer and the longwave sensor is called pyrgeometer. For calculation of sky temperature, a Pt100 temperature sensor is included in the pyrgeometer. To prevent deposition of dew, the pyrgeometer has internal heating. A 2-axis levelling assembly is included.

RA01 6webv1201RA01 Operation
Using RA01 radiometer is easy. It can be connected directly to commonly used data logging systems. The irradiance levels in W/m² are calculated by dividing the RA01 outputs, small voltages, by the sensitivities. The longwave irradiance should be corrected using the instrument body temperature. The sensitivities of all sensors are provided with RA01 on its product certificate. RA01 radiometers are often used in scientific-grade energy balance and surface flux studies.

RA01 radiation sensor 3webv1201RA01 Radiometer Design
RA01 radiometer has a modular design: it is possible to take the instrument apart and replace or re-calibrate individual sensors. A 2-axis levelling assembly is included. The levelling assembly fits a 1 inch NPS tube (the tube’s recommended outer diameter equals 33.4 x 10⁻³ m). With the RA01 shim, included in RA01’s delivery, a ¾ inch NPS tube may also be used.

Suggested Use

  • Energy balance studies
  • Surface flux measurements
  • Climatological networks

Areas of Application

  • Meteorology / surface energy flux measurement

Options

  • longer cable, in multiples of 5 m, cable lengths above 20 m in multiples of 10 m
  • upgrade to NR01 net radiometer

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.