The CMP21, manufactured by Kipp & Zonen, is an ISO Class A (secondary-standard) pyranometer with an internal thermistor. It monitors solar radiation for the full solar spectrum range, and is well-suited for scientific use and in top-level solar-radiation monitoring networks. This pyranometer connects directly to a Campbell Scientific data logger.
CMP21以保护在两层玻璃穹顶罩中的高质量黑化热电堆来测量太阳辐射。内置的热敏电阻用于进行单独的最优温度补偿测量。
CMP21在285至2800 nm波段内具有平直的光谱灵敏度,因而非常适合自然太阳光测量的应用中,以及冠层下、温室中或建筑的太阳辐射监测,还可倒置安装用于监测反射短波辐射。
一支干燥剂筒用于防止CMP21的穹顶内侧结露。Campbell Scientific还提供CVF3加热通风罩,可防止辐射表穹顶表面结冰或结露。
CMP21含有一个直接固定的白色防辐射盖子,用于减小太阳辐射增温。自带的水平泡和可调水平螺丝,使得传感器并不需要额外的调平底座。
Sensor | High-quality blackened thermopile protected by two glass domes |
Measurement Description | Monitors solar radiation for the full solar spectrum range |
ISO Classification | Class A (secondary standard) |
Spectral Range | 285 to 2800 nm |
Sensitivity | 7 to 14 µV/W/m2 |
Temperature Dependence of Sensitivity | < 1% (-20° to +50°C) |
Response Time | < 5 s (95% of final value) |
Zero Offset Due to Thermal Radiation | < 7 W/m2 (200 W/m2) |
Non-Stability | < 0.5% (change/year) |
Non-Linearity | < 0.2% (0 to 1000 W/m2) |
Directional Error | < 10 W/m2 (up to 80° with 1000 W/m2 beam) |
Tilt Error | < 0.2% |
Level Accuracy | 0.1° |
Impedance | 10 to 100 Ω |
Operating Temperature Range | -40° to +80°C |
Typical Signal Output | 0 to 15 mV (for atmospheric applications) |
Maximum Irradiance | 4000 W/m2 |
Expected Daily Uncertainty | < 2% |
Dome Diameter | 5 cm (2 in.) |
Width | 15 cm (5.9 in.) with shield |
Height | 9.25 cm (3.64 in.) |
Weight | 0.9 kg (2 lb) with 10.1 m (33 ft) cable |
Please note: The following shows notable compatibility information. It is not a comprehensive list of all compatible products.
Product | Compatible | Note |
---|---|---|
CR1000X (retired) | ||
CR300 (retired) | ||
CR3000 (retired) | ||
CR310 | ||
CR350 | ||
CR6 | ||
CR800 (retired) | ||
CR850 (retired) |
The CMP21 has a bubble level and two leveling feet, which allow it to be leveled without using a leveling base. This pyranometer mounts to a mast, crossarm, or pole (1.0 in. to 2.1 in. OD) via the CM255 or CM255LS mounting stand. The CMP21 should be mounted away from all obstructions and reflective surfaces that might adversely effect the measurement.
CMP21-L: 6
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The ISO and WMO classify First Class pyranometers, such as the CMP6-L, as suitable for network operations. However, if accuracy is of paramount concern, consider using Class A pyranometers, such as the CMP11-L and CMP21-L, instead.
A cable length of 300 ft can be used with the understanding that additional noise may be introduced into the measurement. Typically, in systems with pyranometers, the sensors are installed near the data logger (within 50 ft). If an application requires long leads, contact Campbell Scientific for assistance.
No. These are all passive devices that create their own voltage signal as a response to the measurement being made. There is, however, a heater and ventilator for these sensors (CVF4-L) that requires a power supply.
All of these pyranometers measure the amount of solar short-wave radiation incident on a surface. Because of their accuracy and performance level, the CMP11-L and CMP21-L are classified by the International Organization for Standardization (ISO) and World Meteorological Organization (WMO) as Secondary Standard sensors, representing the highest level of measurements made by pyranometers. In comparison, the CMP6-L is classified as a First Class sensor, which is the middle classification for pyranometers. (Second Class is the lowest pyranometer classification.)
Yes. Each pyranometer is shipped with an instruction manual provided by Kipp & Zonen that contains information concerning its construction, spectral sensitivity, cosine response, and a simple sensor check out procedure. Included with the sensor and manual is a calibration certificate with the sensor sensitivity value and serial number.
Because of the loss of IR radiation, nearly all thermopile instruments typically have a negative offset. This offset is most easily visible at night-time, when a small negative value is read instead of zero. This same offset is present during the daytime, but it is not as visible because of the large solar signal.
Another common issue involves leveling an instrument. Leveling a thermopile instrument can cause errors in the direct beam component because the cosine response is not correct. These errors are more notable when the sun is close to the horizon because the angle is so shallow.