Overview

The Infrared Cloud Camera (IRCCAM) measures the thermal emission of the atmosphere in the 8 – 14 µm wavelength range in order to determine the fractional cloud-cover during day and night, as opposed to visible cloud cameras which only operate during the day.

Introduction

Data from visible all-sky cameras at Davos, Jungfraujoch and Payerne allow the fractional cloud-cover and cloud types to be automatically determined during the day (Wacker et al., 2015; Aebi et al., 2017). However, in order to complement these methods so that measurements during the night can be conducted, IRCCAM was developed.

IRCCAM consists of a commercial infrared camera (GOBI 640 GigE model) with a microbolometer detector array of 640 x 480 pixels which is sensitive in the 8 – 14 µm wavelength range. The camera points down onto a convex gold-plated mirror which images the sky hemisphere onto the camera detector. Calibration was conducted in the PMOD/WRC reference blackbody over a -20 to +20°C temperature range, with an uncertainty of ± 1°C.

A computer-controlled acquisition system collects sky images with a 1-minute resolution throughout the whole day.  After correction for distortion resulting from the convex mirror, images are then calibrated to give the fractional cloud cover as well as a brightness temperature map of the sky and clouds.

Figure 1. IRCCAM measuring at PMOD/WRC.

Figure 2 below shows a sky image from a visible camera (left panel) and IRCCAM (middle panel) in which the fractional cloud cover can be compared. For the period January to October 2016, >123,000 coincident camera images were collected, and ~65% and 85% were found to agree to within a cloud cover of 1 and 2 octas, respectively. The sky brightness temperature [°C] map (right panel) illustrates a wide-range of temperatures.

Figure 2. Sky image from 3 July 2016 showing: left panel) an image taken with a visible sky camera, middle panel) clouds detected by IRCCAM, and right panel) the sky brightness temperature map. The colours in both pictures on the right, represent the sky temperatures [°C] as shown in the colour-bar.

Specifications

Wavelength range 8 – 14 µm
Camera properties GOBI 640 GigE model, focal length: 25mm, field-of-view: 18° x 24°
Mirror properties Gold-coated aluminium mirror, radius sphere: 286 mm, diameter half-sphere: 390 mm
Detector array 640 x 480 px
Measurement frequency 1-minute (standard)
Outer dimensions Height = 186 cm

References

Aebi, C., Gröbner, J., Kämpfer, N., and Vuilleumier, L., (2017), Cloud radiative effect, cloud fraction and cloud type at two stations in Switzerland using hemispherical sky cameras, Atmos. Meas. Tech., 10, 4587-4600, https://doi.org/10.5194/amt-10-4587-2017
Aebi, C., Gröbner, J., and Kämpfer, N., (2018), Cloud fraction determined by thermal infrared and visible all-sky cameras, Atmos. Meas. Tech., 11, 5549-5563, https://doi.org/10.5194/amt-11-5549-2018
Wacker, S., Gröbner, J., Zysset, C., Diener, L., Tzoumanikas, P., Kazantzidis, A., Vuilleumier, L., Stöckli, R., Nyeki, S., and Kämpfer N., (2015), Cloud observations in Switzerland using hemispherical sky cameras, J. Geophys. Res., 120, https://doi.org/10.1002/2014JD02264
For further information please contact: Dr. Julian Gröbner