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Chilbolton Observatory

Atmospheric Instrument Suite

The atmospheric instrument suite at Chilbolton Observatory allows people to use Atmospheric Instruments for their research and data retrieval. The suite includes radars, lidars, radiometers and meteorological sensors to gather fata on aerosols, water vapour, clouds and precipitation.

Chilbolton satellite dish

Access to instruments

The Atmospheric Instrument Suite at Chilbolton Observatory provides national capability for the remote sensing of clouds, rainfall and aerosols, and is particularly well suited as a site for hosting field campaigns involving visiting instruments.

Access expertise and support

Chilbolton Observatory is managed by a team of dedicated technicians, engineers and scientists who are experienced in the usage of atmospheric facilities. We have a long-standing experience supporting experimentation on site, and can connect you to our network of atmospheric researchers.

Instrument Details

Chilbolton Advanced Meteorological Radar (CAMRa)

CAMRa is a 3 GHz S‑band radar mounted on a 25‑metre fully steerable antenna, offering exceptional sensitivity and high‑resolution observations of clouds and storms. Its dual‑polarisation capability enables measurement of hydrometeor shape and orientation, while full Doppler capability provides radial wind information.

UV Raman Lidar

The Chilbolton UV Raman lidar makes measurements of both elastically and inelastically (Raman) scattered radiation. The system transmits at a wavelength of 355 nm and measures cloud, water vapour and aerosol profiles.

Rain gauges and disdrometers

The range of raingauges at Chilbolton Observatory includes:

  • RAL Rapid Response Drop Counting rain gauges
  • A Distromet RD-80 Impact Disdrometer
  • A RW Munro 0.2mm Tipping Bucket rain gauge

The Chilbolton disdrometers provide an essential link between actual size measurements of rain drops and the drop size information derived from the 3 GHz CAMRa radar.

Sunphotometer

The Chilbolton sunphotometer measures aerosol optical thickness (AOT) in the wavelength range 340 – 1640 nm.

The Cimel CE318 sunphotometer measures the radiation received from the sun at 15 wavelengths in the wavelength range 340 nm to 1640 nm. It uses these measurements to deduce the aerosol optical thickness (AOT) of the atmosphere at these wavelengths. It order to do this reliably, there must be no cloud present in the direction of the sun for the duration of the measurements. If the sky is clear enough it can also derive other quantities such as particle size, real and imaginary components of refractive index and phase function at various wavelengths.

About Chilbolton Observatory

Chilbolton Observatory exists to provide a nationally relevant and unique field test and development environment to power discoveries and innovation so that together we advance knowledge, improve lives and deliver growth

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Control Room Chilbolton

See more facilities at Chilbolton Observatory

Access our facilities

Chilbolton Observatory facilities are available to use by UK and international researchers, industry users and funded programmes. 

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