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12. 12. 2018

Sky Scanner

We have assembled and put into operation a functional sample of equipment for interval imaging of the day sky (image collection, pre-processing and sending to a computer server) – sky scanners. The device consists of an IP camera, Rapberry Pi and aggregation software.

Location

The facility is located and is in operation on the south roof of UCEEB CTU, Třinecká 1024, Buštěhrad.

Technical parameters

It consists of a device consisting of three parts: a panoramic IP camera, a tripod and a Raspberry Pi device with operating software. The tripod consists of a modified concrete tile weighing about 20 kg, ensuring sufficient stability. The selected IP camera requires a POE injector for its power supply, while the Raspberry Pi requires a power adapter. The IP camera is resistant to weather conditions, the power adapter is stored in a covered distribution box.

Purpose and function

Sky Imager is a stand-alone device for acquiring images of the sky, on the basis of which a short-term exposure prediction is calculated on a remote computer server.

The goal of the device is to acquire images of the sky at predefined intervals and time spans. These images are pre-processed mainly by applying a predefined mask, which filters out unwanted (typically static) objects from the image.

The images are then sent to a computer server for further processing via a secure interface. If the image cannot be sent, it is stored in the device’s external memory for later transmission. This greatly increases the resistance of scanning to Internet connection outages. This ensures long-term continuous sensing, which is important for the development and testing of prediction algorithms.

Parameters

A functional connection of the Raspberry Pi with an IP camera and connection to the Internet is assumed. The preprocessing performed by the operating software is given by the image mask. The scanning interval is determined by the configuration of the operating software.

Detailed information about the software, including the source code and its settings, can be found here: https://github.com/UCEEB/Sky-Imager-Aggregator.

The device can cope with a short-term loss of Internet connection depending on the size of the external memory of the Raspberry Pi device, which ensures continuous scanning. Just to give you an idea, in the current setup, the device is able to bridge a 2-day internet connection outage.

Wiring diagram

The sky imaging system physically consists of three parts – an imaging camera, an image aggregation device and a computer server.

  • The camera is a panoramic outdoor IP camera connected to a home LAN. It is located on the highest point of the roof, so that the view of the sky is as unobstructed as possible in all directions.
  • The image aggregation device is a Raspberry Pi. It is connected to the home LAN so that it can communicate with the IP camera and at the same time with the computer server.
  • The computer server is a remote UCEEB CTU server, to which Raspberry Pi sends the acquired images. The server stores images and uses them to predict exposure at the same time.