Astronomical Time Switch Eclipse Detection
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Solution Overview
Problem
Conventional astronomical time switches do not react to local solar eclipses, making them unsuitable for safety-critical applications like street lighting, obstruction lighting for air traffic or shipping, and outdoor lighting systems, as they rely on sunrise and sunset times rather than the specific lighting conditions during an eclipse.
Innovation Solution
An astronomical time switch that calculates the degree of a solar eclipse based on location and time, using astronomical algorithms and constants, and controls a switching element when the eclipse reaches a certain threshold, thereby enabling appropriate lighting during solar eclipses.
Engineering Contradictions & Design Principles
Engineering Contradiction Analysis
1Reliability
If conventional astronomical time switches are used to control lighting systems, then the lighting can be switched automatically based on sunrise and sunset times, but the system does not react to local solar eclipses and is therefore unsuitable for safety-critical applications
Solution Approach 1:
The microcontroller pre-calculates the eclipse degree for future time points using astronomical algorithms and compares it with a threshold value before the eclipse occurs, enabling the lighting system to be switched on in advance for safety-critical applications
Solution Approach 2:
The patent introduces an intermediary calculation layer that computes the eclipse degree based on the relative positions of the sun and moon, serving as a mediator between astronomical data and the lighting control decision
2Adaptability or versatility
If external light sensors are used to detect solar eclipses, then the lighting system can react to changing light conditions, but additional installation work is required and the system reliability decreases due to exposure to ambient climate
Solution Approach 1:
The astronomical time switch performs self-service by internally calculating the eclipse degree using stored astronomical algorithms and current time data, eliminating the need for external light sensors and their associated installation and reliability issues
Solution Approach 2:
The patent replaces the physical light sensing mechanism with a computational approach, substituting mechanical/optical detection with mathematical calculations of celestial body positions
3Adaptability or versatility
If external light sensors are used, then lighting control during eclipses is possible, but the measured values are significantly affected by snow deposits, icing, radiation degradation, dust deposits, and biological impairment
Solution Approach 1:
Instead of directly measuring light conditions that are prone to measurement errors, the system creates a computational model (copy) of the expected light conditions during an eclipse based on astronomical calculations, allowing for accurate prediction without physical measurement
4Adaptability or versatility
If external light sensors are used, then the lighting system can be controlled during eclipses, but the housing material degrades due to radiation and the sensor is exposed to vandalism or targeted manipulation
Solution Approach 1:
The patent extracts the light sensing function from the physical domain and relocates it to the computational domain, removing the vulnerable external light sensor and its housing from the system architecture
Data Source
Figure 1~2b
Figure 3a~4
AI summary
Conventional astronomical timers are used for lighting control and are capable of performing circuits based on locally calculated sunrise and sunset times. However, they do not respond to a local solar eclipse, during which the natural illuminance can decrease so drastically, depending on the degree of the eclipse, that switching on a lighting system becomes necessary. The invention provides that the astronomical timer, based on input data and stored astronomical algorithms and constants, calculates the degree of a solar eclipse (11) depending on the location and local time and switches on at least one switching element (17, 18) as long as the calculated degree of the solar eclipse (11) is equal to or greater than a definable limit (19).