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Choose a frame rate equal to the lighting pulse rate divided by some integer.
This is often the simplest option since most corresponding shutter speeds will appear flicker-free. Choose a shutter speed equal to the lighting pulse rate divided by some integer.
Four LSTs will be arranged at the centre of both the northern and the southern hemisphere arrays to cover the unique low energy sensitivity of CTA between 20 and 200 Ge V.
The LSTs will also have a very good sensitivity up to energies of several Te V, which is, however, covered by Medium-Sized Telescopes (MSTs) more efficiently. It has a 23 m diameter parabolic reflective surface, which is supported by a tubular structure made of reinforced carbon fibre and steel tubes.
Piano lessons mississippi piano lessons mississippi. A reflective surface of 400 mcollects and focuses the Cherenkov light into the camera, where photomultiplier tubes convert the light in electrical signals that can be processed by dedicated electronics.Although the LST will stand 45 m tall and weigh around 100 tonnes, it will be extremely nimble, with the goal to be able to re-position within 20 seconds.Common power sources are 50 Hz (in Europe and most of Asia) and 60 Hz (in North America), which cause 100 and 120 pulses of light each second, respectively.Other than changing the lighting, one has two options for overcoming this problem: Frame Rates.Although light sources might appear continuous to our eyes, many actually illuminate using high frequency pulses of light.