Schlieren Imaging: Difference between revisions
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[[File:Setup V1.jpg|720px|Experimental Setup]] | [[File:Setup V1.jpg|720px|Experimental Setup]] | ||
The light source is a high power led to make | The light source is a high-power led that drives at about 3V 3A. There is an aperture in front of the led to block most of the light and make the source a point source. A concave mirror is located at 2f from the source. The concave mirror has a small angle to the instance beam. So the reflected light will go beside. There is a knife-edge at the reflection path about 2f from the concave mirror. Its function is to block half of the beam. A camera is located behind the knife edge to view the image. | ||
===Version 2=== | ===Version 2=== | ||
Revision as of 08:37, 27 April 2022
Idea
Schlieren Imaging is a technique proposed by the German physicist August Toepler in 1864 to study supersonic motion. We are using this tool to see the ultrasound wave and its propagation. The sound wave is propagation by the vibration of the air. When the air vibrates, the air will be either denser or less.
Setup
Version 1
The optical setup is shown below.
The light source is a high-power led that drives at about 3V 3A. There is an aperture in front of the led to block most of the light and make the source a point source. A concave mirror is located at 2f from the source. The concave mirror has a small angle to the instance beam. So the reflected light will go beside. There is a knife-edge at the reflection path about 2f from the concave mirror. Its function is to block half of the beam. A camera is located behind the knife edge to view the image.
Version 2
Measurements
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