Schlieren Imaging: Difference between revisions

From PC5214 wiki
Jump to navigation Jump to search
Jinyi (talk | contribs)
Jinyi (talk | contribs)
Line 11: Line 11:
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.
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.


The picture of the real setup looks like below. The concave mirror is on the left hand of the picture while the camera, knife edge, and the source are on the right-hand side.  
The picture of the real setup looks like below. The concave mirror is on the left hand of the picture while the camera, knife-edge, and the source are on the right-hand side.  


[[File:Whole real setup.jpeg|720px|Whole real setup]]
[[File:Whole real setup.jpeg|720px|Whole real setup]]


The source and the knife-edge are clearly shown below. A black cover is used to block the stray light so that it will not influence the imaging process as the light from the aperture to relatively too weak.  
The source and the knife-edge are clearly shown below. A black cover is used to block the stray light so that it will not influence the imaging process as the light from the aperture is relatively too weak. There is a bright blue dot on the knife edge. That is the beam with a minimum waist radius. So when the air density changes, the sharp


[[File:source setup.jpeg|720px|source setup]]
[[File:source setup.jpeg|720px|source setup]]

Revision as of 11:00, 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.

Experimental Setup

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.

The picture of the real setup looks like below. The concave mirror is on the left hand of the picture while the camera, knife-edge, and the source are on the right-hand side.

Whole real setup

The source and the knife-edge are clearly shown below. A black cover is used to block the stray light so that it will not influence the imaging process as the light from the aperture is relatively too weak. There is a bright blue dot on the knife edge. That is the beam with a minimum waist radius. So when the air density changes, the sharp

source setup

Version 2

Measurements

....