User:Pranav Rathi/Notebook/OT/2010/03/23: Difference between revisions
Pranav Rathi (talk | contribs) |
Pranav Rathi (talk | contribs) |
||
| Line 8: | Line 8: | ||
==OT alignment== | ==OT alignment== | ||
* Collimating the beam | * Collimating the beam | ||
---- | |||
== Beam Collimation == | |||
Method:I used our regular CCD camera with 3+2 O.D. filters + 25mm lance at .10W. First I diverted the beam at 90 degrees with two mirrors after the telescope, and then I placed the camera on the rail in near far-field. I captured the image and move the camera about 60cms (far field) and captured the image again. I compared the spot size in the two images with the help of image-j. In far-field beam looks smaller so I made its size equal (increase) to near-field, through the center dial of the telescope. I came back in near field and check the size again, this time it was bigger, so made it equal (decrease) to far-field by using the eye-piece of the telescope. I followed the process iteratively until the beam sizes match in far and near-field. The results are presented below. | |||
[[Image:Colimnear1at .10W.jpg|thumb|left|Beam in near-field at .10W; 6mm diameter]] | |||
Revision as of 15:54, 23 March 2010
 Project name
|
<html><img src="/images/9/94/Report.png" border="0" /></html> Main project page <html><img src="/images/c/c3/Resultset_previous.png" border="0" /></html>Previous entry<html> </html>Next entry<html><img src="/images/5/5c/Resultset_next.png" border="0" /></html> |
OT alignment
Beam CollimationMethod:I used our regular CCD camera with 3+2 O.D. filters + 25mm lance at .10W. First I diverted the beam at 90 degrees with two mirrors after the telescope, and then I placed the camera on the rail in near far-field. I captured the image and move the camera about 60cms (far field) and captured the image again. I compared the spot size in the two images with the help of image-j. In far-field beam looks smaller so I made its size equal (increase) to near-field, through the center dial of the telescope. I came back in near field and check the size again, this time it was bigger, so made it equal (decrease) to far-field by using the eye-piece of the telescope. I followed the process iteratively until the beam sizes match in far and near-field. The results are presented below.  |
|
