REVISION DATE: 04-Dec-2015 14:30:29

 
Email from Casey on 4 Dec 2015 11:09 am: 
 
Hi Everyone, 
 
New data is up. 
 
All files were taken without dark noise removed.  You will find the dark noise cube in the folder that is valid for all of  
the cubes.  I have also subtracted the temporal mean of the dark noise cube and included those corrected files as well.   
The Radiometric Response should be the response of the system in microflicks/DN, but I have not had time to error check this yet. 
 
Integration times of the system are in the header files as "shutter".  This reflects the electronic integration time of the CCD, 
as the mechanical shutter is open slightly longer that the CCD is integrating for (as I understand this camera anyway). 
 
The "radiance" file has all of the fibers looking into the integrating sphere. 
 
The data is in calibrated wavelengths.  The spectral range of the system is 503.7 nm to 911.4 nm, although as Mike pointed 
out the cut-on wavelength is closer to 540 nm due to the high pass filter coating. 
 
Please let me know if you have questions or have specific data you would like collected. 
 
Thanks, 
Casey 

Files sent: RadiometricResponse_Microflicks.bip, channel8_radiance.bip, helium.bip allfibers_radiance.bip, channel8_radiance_darkremoved.bip, helium_darkremoved.bip allfibers_radiance_darkremoved.bip, dark_100ms.bip

Below are my graphs of the dark_100ms.bip file. The file contains 20 dark images at 0.1 sec

I removed all the data greater than 5300 and less than 1900 and then meaned all 20 images to get the surface below.

Figure 1

This is a cross section through the tracks at a number of wavelength pixels, from the mean image. Interesting shape, the BS1 darks look the similar.

Figure 2

The darks for each track from the mean dark image.

Figure 3

The darks for each track from the 20 dark images (so there are 20 for each track).

Figure 4