Hello Kai, great & inspiring presentation ! Just one technical question: You are using a (Thorlabs ?) grating with 300 lines / mm. Is this due to the fact that spectra from gratings with higher resolution will not fit onto the relatively small S50 chip ?
Wonderful presentation. However, the spectroscopy introduction using the flame example is not quite correct. The blue flame color generally doesn't correspond to that in blackbody emission. Rather, the blue is usually from chemiluminescence of CH*, and thus may not have temperature correlation. The yellow is generally from soot incandescence, and thus would have better blackbody emission correlation.
Amazing work getting so much out of this scope!
Thanks for the awesome presentation!
Very good presentation. Thank you.
love ur videos
Hello Kai,
great & inspiring presentation !
Just one technical question: You are using a (Thorlabs ?) grating with 300 lines / mm.
Is this due to the fact that spectra from gratings with higher resolution will not fit onto the relatively small S50 chip ?
Thanks for the presentation Kai and TAIC.
Thank you for this presentation
Would LOVE to hear from Eric and Tim about their eclipse results!!!!
We're having an eclipse image processing show on May 12! (Molly)
Pretty cool!
Wonderful presentation. However, the spectroscopy introduction using the flame example is not quite correct. The blue flame color generally doesn't correspond to that in blackbody emission. Rather, the blue is usually from chemiluminescence of CH*, and thus may not have temperature correlation. The yellow is generally from soot incandescence, and thus would have better blackbody emission correlation.
Around minute 21, 'a member'... sorry a member of what organization ???