Public Lab is an open community which collaboratively develops accessible, open source, Do-It-Yourself technologies for investigating local environmental health and justice issues.
This is a testing site only. See the live Public Lab site here »
If you cannot use the ReCaptcha to verify you are not a bot, use this alternative verification.
sign up to join the Public Lab community
Forgot your password? Reset it here
by jsbonillam |
January 05, 2018 19:53 |
I think the Lego spectrometer's suitability for this is an open question, but the Raspberry Pi Camera v2 is very low noise and could be worth testing this idea out with. Please post your results if you do!
Reply to this comment...
Log in to comment
How would you set up the spectrometer next to the other equipment, or the tracker? Are you using a raspberry pi camera as-is, as well, or just as part of a spectrometer?
Is this a question? Click here to post it to the Questions page.
@warren The camera will be just part of the spectrometer. I am still considering whether to use LDRs (light depending resistors), as here http://www.instructables.com/id/Arduino-Solar-Tracker/ or using Pysolar which calculates the Sun's predited position according to your coordinates http://pysolar.org/ . I personally like more the first one but both of them seem fine. Just tell me if you think one of them is better.
Oh, i don't know, but it looks very cool!
Please forgive the question, but what lines are you using and what method of analysis? Thank you for the information.
I am going to make and analyse the graphs with the wavelength and absorption.
Only one suggestion then. Sunlight can be strong. As a safety measure, partially block the sun and work your way up to full exposure. Might not be needed, but better safe than sorry.
I have used photographic neutral density filters and have not been able to view the sun directly using the spec3 highly modified device. The attenuation ranged from 2-400 and have added additional attenuation resultong in overexposed images. Do a search of my previous spectra. I have built many versions of the original.
There are two approaches to this, the hardware and software. Sounds like you took care of the hardware end very well. Can you think of any software modifications or settings you could have changed?
What I was alluding to is that with all of the filter attenuation, the cmos sensor was still overloaded. This can be seen in the spectra submitted by me and others. My opinion is that once the input (sun) is normalized, all of the software tricks can't help.
I, too am trying to get spectral data of sun/sunsets. Would be interested to hear what you've learned
Further to my previous replies, it may be possible to view the sun disk attenuated with the filters used by welders to view their work. I have not as yet tried this idea but do know that these filters are replaceable. Try harrbor freight or some other supply store for these filters. No guarantees that this will work for you, as it would require some form of spectral calibration to see what the response is.
Good luck with your project.
This is part of: