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FrozenGate by Avery

Spectral Emission line DB

M

Mosc007

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Feb 2, 2012
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I have put together some information from the NIST database on Spectral Lines emmitted from 20 different Elements. I also added Graphs to make it easy to see were the strong lines are.

It's surprising how many lines some elements emit in the visable spectrum. Eg, Mercury emits 40 seperate lines. Out of that only 6 are strong lines.

The first sheet in the Excel File shows the Element and the emited spectral lines. The Wavelength is in Angstroms. Divide by 10 to get Nm. The intesnisty of the line I am not sure what units it is.

I was surprised to learn that Argon has some very strong lines in the Orange to Red spectrum. The normal 488nm etc lines from an Argon laser are quite low output. I guess that's why an Argon laser is so inefficient.

Excel Spreadsheet of Spectral Lines

Hopefuly some members will find it usefull. I wanted it to help decide which Spectral Discharge Tubes would be better for calibrating a Spectrometer.
 
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I was looking on eBay and find they combine argon and mercury for calibration sources. Add in neon for some reds. Wonder if you can put all three in a single source. Prob better having separate tubes.

I was looking at the replacement sensors on eBay that cut second order interference and add uv sensitivity. Wonder if they are worth the effort. Not sure why these seem to not let you get to the higher pixel numbers like 2000-2400. It would seem if the grating was set as such you’d see more lower pixels in the 400-450 range but you don’t.

I would think with 2400 pixels 400-800nm would be possible. Maybe the sensor is deaf above 450nm. This replacement might be a way to correct that but then your in the cost range to just buy one already doing that.

I think 1nm accurate is fine for Raman matching and fish tank testing.
 
I think you will find the CCD in these is only 2048 Pixels. The grating gives about 10 pixels per nm. Resulting in about a 200nm bandwidth. Approx 450-650nm.

I have looked at Neon and decided there are just to many lines near each other at similar intensities. It would be difficult to find the correct lines for calibration.
 
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kecked said:
I was looking on eBay and find they combine argon and mercury for calibration sources. Add in neon for some reds. Wonder if you can put all three in a single source. Prob better having separate tubes.

I was looking at the replacement sensors on eBay that cut second order interference and add uv sensitivity. Wonder if they are worth the effort. Not sure why these seem to not let you get to the higher pixel numbers like 2000-2400. It would seem if the grating was set as such you’d see more lower pixels in the 400-450 range but you don’t.

I would think with 2400 pixels 400-800nm would be possible. Maybe the sensor is deaf above 450nm. This replacement might be a way to correct that but then your in the cost range to just buy one already doing that.

I think 1nm accurate is fine for Raman matching and fish tank testing.
Click to expand...

You could change the grating and get a wider bandwidth at the cost of resolution.

Mosc007 said:
I think you will find the CCD in these is only 2048 Pixels. The grating gives about 10 pixels per nm. Resulting in about a 200nm bandwidth. Approx 450-650nm.

I have looked at Neon and decided there are just to many lines near each other at similar intensities. It would be difficult to find the correct lines for calibration.
Click to expand...

I took a sample of a neon light I have and compared it to some charts I found online. At first I thought the same as you, way too many lines but after looking closer at it I noticed it had the same pattern as the charts I found online. It was good enough to let me know my calibration is off a little at the ends lol.
 
I used neon and it was a pain but worked. So maybe I go usb2000 surplus or such. It’s just such fun with these because they are so inexpensive. I want to build a course around them. Change gratings align calibrate. Not many places do that kind of thing because the cost would be through the roof.

A friend of mine brought this to me and gave me cal for hene green, hene red, and a few others so all told I have about 20 lines to calibrate with. Most of my interest is down in the 700range at the moment.
 
kecked said:
I used neon and it was a pain but worked. So maybe I go usb2000 surplus or such. It’s just such fun with these because they are so inexpensive. I want to build a course around them. Change gratings align calibrate. Not many places do that kind of thing because the cost would be through the roof.

A friend of mine brought this to me and gave me cal for hene green, hene red, and a few others so all told I have about 20 lines to calibrate with. Most of my interest is down in the 700range at the moment.
Click to expand...

You can get these from the Science Surplus store with different gratings. But as said wider bandwidth means lower resolution.

I would like a USB4000 but a bit expensive even used.
 
kecked said:
I used neon and it was a pain but worked. So maybe I go usb2000 surplus or such. It’s just such fun with these because they are so inexpensive. I want to build a course around them. Change gratings align calibrate. Not many places do that kind of thing because the cost would be through the roof.

A friend of mine brought this to me and gave me cal for hene green, hene red, and a few others so all told I have about 20 lines to calibrate with. Most of my interest is down in the 700range at the moment.
Click to expand...

The usb2000 is a very good device , but .... it is the same sensor in it like in the B&W-TEK .... 2048 pcx.
 
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I'm assuming your lines are in Angstroms since you neglected to use any units. You said you also put each element in a spectrum. I couldn't find that. It is good information, though.
 
Was looking at the spreadsheet. Thank you for your efforts. It will be very useful.
 
paul1598419 said:
I'm assuming your lines are in Angstroms since you neglected to use any units. You said you also put each element in a spectrum. I couldn't find that. It is good information, though.
Click to expand...

Yes, They are in Angstroms. I did mention that in the first post.

You should see 2 Sheets in the Excel file. One has the Data and the other has the graphs.
 
I just checked again and all I get are the lists. I see the Angstrom remark in the post now. I read it twice looking for units. Don't know how I missed it.
 
paul1598419 said:
I just checked again and all I get are the lists. I see the Angstrom remark in the post now. I read it twice looking for units. Don't know how I missed it.
Click to expand...

What version of Excel are you using ?

There should be a Tab down the bottom to select which sheet to view.
 

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Thanks for the picture. Found them. Can't tell which lines correspond to the wavelength under the graph. I suppose I could figure it out by the relative intensity of the lines in the spread sheet.
 
paul1598419 said:
Thanks for the picture. Found them. Can't tell which lines correspond to the wavelength under the graph. I suppose I could figure it out by the relative intensity of the lines in the spread sheet.
Click to expand...

Yep, The Graph is just a guide to help find the Strong Lines. Once you know approx were they are you can look in the Data Tables for the precise wavelength.
 
Nice. Thanks for posting them. Should come in handy for people trying to calibrated their spectrometers. I just got my 575nm laser in and it has a gorgeous yellow dot with speckle all around it at 15 feet. Can't wait to get back into it. :thanks:

I'm out of rep at the moment, but will get you later today. Unless I got you just recently.
 
paul1598419 said:
Nice. Thanks for posting them. Should come in handy for people trying to calibrated their spectrometers. I just got my 575nm laser in and it has a gorgeous yellow dot with speckle all around it at 15 feet. Can't wait to get back into it. :thanks:

I'm out of rep at the moment, but will get you later today. Unless I got you just recently.
Click to expand...

Sounds great. Australia Post seems to be slow with mine. Expected today but not delivered. Hopefully tomorrow.
 
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