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This is an old revision of this page, as edited by 82.233.216.159 (talk) at 21:54, 12 December 2007 (→‎Regarding the first paragraph -last sentence). The present address (URL) is a permanent link to this revision, which may differ significantly from the current revision.

confusion surrounding the term

The confusion surrounding the term spectrometer is not Wikipedia's fault, but we do need to sort it out.

See [1], [2], [3], [4], [5], [6] for some conflicting definitions.

Work in progress. Ultimately, we need to combine several articles and disambiguate others, so all the accepted usages are clearly explained and so readers of all backgrounds can easily get the information they want. Andrewa 20:09, 1 Dec 2003 (UTC)

See also for some history and other background:

I'll incorporate these links and material as I get time... or feel free! Andrewa 07:00, 2 Dec 2003 (UTC)

Blackbody

The article says:

When a material is heated to incandescence it emits light that is characteristic of the atomic makeup of the material.

Shouldn't blackbody radiation be mentioned on this place? --Abdull 5 July 2005 15:14 (UTC)

Everything with any non zero temperature emits blackbody radiation. To the first order, blackbody radiation is independent of the material. --150.203.177.218 06:44, 10 October 2006 (UTC)[reply]

The article is alluding to atomic emission lines. The energy of an emission line (which has a reciprocal relation to wavelength or color in the visible range) is related to the differences in the quantum energy levels of the electrons that emit the photons in question.

Incandescent objects usually do emit something like a blackbody spectrum, in fact we speak of the color temperature of a source, the temperature of the blackbody that would emit such a spectrum.

So I think that using the term incandescence to describe the origin of the phenomenon confuses the issue, it ought to be changed. The emission lines are real though, and important.

AJim 04:06, 27 May 2007 (UTC)[reply]

Fraunhofer or Kirchhoff/Bunsen?

The Joseph von Fraunhofer page describes him as the inventor of the spectroscope. A search for spectrosocope redirects to spectrometer which is said to have been invented by Kirchhoff and Bunsen. No doubt relates to the confusion over the term spectrometer as described below by Andrewa.

—The preceding unsigned comment was added by 59.92.140.254 (talkcontribs) .

Rearding the first sentence

, please note that a spectrometer is not necessarily a optical device!!. For example, s nuclear spectrometer uses no optics. Someone, other than me, could fix that. :)

Regarding the first paragraph -last sentence

.. radio and audio? audio isn't part of the EM spectrum.. is this true, does it need clarifying?

I agree, I removed it.

Build Your Own

This is an important article, that many other articles need to refer to -- and it needs a lot of work. We need an article about just optic applications, either this one or some other -- all the acoustic etc other uses need to be separated. We need lots of illustrations, some in color -- let's start with the ones from the Spectroscopy article.

Although the fancy versions of these instruments can cost thousands of dollars, let's also emphasize that any prism or diffraction grating can manifest these behaviors, and they are all around us, even the surface of a CD. Edmund Scientific offers a variety of Spectrometers and Spectroscopes in their Light Analysis category for $1-50. They also offer info on:

  • Build Your Own Grating Spectroscope
  • How Diffraction Gratings Work [7]

These are interesting resources:

-69.87.199.97 11:26, 26 May 2007 (UTC)[reply]

"A simple spectrometer can be built from a CD and a box. Cut a slit on one side of the box. Place the CD on the other side with about 60 degree angle. Look down into the openning on the box. The slit should not be too wide, otherwise the spectrum lines will be blurred. It should not be too narrow either, otherwise the spectrum is too dim. I use a 0.2mm wide slit."
Spectrographs of common light sources

  • CD spectrometer CD + cardboard tube or cereal box
  • [8] Great construction photos, razor-blade slit
  • [9] "MiniSpectroscopy displays a visual representation (a "spectroscope view") of a sample spectrum simultaneously with a graphical (intensity vs. wavelength) representation. Students draw or redraw the graph using the computer mouse, and the corresponding "spectroscope view" appears or changes immediately as they draw, changing just as changes are made in the graph. This immediate feedback gives students a kinesthetic connection between making the graph and viewing the spectrum being represented."
  • Mini Spectroscopes "You can make a spectroscope to allow you to separate the colors of light..."
  • How to work with the spectroscope : a manual of practical manipulation with spectroscopes of all kinds 1882;

Browning, John (1835-1925) NOT_IN_COPYRIGHT - online full-text download -69.87.204.146 16:17, 26 May 2007 (UTC)[reply]

It is indeed easy to build a simple device, although the CD device described is more like a spectrograph than a spectrometer. The problems begin when you attempt to make quantitative measurements, which is what the term spectrometer implies. It is quite difficult to build an instrument where measurements will obey the Beer-Lambert law over more than a small range of absorbance, for instance, especially when high spectral resolution in needed at the same time. The monochromator article tries to explain some of the difficulties and the range of devices for the optical range. There is an big difference between even a simple .1m single monochromator instrument and a .4m double monochromator instrument for use in analytical chemistry. There is an even bigger difference between these and a 2m double monochromator astronomical instrument. The relative prices of such instruments reflect that difference.

AJim 04:27, 27 May 2007 (UTC)[reply]

When one builds a simple CD, DVD, or other cheap diffraction grating/hologram-based device, the usable frequency response is normally limited by the human eye looking at the output, or the ordinary camera recording the picture. But, what are the inherent limits of these simple devices? How flat in the visible? How far into the UV/IR, how flat? And what simple/cheap detectors, multi-element (CCD etc) or single element (mechanically scannable) would have usable response into the UV/IR bands? And is there a simple/cheap way to use film etc to record the bands? This must have been important, decades ago? Links to detailed info about how it was done, and most practical ways to do now?-69.87.203.17 21:15, 27 May 2007 (UTC)[reply]

equal-area power graphs?

Standard optical power spectrum plots are spaced equal-nm on the X axis. The Y axis is some unit of power (if one is lucky enough to have calibrated data). Does this result in equal-area power graphs? If not, is there a standard way to distort the X or Y axis to obtain equal-area power graphs, and if so, what are such plots called. (In other words, what we want is a graph that shows visually, vividly, obviously, what portion (half?) of the sun's radiation is in the visible spectrum, for example. Are the plots in the Solar radiation article properly conveying such info?)-69.87.203.17 21:25, 27 May 2007 (UTC)[reply]

I've noticed that somebody has been adding links to my spectroscopy website and somebody later removes them. For the information of both the adder and remover: When you add a link to my website, include my full name and specifics on what the website is added for. When you remove a link, keep in mind that I am not the one who adds the links. I have published links from my website to certain articles/sections, but I always sign with my name.

This idiocy must stop sometime. Galidakis 16:59, 4 June 2007 (UTC)[reply]