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Molecular spectroscopy is the study of absorption of light by molecules.
In the gas phase at low pressures, molecules exhibit absorption in narrow
lines which are very characteristic of the molecule as well as the temperature
and pressure of its environment. In the microwave and long-wavelength infrared
regions of the spectrum, these lines are due to quantized rotational motion
of the molecule. At shorter wavelengths similar lines are due to quantized
vibration and electronic motion as well as rotational motion. The precise
frequencies of these lines can be fit to quantum mechanical models which
can be used both to determine the structure of the molecule and to predict
the frequencies and intensities of other lines. Because this absorption
is so characteristic, it is very valuable for detecting molecules in the
Earth's stratosphere, planetary atmospheres, and even the interstellar
medium. This web site contains very specialized technical information.
While the general user is welcome to browse its contents, the descriptions
assume a knowledge of spectroscopy and quantum mechanics.
The JPL Molecular Spectroscopy Team supports NASA programs in Astrophysics,
Atmospheric Science, and Planetary Science. Its activities include measurement
of rotational lines, fitting the lines, and preparing a catalog of line
positions and intensities. The members of the team include
Pin Chen,
Timothy J. Crawford,
Brian J. Drouin,
John C. Pearson,
Shanshan Yu, and
Keeyoon Sung, and
Deacon Nemchick.
Quick Links
Guide to anonymous ftp file system for spec.jpl.nasa.gov
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The sub-directory calpgm
contains programs for fitting spectra. These programs are copyrighted,
but made freely available as a service to the spectroscopic community.
Some of the details of the program are described in H. M. Pickett, "The
Fitting and Prediction of Vibration-Rotation Spectra with Spin Interactions,"
J. Molec. Spectroscopy 148, 371-377 (1991). Check out the
on-line
documentation. There is also a manuscript detailing some of the uses
of the software; B. J. Drouin, "Practical Uses of SPFIT," J. Molec.
Spectroscopy 340, 1-15, 2017.
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The sub-directory catalog
contains files related to the JPL spectral line catalog. The file
catdir.cat
contains the current catalog directory in a format described in the written
catalog description. Line files are designated as ctttttt.cat, where tttttt
is the zero-filled catalog tag number (the first entry in each line of
the catdir.cat file). For example, the H atom line list is in file c001001.cat.
The line files and the directory file are text files readable with usual
TExt file system utilities. It is recommended that they be transferred
under ftp using the ASCII option, although binary should work with UNIX
hosts. The file README
contains a short description of the format of catdir.cat and the catalog
files. A html
catalog directory is available which provides links to the catalog
entries and the associated documentation (in either pdf or Tex format).
The current literature reference for the catalog is H. M. Pickett,
R. L. Poynter, E. A. Cohen, M. L. Delitsky, J. C. Pearson, and H. S. P. Muller,
"Submillimeter, Millimeter, and Microwave Spectral Line Catalog,"
J. Quant. Spectrosc. & Rad. Transfer 60, 883-890 (1998).
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Documentation for the fitting and predicting software, SPFIT and SPCAT can be found in spinv.pdf.
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The sub-directory catalog/doc
contains the documentation for the line files. Documentation for a particular
species follows the line file naming convention except that the first character
is 'd' rather than 'c'. These files are text files in LATeX format. The
files catdoc.tex, catintro.tex, catdir.tex, and moldoc.tex are the files
used to generate the catalog descriptive report. The file pretex.tex can
be used to prepare a single document page. Processing the full documentation
will generate a document of over 300 pages!
If you have the free Adobe
Acrobat reader, you can read the document
catdoc.pdf
. A pdf version of the introductory information
about formats, etc., is available as
catintro.pdf
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The sub-directory catalog/pgm
contains utility programs for catalog access. The subroutine set catread.f
contains code for reading files into a FORTRAN program. These routines
use random access, and assume that the files have a fixed line length within
the file. Some modification of path names and file open options will be
required for operating systems other than UNIX. The program catlist.f uses
catread.f to provide listing of lines for selected molecules over a selected
frequency range.
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The sub-directory catalog/archive
contains the some of the input files for calculating the catalog files. The page provides a directory listing with links to the archive files.
WARNING: this file system is the living repository of the JPL
catalog. Recently added files may still be in a preliminary state. Caution
should be used for species which have a catdir.cat
line ending with '*', which have been modified since the last published
edition of the catalog.
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CL#97-1576 |
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Site
Manager: Brian Drouin
Webmasters: |
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