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VI/83 O3 and SO2 Absorption Cross Sections (Freeman+ 1984,88,93)
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High Resolution Absorption Cross-section Measurements of Ozone at 195 K in the
Wavelength Region 240-350 nm
Freeman D.E., Yoshino K., Esmond J.R., Parkinson W.H.
<Planetary Sp. Sci. 32(2): 239-248, (1984)>
Absolute Absorption Cross-section Measurements of Ozone in the Wavelength Region
238-335 nm and the Temperature Dependence
Yoshino K., Freeman D.E., Esmond J.R., Parkinson W.H.
<Planetary. Sp. Sci., 36(4): 395-398, (1988)>
Measurements of Absolute Absorption Cross Sections of Ozone in the 185-to 254-nm
Wavelength Region and the Temperature Dependence
Yoshino K., Esmond J.R., Freeman D.E., Parkinson W.H.
<J. Geophys. Res., March 20, 98(D3): 5205-5211 (1993)>
High Resolution Absorption Cross Section Measurements of SO2 at 213 K in the
Wavelength Region 172-240 nm
Freeman D.E., Yoshino Y., Esmond J.R., Parkinson W.H.
<Planetary Sp. Sci. 32, 1125-1134 (1984)>
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ADC_Keywords: Atomic physics; Spectroscopy; Cross sections
Abstract:
Cross sections of the Hartley-Huggins bands of O3 at the temperature
195K were obtained from photoabsorption measurements at column densities
in the range 2 x 10^17 - 1 x 10^21 cm-2 throughout the wavelength region
240-350 nm. Measurements of the absolute absorption cross-section of
ozone at the temperatures 195, 228 and 295 K were made at several
discrete wavelengths in the region 238-335 nm and measurements of the
relative absorption cross sections were made temperatures 195, 228 and
295 K throughout the wavelength region 185-254 nm. Laboratory
measurements at high resolution of the absorption cross section of SO2
at the temperature 213 K in the wavelength region 172-240 nm are also
given.
Introduction:
O3:
Cross sections of the Hartley-Huggins bands of O3 at the temperature 195
K were obtained from photoabsorption measurements at column
densities in the range 2 x 10^17 - 1 x 10^21 cm-2 throughout the
wavelength region 240-350 nm with a 6.65 m photoelectric scanning
spectrometer equipped with a 2400 lines mm-1 grating and operated at an
instrumental width (FWHM) of 0.003 nm. These were published in 1984.
The cross sections were later put on a different absolute basis
reflecting the absolute cross section measurements at discrete points of
ozone at three different temperatures, published in 1988 (Planetary
Space Science, 36(4): 395-398). The files available here reflect this
recalibration.
Laboratory measurements of the absolute absorption cross-section of
ozone at the temperatures 195, 228 and 295 K were made at several
discrete wavelengths in the region 238-335 nm. The results for ozone at
295 K are in excellent agreement with those of Hearn (1961, Proc. phys.
Soc. Lond., 78, 932), who used a different technique. Their absolute
cross-section measurements of ozone at 195 K have been used by the
authors to put their recent relative cross-section measurements at that
temperature (Freeman et al., 1984, Planet. Space Sci., 32, 239) on a
firm absolute basis throughout the region 240-335 nm;
Laboratory measurements of the relative absorption cross sections of
ozone at the temperatures 195, 228 and 295 K were made throughout the
wavelength region 185-254 nm. The absolute absorption cross sections at
the same temperatures were measured at several discrete wavelengths in
the region 185-254 nm. The absolute cross sections of ozone were used to
put relative cross sections on a firm absolute basis throughout the
region 185-255 nm. These recalibrated cross sections below 250 nm are
slightly lower than those of Molina and Molina (J. Geophys. Res., 91,
14501 (1986) ), but differences are within a few percent and would not
be significant in atmospheric applications.
These later measured cross sections supersede the earlier high
resolution measurements published (Planet. Space Sci., 32(2): 239-248,
(1984); and Planet. Space Sci., 36(4): 395-398, (1988) ) in the region
where they overlap.
SO2:
Laboratory measurements at high resolution of the absorption cross
section of SO2 at the temperature 213 K were made in the wavelength
region 172-240 nm with a 6.65 m scanning spectrometer/ spectrograph
operated at an instrumental width of 0.002 nm. The measured cross
sections are presented graphically in representative wavelength regions
and are available throughout the region 172-240 nm at wavenumber
intervals of 0.4-0.1 cm-1 The measured cross sections, which are
relevant to the photochemistry of planetary atmospheres, possess
significantly more spectroscopic structure, and are more accurate, than
previous measurements made at lower resolution.
File information:
The file o3k195 contains high resolution cross sections of ozone
at 195 K are arranged in files with points in ascending order of
wavenumber. This data was originally published in 1984, (Planetary Space
Science, 32(2): 239-248) with a discussion of the assumptions on which
the relative cross sections were put on an absolute basis. Later, in
1988, absolute cross section measurements were made with which the
original data was renormalized (Planetary Space Science, 36(4):
395-398). The cross section files here reflect these most recent
absolute measurements. The files sent only go down to 253.75 nm since
the cross section measurements of the region with wavenumber lower than
that has been superseded by new measurements in the region 185-254 nm
published in the Journal of Geophysical Research. This new data is at
significantly lower resolution than the earlier data.
The 3 files of data containing vuv cross sections of ozone at 195, 228
and 295 K are arranged in files with points in ascending order of
wavenumber. The file o3uvr.dat contains the cross sections measured at
295 K, o3uvd.dat at 195 K, and o3uvm.dat at 228 K. This data is
published in the March 20, 1993, edition of the Journal of Geophysical
Research, 98(D3): 5205-5211. These files supersede the old high
resolution measurements in the region where the two sets of data overlap
(240-254 nm).
The file so2k213.dat contains cross sections of SO2 at 213 K
arranged in ascending order of wavenumber. This data is published
in 1984, (Planetary Space Science, 32: 1125-1134).
The 3 files of data containing vuv cross sections of ozone at 195, 228
and 295 K are arranged in files with points in ascending order of
wavenumber. The file o3uvr.dat contains the cross sections measured at
295 K, o3uvd.dat at 195 K, and o3uvm.dat at 228 K. This data is
published in the March 20, 1993, edition of the Journal of Geophysical
Research, 98(D3): 5205-5211. These files supersede the old high
resolution measurements in the region where the two sets of data overlap
(240-254 nm).
File Summary:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
so2k213.dat 20 152512 sulfur dioxide cross sections
o3k195.dat 20 117011 Ozone cross sections at 213K
o3uvd.dat 20 5122 Ozone cross sections at 195K
o3uvm.dat 20 5122 Ozone cross sections at 228K
o3uvr.dat 20 5122 Ozone cross sections at 295K
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Byte-by-byte Description of file: *.dat
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Bytes Format Units Label Explanations
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1- 9 F9.3 cm-1 nu Wavenumber position,
10- 20 E11.3 --- sigma Cross section/molecule
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NOTE:
The measured data points are not necessarily equally spaced or constant
within a file or between files.
Acknowledgement:
We thank Dr. Yoshino and Jim Esmond for forwarding the files to us. We
also thank Mr. Esmond for reviewing our original document, providing
corrections and substantial additional information, and replacing a data
file which had been received in garbled form.
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(End) Nancy G. Roman [ADC/SSDOO] Oct-04-1995
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