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We record laboratory spectra at wavelengths of 2.47, 2.87, and
4.56 microns to study CH3D. We report temperature-dependent
absorption coefficients of these bands when the CH3D is diluted
in CH4 ice and also when it is dissolved in N2 ice.
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Citation |
Grundy, W.M., Morrison, S.J., Bovyn, M.J., Tegler, S.C., and
Cornelison, D.M., CH3D ice absorption coefficients V1.0.
EAR-X-I2041-5-CH3DICESPEC-V1.0. NASA Planetary Data System, 2014. |
Digital Object Identifier (DOI) |
Unable to retrieve DOI information. Please contact the PDS Help Desk for assistance.
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Data Set Abstract |
This data set is the result of laboratory transmission
spectroscopy experiments performed within a sealed cell in the
ice laboratory at Northern Arizona University. We record spectra
at wavelengths from 1 to 6 microns to study CH3D bands at 2.47,
2.87, and 4.56 microns (as indicated by '25',
'29' and '45' in the data file names). We
report temperature-dependent absorption coefficients of these
bands when the CH3D is diluted in CH4 ice and also when it is
dissolved in N2 ice. These absorption coefficient spectra can be
combined with data from the literature to simulate arbitrary D/H
ratio absorption coefficients for CH4 ice and for CH4 in N2 ice.
The data were originally published in 2011 in Icarus, vol. 212,
pp. 941-949, and that paper should be consulted for details about
laboratory procedures and limitations of the data. |
Search/Access Data |
SBN Comet Website
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Additional Information |
Mission Information |
SUPPORT ARCHIVES
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Data Set Information |
EAR-X-I2041-5-CH3DICESPEC-V1.0 |
Instrument Host Information |
LAB9884
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Instrument Information |
I2041
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Target Information |
CH3D DILUTED IN CH4 (METHANE) ICE
CH3D DILUTED IN N2 (NITROGEN) ICE
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