Analysis of Halogen Occultation Experiment HF versus CH 4 correlation plots: Chemistry and transport implications
Author(s) -
Luo M.,
Cicerone R. J.,
Russell J. M.
Publication year - 1995
Publication title -
journal of geophysical research: atmospheres
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.67
H-Index - 298
eISSN - 2156-2202
pISSN - 0148-0227
DOI - 10.1029/95jd00621
Subject(s) - polar vortex , solstice , zonal and meridional , atmospheric sciences , latitude , occultation , atmosphere (unit) , altitude (triangle) , halogen , climatology , stratosphere , physics , chemistry , geology , meteorology , astrophysics , geodesy , geometry , alkyl , mathematics , organic chemistry
The relationship between stratospheric CH 4 and Hydrogen Fluoride (HF) observed simultaneously by the Halogen Occultation Experiment (HALOE) on the Upper Atmosphere Research Satellite (UARS) has been examined globally. The meridional structures of the two long‐lived species for the equinox and solstice seasons are found to be very similar. Their surfaces of constant mixing ratio, however, are found to not quite coincide. The isopleth of CH 4 graphed as pressure versus latitude shows a steeper slope than that of HF. This feature can be clearly seen from the scatterplots of CH 4 versus HF for a sequence of latitude regions. In general, CH 4 ‐HF correlation plots are characterized by tightly fitted curves for different latitude bands; curves for the tropics and high latitudes define the envelope for the correlations. The NCAR two‐dimensional model simulation of CH 4 and HF agrees well with HALOE observations, and it shows that the altitude‐latitude dependences of CH 4 removal and HF production rates play an important role in determining global CH 4 ‐HF correlations. It is found that the CH 4 ‐HF correlation inside the Antarctic vortex is nearly linear and is shifted from that of outside the vortex and from that of polar late‐summer before the formation of the vortex. HALOE observations of CH 4 and HF indicate that the two species are not in states of perfect “slope equilibrium” or “gradient equilibrium” globally. The obvious shift of HF values on CH 4 surfaces or vice versa is usually found across dynamical barriers. There is no universal relationship between CH 4 and HF. The HF mixing ratios are observed to change up to 20–35% for a given CH 4 from different dynamically isolated regions such as the polar vortex, midlatitudes, and the tropics, and the same magnitudes of change in CH 4 could also be found for a fixed HF. Therefore one must be cautious in the usage of correlation‐inferring methods for any pair of tracers in place of unavailable measurements or for evaluating chemical disturbances.
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