Tropospheric Ozone Profiles From Ground-based UV Measurements
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Liu, X., K. Chance, C.E. Sioris, M.J. Newchurch, T.P. Kurosu, Tropospheric ozone profiles from a ground-based ultraviolet spectrometer: a new retrieval method, Appl. Opt., 45(10), 2352-2359, 2006. [Full text (pdf)]
The first technique for measuring O3 profiles from ground-based measurements in the UV is the Umkehr technique [Gotz, 1931, 1934], and it has been used for routine observations of O3 trends from both Dobson and Brewer instruments. In this technique, ratios of zenith-sky radiances at two wavelengths in the UV, one strongly and the other weakly O3 absorbing, are measured with the solar zenith angle varying from 60 to 90 during the twilight [Mateer and Deluisi, 1992]. Measured total O3 column from Dobson or Brewer measurements are used to constrain profiles. The Umkehr technique mainly contains information about the vertical distribution of O3 in the stratosphere, with about four independent pieces of information (i.e, significant eigenvectors) at 20-40 km [Mateer, 1965]. Only limited information is in the troposphere, which is provided by the total O3 measurement. In addition, the Umkehr observation lasts about two hours and is restricted to the sunset and sunrise periods.
We presents a new method to retrieve tropospheric O3 profiles from ground-based UV spectra in the Huggins bands (300-340 nm) at three viewing zenith angles (VZAs) using the optimal estimation technique. This method refines the idea of using diffuse radiances and direct irradiances by Jiang et al.[1997] to derive tropospheric O3 profiles in the troposphere and extends the method of Liu et al.[2004] from airborne UV spectra to ground-based spectra. Measurements are normalized to direct-sun irradiances or zenith-sky radiances, so no external solar reference is needed. Total O3 is simultaneously measured using the Dobson or Brewer method and is used to constrain the profile. The altitude-dependent, wavelength-dependent, and viewing angle-dependent photon path lengths in the troposphere and lower stratosphere provide the height-resolved O3 profiling information [Figure 1].
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Figure 1. (a) Air Mass Factors (AMFs) for direct-sun irradiance, radiances at 310 and 340 nm for zenith and three view zenith angles(VZA) (45º, 75º and 85º). (b) AMFs for normalized radiances at 300, 310, 320, 330, and 340 nm for VZAs 45º, 75º and 85º. (c) Profiles of Degrees of Freedom for Signal (DFS) using radiance spectra at VZAs 0º, 30º, 45º, 60º, 75º, 85º, and 88º, respectively. The total DFS is also shown in the parentheses. Surface albedo is assumed to be 0.1; the solar zenith angle is 45º. |
This technique measure O3 in the troposphere and lower stratosphere with vertical resolutions ranging from ~3 km near the surface to ~10 km at 20 km and could be readily combined with the Umkehr technique to measure O3 profiles both in the troposphere and the stratosphere [Figure 2, Figure 3].
This technique can be used to accurately measure diurnal variation of tropospheric ozone under remote regions as well as highly-polluted regions [Figure 4].
References
Gotz, F.W.P., Zum Strahlungsklima des Spitzbergensommers. Strahlugns-und Ozonmessungen in der Konigsbucht 1929, Gerlands Beltr, 31, 119-154, 1931.
Gotz, F.W.P., A.R. Meetham, and G.M.B. Dobson, The vertical distribution of ozone in the atmosphere, Proc. Roy. Soc. London, A145, 416-446, 1934.
Jiang, Y., Y.L. Yung, and S.P. Sander, Detection of tropospheric ozone by remote sensing from the ground, J. Quant. Spectrosc. Radiat. Transfer, 57, 811-818, 1997.
Liu, X., C.E. Sioris, K. Chance, T.P. Kurosu, M.J. Newchurch, R.V. Martin, and P.I. Palmer, Mapping tropospheric ozone profiles from an airborne UV/Visible spectrometer, submitted to Appl. Opt., 2004.
Mateer, C.L., On the information content of Umkehr observations, J. Atmos. Sci., 22, 370-381, 1965.
Mateer, C.L., and J.J. DeLuisi, A new Umkehr inversion algorithm, J. Atmos. Terr. Phys., 54, 537-556, 1992.
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Last updated on 04/04/2006 .