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Overview of Oxford MIPAS Cloud Products 

Jane Hurley, Anu Dudhia, Don Grainger University of Oxford. Overview of Oxford MIPAS Cloud Products . Aim to retrieve most obvious macrophysical cloud properties: Cloud Top Height CTH (relative to instrument pointing) ‏ Cloud Top Temperature CTT Cloud Extinction Coefficient k ext.

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Overview of Oxford MIPAS Cloud Products 

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  1. Jane Hurley, Anu Dudhia, Don Grainger University of Oxford Overview of Oxford MIPAS Cloud Products 

  2. Aim to retrieve most obvious macrophysical cloud properties: • Cloud Top Height CTH (relative to instrument pointing)‏ • Cloud Top Temperature CTT • Cloud Extinction Coefficient kext

  3. Cloud Forward Model (CFM): Radiance in MIPAS FOV Assume that: a cloud in the MIPAS FOV is horizontally homogeneous – that is, has a constant cloud top height across the FOV and can be characterized by a single extinction coefficient. the temperature structure within the cloud can be determined by the wet adiabatic lapse rate estimated downwards from the cloud top temperature.

  4. The radiance is considered in the clearest microwindow of the MIPAS A band: 960 cm-1 – 961 cm-1 ... has been tried with other microwindows ... O3 & CO2 O3 & CO2 O3 O3 O3 O3 & NH3 O3

  5. Gas Correction and Validation with Simulations Real MIPAS measurements Rm will include significant gaseous radiation contributions Rg, while the CFM calculates only the radiation contribution by the cloud itself Rc. It is thus necessary to deduce what portion of the measured signal is due to the cloud. Assume that the cloud has a continuum signal and that the gaseous contribution has emission/absorption lines.

  6. Total radiance measured within two MIPAS FOVs (the FOV containing the cloud top and the FOV immediately below) calculated by the CFM for varying cloud top heights and extinction coefficients.

  7. Retrieval and A Priori Dependence • Cloud modelling is a highly non-linear process, even when considered on the vastly simplified scale. • Given a pair of radiances from two adjacent sweeps in a scan pattern, there can be two possible clouds present: a high thin cloud, or a low thick cloud. • Depending upon which a priori is supplied to an OER, equally valid different solutions will result. • NEED TO ADD MORE INFORMATION, to better characterize the a priori extinction. Easiest way to get information is to use quantity we already have: THE COLOUR INDEX CI which should already be highly correlated with Cloud Effective Fraction EF, which is the ‘effective blocking power’ of the cloud in the FOV.

  8. Optimal Estimations retrieval of form with state vector and using: Real Measurements: 2 radiance measurements from MIPAS spectrum – the first sweep flagged as cloudy and the one immediately below DIRECT Pseudo-Measurements: Tret = temperature corresponding to first flagged cloudy sweep EF = Cloud effective fraction, as estimated from CI RELATE

  9. Application to MIPAS Spectra • “Hot spot” of high cloud over Indonesian toga core, mountainous regions such as the Southern Andes and Rockies, Amazon Basin and the Congo; • Increasing cloud top height towards the tropics; • Retrieved CTT is nearly fully correlated with CTH; • Retrieved log(kext) is more or less constant over the globe.

  10. If there IS a cloud in the FOV at a certain latitude, this shows the probability that it will occur at a given altitude …

  11. If there IS a cloud in the FOV at a certain latitude, this shows the probability that it will occur at a given temperature … • Basically anti-correlated with cloud top height/altitude

  12. If there IS a cloud in the FOV at a certain latitude, this shows the probability that it will have a given extinction …

  13. Future Work • Check retrieval against other retrievals of macroscopic properties: McClouds etc • Run over larger MIPAS dataset to get a high cloud climatology • Compare high cloud climatology with others: ISCCP etc

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