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91探花
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Anu Dudhia

University Research Lecturer

Sub department

  • Atmospheric, Oceanic and Planetary Physics
Anu.Dudhia@physics.ox.ac.uk
Robert Hooke Building, room S50
  • About
  • Publications

An optimized forward and retrieval model for MIPAS near real time data processing

Proceedings of SPIE - The International Society for Optical Engineering 3501 (1998) 170-185

Authors:

M Ridolfi, B Carli, M Carlotti, A Dudhia, JM Flaud, M H枚pfner, PE Morris, P Raspollini, G Stiller, RJ Wells

An optimized forward and retrieval model for MIPAS near real time data processing

P SOC PHOTO-OPT INS 3501 (1998) 170-185

Authors:

M Ridolfi, B Carli, M Carlotti, A Dudhia, JM Flaud, M Hopfner, PE Morris, P Raspollini, G Stiller, RJ Wells

Abstract:

The infrared emission limb sounder MIPAS (Michelson Interferometer for Passive Atmospheric Sounding) will be operated as an ESA core instrument on the ENVISAT-1 satellite. Near real time retrieval of pressure, temperature (p,T) and volume mixing ratio (VMR) of five key species (O-3, H2O, N2O, CH4, and HNO3) from calibrated spectra will be performed in the Level 2 processor of the ENVISAT Payload Data Segment. In order to develop an optimized (with respect to speed and accuracy) retrieval algorithm suitable for the implementation in MIPAS Level 2 processor, an ESA 91探花ed study is being carried out. In the framework of this study, an optimized forward / retrieval code based on the global fit approach was implemented. In this approach all the spectra of a limb-scanning sequence are simultaneously fitted, so that error propagation in the altitude domain is avoided.The attained accuracy performances of the retrieval code are the following:Temperature error < 2 K at all the altitudes covered by the standard MIPAS scan (8-53 km)Tangent pressure error: < 3%Error on the retrieved VMR of the key species: < 5 % at most of the altitudes of scientific interest covered by the standard MIPAS scan.The run-time required to perform p,T and VMR retrieval of the five MIPAS target species from a limb-scanning sequence of 16 limb-views is less than 6 minutes on a SUN SPARCstation 20. The most effective code optimizations were implemented in the radiative transfer model and in the computation of the jacobian of the retrieval.

Evidence of non-LTE in the CO2 15 渭m weak bands from ISAMS and WINDII observations

Geophysical Research Letters 24:4 (1997) 361-364

Authors:

M L贸pez-Puertas, A Dudhia, MG Shepherd, DP Edwards

Abstract:

An analysis of the measurements of the CO2 15 渭m radiance emission by the UARS/ISAMS 30W channel and the kinetic temperature from UARS/WINDII taken on July 21, 1992 at northern latitudes around the mesopause is presented. The modeling of the measurements clearly show evidence of non-LTE emissions in the CO2(v2=1) levels of the minor isotopes 636, 628, and 627 in the 70-90 km region. A comparison with non-LTE model predictions by L贸pez-Puertas et al. [1992a] shows a good agreement within the errors in the measured quantities. This constitutes the first experimental evidence of non-LTE emissions in these CO2 15 渭m weak bands. The measurements also represent indirect evidence of the net radiative heating produced by these bands around the summer mesopause.

Upper mesosphere temperatures in summer: WINDII observations and comparisons

Geophysical Research Letters 24:4 (1997) 357-360

Authors:

MG Shepherd, A Dudhia, M L贸pez-Puertas, WFJ Evans

Abstract:

Atmospheric temperature measurements from the Wind Imaging Interferometer (WINDII) on the Upper Atmosphere Research Satellite (UARS), determined from the observed Rayleigh scattering are presented. Infrared radiances predicted from these profiles are compared with measurements from the Improved Stratospheric and Mesospheric Sounder on UARS for nine cases of spatial and temporal coincidence with an effective difference of about 5-10 K in the height range 70-85 km. A comparison with monthly averaged SME results and Rayleigh lidar temperature observations at mid-latitudes taken 8 years earlier indicated that WINDII temperatures were cooler on average by 10 K; this is consistent with a temperature decrease of 1.5 K/year inferred from the SME and lidar results. At high latitudes the agreement between falling spheres and WINDII was found to be very good.

Reference Model for Methane and Nitrous Oxide

Advances in Space Research 18:9-10 (1996) 91-124

Authors:

FW Taylor, A Dudhia, CD Rodgers

Abstract:

Data from the Stratospheric and Mesospheric Sounder (SAMS) on Nimbus 7 have been used as the basis for a model of the abundances of nitrous oxide and methane in the stratosphere. The model is presented in tabular form on seventeen pressure surfaces from 20 to 0.1-mb, in 10掳 latitude bins from 50掳S to 70掳N, and for each month of the year. Some details of the acquisition of the data which went into the model, its limitations, and the general behaviour of methane and nitrous oxide in the middle atmosphere are given. Formal errors in the data and other uncertainties, interannual variability, and systematic trends are discussed. As expected, no trends which exceed the estimated error in the data are found in either methane or nitrous oxide over the five-year period of SAMS observations.

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