Abstract
This paper proposes a method to retrieve the land surface bidirectional reflectivity ρb in the mid‐infrared (MIR) from MODIS channels 22 and 23. A split‐window‐like algorithm was developed to determine the MIR ground brightness temperature without the contribution of the solar direct beam from ground brightness temperatures measured at two adjacent MIR channels. Comparing the actual values of ρb with those estimated using our proposed method, the root mean square error (RMSE) was determined to be 0.0022 for the solar zenith angle (SZA) at nadir. Similar results were obtained for other SZAs, indicating that the proposed method can retrieve ρb accurately. A detailed sensitivity analysis found that the effects of instrumental noise, variations in water vapour content in the atmosphere, and reasonable variations in horizontal visibility on the retrieval of ρb were negligible and an error of 1 K on the ground brightness temperature caused by the inaccuracy of atmospheric corrections can lead to a maximum error of 0.034 on the retrieved ρb. We compared the use of radiosonde data and European Centre for Median‐range Weather Forecast (ECMWF) atmospheric data to perform atmospheric corrections. The results show that atmospheric corrections can be performed with ECMWF data instead of radiosonde data without losing the accuracy of the retrieved ρb. MODIS land surface temperature/emissivity product MOD11B1 data were also used to validate
. Comparison of
estimated respectively with the proposed method and with MOD11B1 data showed that the RMSE is less than 1 K for cloud‐free skies.
Acknowledgements
We thank Drs Z. Wan and F. Nerry for providing some helpful suggestions, and the anonymous reviewers for their valuable comments. This work was supported by the National Natural Science Foundation of China under Grant 4042501 and the ‘Hundred Talent’ programme of the Chinese Academy of Science.