Comparison of GRUAN RS92 and RS41 Radiosonde Temperature Biases

In this study, we validated the consistency of the GRUAN RS92 and RS41 datasets, versions EDT.1 and GDP.2, in the upper troposphere and lower stratosphere (200–20 hPa), through dual launch campaigns at the GRUAN site and using the radio occultation (RO) product and the ERA5 reanalysis from ECMWF as...

Full description

Bibliographic Details
Main Authors: Xin Jing, Xi Shao, Tung-Chang Liu, Bin Zhang
Format: Article
Language:English
Published: MDPI AG 2021-06-01
Series:Atmosphere
Subjects:
Online Access:https://www.mdpi.com/2073-4433/12/7/857
_version_ 1797528142839021568
author Xin Jing
Xi Shao
Tung-Chang Liu
Bin Zhang
author_facet Xin Jing
Xi Shao
Tung-Chang Liu
Bin Zhang
author_sort Xin Jing
collection DOAJ
description In this study, we validated the consistency of the GRUAN RS92 and RS41 datasets, versions EDT.1 and GDP.2, in the upper troposphere and lower stratosphere (200–20 hPa), through dual launch campaigns at the GRUAN site and using the radio occultation (RO) product and the ERA5 reanalysis from ECMWF as standards for double difference comparison. Separate comparisons with the references were also performed in order to trace the origin of the bias between the two instruments. Then, the performance of the GRUAN raw temperature correction algorithm was evaluated, from the aspects of day–night, the solar zenith angle, and the pressure level, for GDP.2 version products. The results show that RS92.EDT.1 has a warm bias of 0.355 K, compared to RS41.EDT.1, at 20 hPa, during daytime. This bias was found to mainly originate from RS92.EDT.1, based on the separate comparison with RO or ECMWF ERA5 data. RS92.GDP.2 is consistent with RS41.GDP.2, but a separate comparison indicated that the two original GDP.2 products have a ~1 K warm bias at 20 hPa during daytime, compared with RO or ECMWF ERA5 data. The GRUAN correction method can reduce the warm bias up to 0.5 K at 20 hPa during daytime. As a result, this GRUAN correction method is efficient, and it is dependent on the solar zenith angle and pressure level.
first_indexed 2024-03-10T09:53:57Z
format Article
id doaj.art-94e6f655bb694822a66cf0191d6bae15
institution Directory Open Access Journal
issn 2073-4433
language English
last_indexed 2024-03-10T09:53:57Z
publishDate 2021-06-01
publisher MDPI AG
record_format Article
series Atmosphere
spelling doaj.art-94e6f655bb694822a66cf0191d6bae152023-11-22T02:33:16ZengMDPI AGAtmosphere2073-44332021-06-0112785710.3390/atmos12070857Comparison of GRUAN RS92 and RS41 Radiosonde Temperature BiasesXin Jing0Xi Shao1Tung-Chang Liu2Bin Zhang3Cooperative Institute for Satellite Earth System Studies (CISESS), Earth System Science Interdisciplinary Research Center, University of Maryland, College Park, MD 20740, USACooperative Institute for Satellite Earth System Studies (CISESS), Earth System Science Interdisciplinary Research Center, University of Maryland, College Park, MD 20740, USACooperative Institute for Satellite Earth System Studies (CISESS), Earth System Science Interdisciplinary Research Center, University of Maryland, College Park, MD 20740, USACooperative Institute for Satellite Earth System Studies (CISESS), Earth System Science Interdisciplinary Research Center, University of Maryland, College Park, MD 20740, USAIn this study, we validated the consistency of the GRUAN RS92 and RS41 datasets, versions EDT.1 and GDP.2, in the upper troposphere and lower stratosphere (200–20 hPa), through dual launch campaigns at the GRUAN site and using the radio occultation (RO) product and the ERA5 reanalysis from ECMWF as standards for double difference comparison. Separate comparisons with the references were also performed in order to trace the origin of the bias between the two instruments. Then, the performance of the GRUAN raw temperature correction algorithm was evaluated, from the aspects of day–night, the solar zenith angle, and the pressure level, for GDP.2 version products. The results show that RS92.EDT.1 has a warm bias of 0.355 K, compared to RS41.EDT.1, at 20 hPa, during daytime. This bias was found to mainly originate from RS92.EDT.1, based on the separate comparison with RO or ECMWF ERA5 data. RS92.GDP.2 is consistent with RS41.GDP.2, but a separate comparison indicated that the two original GDP.2 products have a ~1 K warm bias at 20 hPa during daytime, compared with RO or ECMWF ERA5 data. The GRUAN correction method can reduce the warm bias up to 0.5 K at 20 hPa during daytime. As a result, this GRUAN correction method is efficient, and it is dependent on the solar zenith angle and pressure level.https://www.mdpi.com/2073-4433/12/7/857GRUANRS92RS41radiosondeROECMWF ERA5
spellingShingle Xin Jing
Xi Shao
Tung-Chang Liu
Bin Zhang
Comparison of GRUAN RS92 and RS41 Radiosonde Temperature Biases
Atmosphere
GRUAN
RS92
RS41
radiosonde
RO
ECMWF ERA5
title Comparison of GRUAN RS92 and RS41 Radiosonde Temperature Biases
title_full Comparison of GRUAN RS92 and RS41 Radiosonde Temperature Biases
title_fullStr Comparison of GRUAN RS92 and RS41 Radiosonde Temperature Biases
title_full_unstemmed Comparison of GRUAN RS92 and RS41 Radiosonde Temperature Biases
title_short Comparison of GRUAN RS92 and RS41 Radiosonde Temperature Biases
title_sort comparison of gruan rs92 and rs41 radiosonde temperature biases
topic GRUAN
RS92
RS41
radiosonde
RO
ECMWF ERA5
url https://www.mdpi.com/2073-4433/12/7/857
work_keys_str_mv AT xinjing comparisonofgruanrs92andrs41radiosondetemperaturebiases
AT xishao comparisonofgruanrs92andrs41radiosondetemperaturebiases
AT tungchangliu comparisonofgruanrs92andrs41radiosondetemperaturebiases
AT binzhang comparisonofgruanrs92andrs41radiosondetemperaturebiases