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Observing upper troposphere-lower stratosphere climate with radio occultation data from the CHAMP satellite

机译:利用来自CHAMP卫星的无线电掩星数据观测对流层-平流层下部

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High quality observations of the atmosphere are particularly required for monitoring global climate change. Radio occultation (RO) data, using Global Navigation Satellite System (GNSS) signals, are well suited for this challenge. The special climate utility of RO data arises from their long-term stability due to their self-calibrated nature. The German research satellite CHAllenging Mini-satellite Payload for geoscientific research (CHAMP) continuously records RO profiles since August 2001 providing the first opportunity to create RO based climatologies for a multi-year period of more than 5 years. A period of missing CHAMP data from July 3, 2006 to August 8, 2006 can be bridged with RO data from the GRACE satellite (Gravity Recovery and Climate Experiment). We have built seasonal and zonal mean climatologies of atmospheric (dry) temperature, microwave refractivity, geopotential height and pressure with 10° latitudinal resolution. We show representative results with focus on dry temperatures and compare them with analysis data from the European Centre for Medium-Range Weather Forecasts (ECMWF). Although we have available only about 150 CHAMP profiles per day (compared to millions of data entering the ECMWF analyses) the overall agreement between 8 and 30 km altitude is in general very good with systematic differences < 0.5 K in most parts of the domain. Pronounced systematic differences (exceeding 2 K) in the tropical tropopause region and above Antarctica in southern winter can almost entirely be attributed to errors in the ECMWF analyses. Errors resulting from uneven sampling in space and time are a potential error source for single-satellite climatologies. The average CHAMP sampling error for seasonal zonal means is < 0.2 K, higher values occur in restricted regions and time intervals which can be clearly identified by the sampling error estimation approach we introduced (which is based on ECMWF analysis fields). The total error of this new type of temperature climatologies is estimated to be < 0.5 K below 30 km. The recently launched Taiwan/U.S. FORMOSAT-3/COSMIC constellation of 6 RO satellites started to provide thousands of RO profiles per day, but already now the single-satellite CHAMP RO climatologies improve upon modern operational climatologies in the upper troposphere-lower stratosphere and can act as absolute reference climatologies for validation of more bias-sensitive climate datasets and models.
机译:监测全球气候变化特别需要高质量的大气观测。使用全球导航卫星系统(GNSS)信号的无线电掩星(RO)数据非常适合此挑战。反渗透数据的特殊气候用途是由于它们具有自校准特性,因此具有长期稳定性。自2001年8月以来,德国研究卫星CHAllenging微型卫星有效载荷用于地球科学研究(CHAMP)连续记录反渗透剖面,这为五年以上的多年期第一个创造基于反渗透气候的机会。可以将2006年7月3日至2006年8月8日期间丢失的CHAMP数据与GRACE卫星的RO数据进行桥接(重力恢复和气候实验)。我们建立了大气(干燥)温度,微波折射率,地势高度和压力为10°纬度分辨率的季节性和纬向平均气候。我们展示了针对干燥温度的代表性结果,并将其与欧洲中距离天气预报中心(ECMWF)的分析数据进行了比较。尽管我们每天只能获取约150个CHAMP配置文件(与进入ECMWF分析的数百万数据相比),但在8公里和30公里的高度之间的总体协议通常非常好,在该领域的大部分地区,系统差异<0.5K。热带对流层顶地区和南极冬季南极洲上方明显的系统差异(超过2 K)几乎可以完全归因于ECMWF分析中的误差。由空间和时间上不均匀的采样引起的误差是单卫星气候的潜在误差源。季节性纬向平均值的平均CHAMP采样误差为<0.2 K,在受限区域和时间间隔内会出现更高的值,这可以通过我们引入的采样误差估计方法(基于ECMWF分析字段)清楚地识别出来。在30 km以下,这种新型温度气候的总误差估计为<0.5K。最近启动的台湾/美国6颗反卫星的FORMOSAT-3 / COSMIC星座开始每天提供成千上万的反卫星资料,但是现在单卫星CHAMP RO的气候状况已经改善了对流层-低平流层上方的现代运行气候,并且可以作为绝对参考气候验证更多对偏差敏感的气候数据集和模型。

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