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首页> 外文期刊>The Cryosphere Discussions >Combined SMAP–SMOS thin sea ice thickness retrieval
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Combined SMAP–SMOS thin sea ice thickness retrieval

机译:SMAP–SMOS组合薄海冰厚度反演

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The spaceborne passive microwave sensors Soil Moisture Ocean Salinity (SMOS) and Soil Moisture Active Passive (SMAP) provide brightness temperature data in the L band (1.4?GHz). At this low frequency the atmosphere is close to transparent and in polar regions the thickness of thin sea ice can be derived. SMOS measurements cover a large incidence angle range, whereas SMAP observes at a fixed 40 sup°/sup incidence angle. By using brightness temperatures at a fixed incidence angle obtained directly (SMAP), or through interpolation (SMOS), thin sea ice thickness retrieval is more consistent as the incidence angle effects do not have to be taken into account. Here we transfer a retrieval algorithm for the thickness of thin sea ice (up to 50?cm) from SMOS data at 40 to 50 sup°/sup incidence angle to the fixed incidence angle of SMAP. The SMOS brightness temperatures (TBs) at a given incidence angle are estimated using empirical fit functions. SMAP TBs are calibrated to SMOS to provide a merged SMOS–SMAP sea ice thickness product. The new merged SMOS–SMAP thin ice thickness product was improved upon in several ways compared to previous thin ice thickness retrievals. (i)?The combined product provides a better temporal and spatial coverage of the polar regions due to the usage of two sensors. (ii)?The radio frequency interference (RFI) filtering method was improved, which results in higher data availability over both ocean and sea ice areas. (iii)?For the intercalibration between SMOS and SMAP brightness temperatures the root mean square difference (RMSD) was reduced by 30?% relative to a prior attempt. (iv)?The algorithm presented here allows also for separate retrieval from any of the two sensors, which makes the ice thickness dataset more resistant against failure of one of the sensors. A new way to estimate the uncertainty of ice thickness retrieval was implemented, which is based on the brightness temperature sensitivities.
机译:星载无源微波传感器土壤水分海洋盐度(SMOS)和土壤水分有源无源(SMAP)提供L波段(1.4?GHz)的亮度温度数据。在这种低频下,大气层接近于透明,并且在极地地区,可以得出稀薄的海冰的厚度。 SMOS测量覆盖较大的入射角范围,而SMAP则以固定的40 °入射角进行观测。通过使用直接获得的固定入射角(SMAP)或通过插值(SMOS)的亮度温度,稀薄的海冰厚度反演更加一致,因为不必考虑入射角的影响。在这里,我们将入射角为40至50 °的SMOS数据中的薄海冰厚度(最大50?cm)的检索算法转换为SMAP的固定入射角。使用经验拟合函数估算给定入射角下的SMOS亮度温度(TBs)。 SMAP TB已根据SMOS进行了校准,以提供合并的SMOS–SMAP海冰厚度产品。与以前的薄冰厚度取回相比,新合并的SMOS–SMAP薄冰厚度产品得到了一些改进。 (i)由于使用了两个传感器,组合产品提供了更好的极地时间和空间覆盖率。 (ii)改进了射频干扰(RFI)过滤方法,这使得海洋和海冰区域的数据可用性更高。 (iii)对于SMOS和SMAP亮度温度之间的相互校准,相对于先前的尝试,均方根差(RMSD)降低了30%。 (iv)此处介绍的算法还允许从两个传感器中的任何一个单独进行检索,这使得冰厚度数据集更能抵抗其中一个传感器的故障。基于亮度温度敏感性,实现了一种新的估计冰厚反演不确定性的方法。

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