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Sea surface signature of tropical cyclones using microwave remote sensing

机译:使用微波遥感的热带气旋海表面签名

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Measuring the sea surface during tropical cyclones (TC) is challenging due to severe weather conditions that prevent shipboard measurements and clouds which mask the sea surface for visible satellite sensors. However, sea surface emission in the microwave L-band can penetrate rain and clouds and be measured from space. The European Space Agency (ESA) MIRAS L-band radiometer on the Soil Moisture and Ocean Salinity (SMOS) satellite enables a view of the sea surface from which the effects of tropical cyclones on sea surface emissivity can be measured. The emissivity at these frequencies is a function of sea surface salinity (SSS), sea surface temperature (SST), sea surface roughness, polarization, and angle of emission. If the latter four variables can be estimated, then models of the sea surface emissivity can be used to invert SSS from measured brightness temperature (T_B). Actual measured T_B from space also has affects due to the ionosphere and troposphere, which have to be compensated for, and components due to the galactic and cosmic background radiation those have to be removed. In this research, we study the relationships between retrieved SSS from MIRAS, and SST and precipitation collected by the NASA TMI sensor from the Tropical Rainfall Measuring Mission (TRMM) satellite during Hurricane Isaac, in August 2012. During the slower movement of the storm, just before landfall on the vicinity of the Louisiana Shelf, higher precipitation amounts were associated with lower SSS and slightly increased SST. This increased trend of SST and lower SSS under regions of high precipitation are indicative of inhibited vertical mixing. The SMOS Level 2 SSS were filtered by a stepwise process with removal of high uncertainty in T_B under conditions of strong surface roughness which are known to create noise. The signature of increased SST associated with increasing precipitation was associated with decreased SSS during the storm. Although further research is required, this study shows that there is a T_B signal from the sea surface beneath a tropical cyclone that provides information on roughness and salinity.
机译:在热带气旋(TC)期间测量海面是挑战,由于防止船舶测量和遮蔽海面的船舶测量和遮蔽可见卫星传感器的云。然而,微波L波段的海面发射可以穿透雨和云并从空间测量。欧洲航天局(ESA)Miras L波段辐射计在土壤水分和海洋盐水(SMOS)卫星上,可以测量热带气旋在海面发射率上的海面视图。这些频率的发射率是海表面盐度(SSS),海表面温度(SST),海表面粗糙度,极化和发射角度的函数。如果可以估计后四个变量,则海面发射率的模型可用于反转SSS从测量的亮度温度(T_B)。来自空间的实际测量T_B也存在由于电离层和对流层引起的影响,这必须被补偿,并且由于银河系和宇宙背景辐射而导致的部件必须被移除。在这项研究中,我们在2012年8月期间研究了来自热带降雨测量任务(TRMM)卫星的NASA TMI传感器从Miras和NASA TMI传感器收集的SST和降水之间的关系。在暴风雨的速度较慢,就在路易斯安那架附近的登陆前,较高的降水量与较低的SSS相关,SST略微增加。在高沉淀区域下SST和下SSS的这种趋势增加了抑制垂直混合。通过逐步处理SMOS 2 SSS,通过在众所周知的强大的表面粗糙度下除去T_B的高不确定性,这是已知产生噪声的。与沉淀增加相关的SST增加的签名与风暴期间的SSS降低有关。虽然需要进一步研究,但本研究表明,来自海面的热带气旋中有一个T_B信号,提供有关粗糙度和盐度的信息。

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