...
首页> 外文期刊>Journal of Geophysical Research, D. Atmospheres: JGR >Characteristics of the double intertropical convergence zone over the tropical Indian Ocean
【24h】

Characteristics of the double intertropical convergence zone over the tropical Indian Ocean

机译:热带印度洋上热带双热带辐合带的特征

获取原文
获取原文并翻译 | 示例
   

获取外文期刊封面封底 >>

       

摘要

Investigations on the double intertropical convergence zone (DITCZ) over the Indian Ocean using the monthly mean surface wind divergence data obtained from scatterometers on board the ERS-1/2 and QuikSCAT satellites (1991–2005) and the monthly mean cloud amount obtained from the International Satellite Cloud Climatology Project (1988–1989, 1998–2005) and the Advanced Very High Resolution Radiometer (AVHRR) data (1996–2003) reveal that its frequency of occurrence is considerably larger than that reported earlier, though the DITCZ feature in this region is rather diffused compared to Pacific. The 14-year analysis of monthly mean surface wind divergence shows that DITCZ structure is clearly discernible in April (frequency of occurrence, f = 64%), November (f = 73%) and December (f = 60%) in the 50–85°E longitude band over the tropical Indian Ocean. Though less frequent, DITCZ occur during other months also, except the Asian summer monsoon season. Most preferred latitudes of the north and south bands of DITCZ are ~6°N and ~7°S, respectively, during November and December. The DITCZ structure is well manifested in the cloud amount also during November and December, while it is less prominent in April. A weak but clearly identifiable hemispherical asymmetry is observed in latitude of occurrence and amplitude of the DITCZ bands. Since the sea surface temperature (SST) at the equatorial region over the Indian Ocean is nearly uniform, the DITCZ appears to be generated mainly by the atmospheric dynamics. This provides a unique opportunity to investigate the structure of ITCZ created by the atmospheric dynamics alone, which is one of the important problems in ITCZ dynamics.
机译:使用从ERS-1 / 2和QuikSCAT卫星上的散射仪获得的月平均地表风散度数据(1991-2005年)以及从月球获得的月平均云量,对印度洋上的双热带辐合带(DITCZ)进行调查。国际卫星云气候学项目(1988–1989、1998–2005)和高级超高分辨率辐射计(AVHRR)数据(1996–2003)揭示了它的发生频率比以前报道的要大得多,尽管该区域具有DITCZ功能与太平洋地区相比,该地区分布较为分散。对月平均表面风向散度的14年分析表明,在50–50年间,DITCZ的结构在4月(发生频率,f = 64%),11月(f = 73%)和12月(f = 60%)清晰可见。热带印度洋上的85°E经度带。尽管不那么频繁,但除亚洲夏季风季节外,DITCZ也发生在其他月份。在11月和12月,DITCZ北部和南部最优选的纬度分别是北纬6°和南纬7°。 DITCZ结构在11月和12月的云量中也很明显,而在4月则不那么明显。在DITCZ波段的出现纬度和振幅中观察到了一个微弱但可明确识别的半球不对称性。由于印度洋赤道区域的海表温度(SST)几乎是均匀的,因此DITCZ似乎主要是由大气动力学产生的。这提供了一个独特的机会来研究仅由大气动力学产生的ITCZ的结构,这是ITCZ动力学中的重要问题之一。

著录项

相似文献

  • 外文文献
  • 中文文献
  • 专利
获取原文

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号