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首页> 外文期刊>Revista Brasileira de Meteorologia >Taxa de absor??o atmosférica sobre as cidades de Botucatu-SP e Rio de Janeiro-RJ
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Taxa de absor??o atmosférica sobre as cidades de Botucatu-SP e Rio de Janeiro-RJ

机译:Botucatu-SP和Rio de Janeiro-RJ城市的大气吸收率

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The second satellite of the Brazilian Complete Space Mission (SCD2/MECB) was launched on October 23, 1998 and it hosts on board a solar cell experiment. Silicon solar cell is a semiconductor device that senses visible and near infrared (400-1100 nm) radiations. The experiment permits the simultaneous inference of direct insolation and the insolation that is reflected outside of Earth. The data of the solar cell experiment are transmitted in real time by the satellite telemetry and are received by the ground station of Cuiabá, MT-Brazil (16°S, 56°W). This fact limits their spatial coverage to a circle on the South America. The planetary albedo is obtained inside this coverage area and the data can be grouped into periods of time (annual, seasonal or monthly) or studied for several places (latitude and longitude) during the life of the satellite. Atmospheric transmission coefficient or clearness index (Kt), measured at meteorological stations around the Earth surface, together with simultaneous measured of the planetary albedo permits to calculate the atmospheric absorption coefficient (Ka). The developed method in this work for evaluating the Ka considers that the planetary albedo is composed by two parts: the local and the non local reflectivity. Considering this new concept, an atmospheric absorption ratio (called here Ra) is defined as the quotient between Ka and the net solar irradiance power that is not transmitted through the atmosphere (100%-Kt). The atmospheric absorption ratio defined by this way is not cloud cover dependent. The frequency histogram of Ra indicates the values of 0.86±0.07 and 0.88±0.09 on the cities of Botucatu-SP and Rio de Janeiro-RJ respectively, during the years of 1999 to 2006.
机译:1998年10月23日,巴西完成太空任务(SCD2 / MECB)的第二颗卫星发射升空,并在其上进行了太阳能电池实验。硅太阳能电池是一种半导体器件,可感应可见和近红外(400-1100 nm)的辐射。实验允许同时推断直接日照和反射到地球外部的日照。太阳电池实验的数据通过卫星遥测实时传输,并由巴西MT-Cuiabá地面站接收(16°S,56°W)。这个事实将它们的空间覆盖范围限制在南美。可以在该覆盖区域内获得行星反照率,并且可以将数据分组为一段时间(每年,季节性或每月),或者在卫星生命周期内针对多个位置(经度和纬度)进行研究。在地球表面附近的气象站测量的大气传输系数或净度指数(Kt),以及同时测量的行星反照率,可以计算出大气吸收系数(Ka)。在这项工作中开发的评估钾的方法认为,行星反照率由两部分组成:局部反射率和非局部反射率。考虑到这一新概念,将大气吸收率(在此称为Ra)定义为Ka与不通过大气传输的净太阳辐照功率之间的商(100%-Kt)。用这种方法定义的大气吸收率与云量无关。 Ra的频率直方图分别表示Botucatu-SP和Rio de Janeiro-RJ的城市在1999年至2006年期间的值为0.86±0.07和0.88±0.09。

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