首页> 外文会议>NATO Advanced Study Institute on Sprites, Elves and Intense Lightning Discharges; 20040724-31; Corte(FR) >OBSERVATIONS OF SPRITES FROM SPACE AT THE NADIR: THE LSO (LIGHTNING AND SPRITE OBSERVATIONS) EXPERIMENT ON BOARD OF THE INTERNATIONAL SPACE STATION
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OBSERVATIONS OF SPRITES FROM SPACE AT THE NADIR: THE LSO (LIGHTNING AND SPRITE OBSERVATIONS) EXPERIMENT ON BOARD OF THE INTERNATIONAL SPACE STATION

机译:纳迪尔太空中的星云观测:国际空间站上的LSO(闪电和星云观测)实验

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The experiment LSO (Lightning and Sprite Observations) on board of the International Space Station is the first experiment dedicated to sprite observations at the nadir. Such observations are difficult because the luminous emissions of sprites and lightning can be superimposed when they are observed from space at the nadir. Such observations are however needed for measuring simultaneously all possible emissions (radio, X-γ, high energy electrons) associated with sprites for a better understanding of the implied mechanisms. They are possible in specific spectral lines where sprites are differentiated from lightning. Absorption bands of the atmosphere are well adapted for this differentiation because the light emissions from sprites occurring in the middle and upper atmosphere are less absorbed in these bands than lightning emissions occurring more deeply in the atmosphere. The most intense spectral emission band of the sprites, corresponding to the N_21P band at 761 nm, partly superimposed with the oxygen absorption A band of the atmosphere, is used by the LSO experiment. The experiment is composed of two micro-cameras, one in the visible and near infra red, the other equipped with an adapted filter. Only sprites, halos and super-bolts, which correspond to a class of rare very intense lightning, are transmitted through the filter. Sprites, halos and superbolts are identified by the ratio of the intensities received through the filter and in the whole spectrum. This ratio is lower for superbolts than for sprites and halos. The response of the sprites is also more complex and variable than the response of superbolts which is very flat and comparable from an event to another. Finally, LSO observed 17 sprites, 3 halos and 9 superbolts. Several examples of differentiation of sprite and super-bolts are given. The results of a first global statistical study are also presented.
机译:国际空间站上的LSO(闪电和雪碧观测)实验是第一个致力于在最低点进行雪碧观测的实验。这种观察是困难的,因为从天底的太空观察时,可以将子画面和闪电的发光叠加在一起。然而,需要这样的观察来同时测量与子画面相关的所有可能的发射(无线电,X-γ,高能电子),以便更好地理解隐含的机理。它们在特定的光谱线中是可能的,在这些光谱线中,精灵与闪电有所区别。大气的吸收带非常适合此区分,因为与在大气中更深处发生的雷电发射相比,在中层和高层大气中发生的精灵发出的光在这些吸收带中的吸收较少。 LSO实验使用了精灵的最强光谱发射带,对应于761 nm的N_21P带,部分与大气的氧吸收A带重叠。该实验由两台微型相机组成,一个在可见光和近红外光下,另一个则装有自适应滤镜。只有与一类罕见的非常强烈的闪电相对应的精灵,光晕和超螺栓才能通过过滤器传输。子画面,光晕和超级螺栓通过通过滤波器接收的强度与整个光谱之比来识别。超级螺栓的这个比率低于精灵和光环。与超级螺栓的响应相比,子画面的响应也更加复杂和可变,而超级螺栓的响应非常平稳,并且可以在事件之间相互比较。最后,LSO观测到17个精灵,3个光环和9个超螺栓。给出了区分精灵和超级螺栓的几个例子。还介绍了第一个全球统计研究的结果。

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