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METHOD OF PREDICTION OF PARAMETERS OF SOLAR WIND AT LEVEL OF ORBIT OF THE EARTH

机译:预测地球轨道上太阳风参数的方法

摘要

Uses: studies communication parameters interplanetary medium with the condition geomagnitosfery and geomagnetic field having an effect on human health and performance of technical systems creates them SUMMARY OF THE INVENTION, solar wind parameters are recorded spacecraft (SC) mounted on the distances D from Earth greater than the distance to front point libration. In this moving spacecraft in interplanetary space and retaining it in the selected area is accomplished by using a force of pressure of sunlight on the surface is yuschuyus part Ka (sail) and oriented so that the vector of the solar wind pressure directed quasi-normal (from the sun) Registered satellite parameters solar wind will be observed at the level geomagnitosfery after a time interval t D / v, where v - rate of the solar wind forecast This zablagovremen- NOSTA t can be 8 hours or more that allows interested offices podgotovits possible disastrous consequences to the m strongest geomagnetic disturbances Thus sailing spacecraft can be placed in this manner. which compensates for the movement of the Earth in interplanetary space for the propagation time of the solar wind of spacecraft to geomagnitosfere that ensures the accuracy of prediction for the solar wind conditions prevent the AC bias from the initial position under the influence of the component the force of attraction can be balanced component light pressure force generated rotated for some sails or portions thereof relative orientation quasinormal 2zpf-ly. 4 yl y V & amp; amp; JS 1
机译:用途:研究地球物理条件和地磁场对人类健康和技术系统性能有影响的条件下的行星际通信参数,发明概述,太阳风参数记录在航天器(SC)上,距地球的距离D大于到前端解放的距离。在这种在行星际空间中移动的航天器中并将其保留在选定区域中是通过使用太阳表面上的太阳压力yuschuyus部分Ka(帆)并使其取向成使太阳风压力的矢量指向准法线(时间间隔t D / v之后,将在地磁观测层观测到已注册的卫星参数太阳风,其中v-太阳风的预报速率。这个zablagovremen- NOSTA t可以为8小时或更长时间,从而使感兴趣的办公室可以进行工作对m个最强烈的地磁干扰可能造成的灾难性后果因此,可以这种方式放置航行中的航天器。它可以补偿地球在行星际空间中的运动,从而使航天器的太阳风传播到地磁反射器,从而确保了对太阳风条件的预测精度,从而防止了在力的作用下交流偏置从初始位置开始吸引力的平衡可以是针对某些风帆或其部分相对于准垂直2zpf-ly旋转而旋转的分量光压力。 4 yl y V&放大器; amp; JS 1

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