發(fā)布時間：2022-01-10 06:11

　　An overall bi-directional panoramic solar system exploration activity, not just looking at the solar system at a macro level and helping to build a simulation model for the solar system, but the probe will also be able to explore the Milky Way and the vast universe from a much wider perspective. By observing the characteristics of the solar system, solar wind, ionization envelope and other parameters from a bi-directional panorama on both sides of the solar ecliptic plane, it will assist the sci... 

【文章來源】：Aerospace China. 2019,20(02)

【文章頁數(shù)】：7 頁

【文章目錄】：
1 INTRODUCTION
    1.1 Necessity and Inevitability of Detection
    1.2 Purpose of the Observation
    1.3 Targets of the Observation
2 OVERALL BI-DIRECTIONAL PANORAMIC EX-PLORATION OF THE SOLAR SYSTEM
    2.1 The Existing Basis
        2.1.1 Measuring means
        2.1.2 The international situation
        2.1.3 Measurement and control ability
    2.2 Cooperation Opportunities
        2.2.1 Rich cooperation contents
        2.2.2 Seeking international cooperation
    2.3 Navigation Mode
        2.3.1 Basic definition of launch direction
        2.3.2 Detection method 1:navigation referenced on the polestar and south pole star
        2.3.3 Detection method 2:navigation referenced on the constellations directly above or below the sun
        2.3.4 Detection method 3:Launch solar and galactic satel-lites
    2.4 Launch Timing
        2.4.1 Timing of launch above the ecliptic plane
        2.4.2 Timing of launch below the ecliptic plane
    2.5 Requirements
        2.5.1 Implementation difficulty analysis
        2.5.2 Speed requirement
        2.5.3 Innovative navigation method
    2.6 Influence Factors
        2.6.1 The influence of aphelion and perihelion
        2.6.2 The influence of solar motion
        2.6.3 Influence of solar wind and strong magnetic field
    2.7 Predicting Results
3 IMPLEMENTATION STEPS
4 CONCLUSION


【參考文獻】：
期刊論文
[1]航天技術(shù)與甚長基線陣的結(jié)合探索[J]. 吳志敏,華均康.  科學. 2020(05)



本文編號：3580190