根据第一段The intrepid Voyager 1 and 2 space-crafts were launched in 1977, and despite having a roughly 12—year mission lifespan,(选项B同义替换) are still hurtling through space and returning data to eager scientists on Earth(选项A同义替换). They’ve broken through barrier...and are now ...
In 1977, two spacecraft calledVoyager 1 and Voyager 2 were sent out to explore the s___system. (根据首字母单词拼写) 相关知识点: 试题来源: 解析 答案: solar/olar详解: 考查形容词。 句意:1977年,两艘名为旅行者1号和 旅行者2号的宇宙飞船被发射出去探索太阳系。 根据 单词首字母可知, 这里需要...
【Voyager | 旅行者号】旅行者1号和2号是由NASA在1977年发射的两枚空间探测器,主要目的是探索太阳系内的其它行星及其卫星。在顺利完成任务之后逐渐远离太阳系,1号与2号分别于2012年和2018年进入星际空间。除了...
Voyager 1 has recently crossed the boundary of our solar system and passed into interstellar space, and Voyager 2 is likely to follow suit, on a different path, between 2016 and 2017. The two Voyager probes will continue to transmit details of discoveries beyond our solar system until at leas...
Izmodenov, V., Gloeckler, G., Malama, Y., 2003, "When Will Voyager 1 and 2 Cross the Termi- nation Shock?", Geophys. Res. Lett., 30, 1351-1354 2.3V. Izmodenov, G. Gloeckler, Y. Malama, When will Voyager 1 and 2 cross the termi- nation shock? 30 (2003) 3-1....
HARD-2-FIND! Part of an 11-title series of audio discs recorded by NASA with specially designed recording instruments on board Voyagers 1 & 2, which picks up electromagentic vibrations, interactions between the Solar Wind and magnetosphere of planets, moons and even the rings of planets! These...
In 1977, two spacecraft called Voyager 1 and Voyager 2 were sent out to explore the solar system. 1. 第一个空格需要填入动词,构成完整的句子。 2. “Voyager 1 and Voyager 2”是“two spacecraft”的名字,两者之间是过去分词作后置定语的关系,所以空格处应填入“call”的过去分词形式“called”。 3...
Ness, Large-scale distant heliospheric magnetic field: Voyager 1 and 2 observations from 1986 through 1989, J. Geophys. Res., 98, 17,415, 1993.Burlaga, L. F. and Ness, N. F. (1993). Large-scale distant heliospheric magnetic field: Voyager 1 and 2 observations from 1986 through 1989....
Using Voyager 1 and 2 energetic ( 30 keV) ion measurements near the magnetopause, in the magnetosheath, and immediately upstream of the bow shock, we examine the compositional patterns together with typical energy spectra in each of these regions. We find characteristic spectral changes late in ...
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