Oak city 建了个shopping mall,是个mistake,local business failed了很多,当地的parking lot 不够了,且arrest的crime和vagrancy多了。所以Elm city也不能建。 Should a society be measured more by the scientific and artistic achievements than by businesses successes.
阅读:
机经里的2.2.3测量误差题,说management error是啥啥啥,前面貌似没啥题。 第二段说Thomas做实验,发现说陆地上记录到的温度和海洋记录到的温度差了0.5度。【这里有一道题,问说出现这个问题之后,which of the following initially suggested。。。就是说Thomas这个人立马想到了啥,文中说这个人立马想到了management error,答案里我选的是:有个different location结尾的选项。】 第三段解释说1945年啊,wartime之前和wartime之后是米国和英国人记的【前后顺序忘了,不影响做题】,后来有道题问说,如果1945年,科学家们做了which of the following,Thomas和他的同事就不会发现数据有这么多问题。我选的是,accurate record啥啥啥,包括是美国还是英国人记录的数据。 有主旨题,我选的是一个XXX persistent error。
考到1.1.1的service guarantee题。 关于机经我补充下:问的一个是关于electric work哪个是对的。这个eclectic work的词,前面是在讲说差的restaurant有guarantee会有坏处……然后,customers知道你个质量如何,知道该期待啥,所以empower them to question the qualify. 然后作者提到了electric work。然后我杯具的忘了我选了啥了。。。 PS,我怎么感觉我的题目和机经的题目都不一样。。。但是题目貌似也不难,基本上文章懂了就没有太多问题。
还有1.1.16企业联合 有两种模式: Brand sharing和 asset sharing 对A考的比较多,要求说两个联合方可以有完全不同的产品,但可以share real estate and technology,主要是为了降低成本 第二段讲这两个联合模式的可能风险。前者要求按比例,后者要求什么market target,然后举例,然后有题目。 主旨题,选那个有risk的。 和A相似的模式,【机经里说的是B模式】选那个某个店把自己的某东西租给另外一个店。
逻辑
考到机经32,那道什么生气的人评价自己和别人评价自己是一样的
考到那道iron放到水里,但是遇到了current~~
机经12 考到某人说,经济不好,政府要减少什么图书馆和公园的支出,反对者说,要收费,而不是不支出。问反对者如何反对,选那个提出一个alternative with an analogy…
动词1,动词2,and 动词3 perhaps 动词4 VS 动词1,动词2,动词3 and perhaps 动词4
The biography of the EEE sisters includes XX, YY and ZZ, provides/ providing (楼主在这里纠结了,不知道前面那个includes算不算是谓语了,如果是就该选providing……) a ### of the family-- they are(有个有they are, 有个没有) ### about ……【答案我自己也不确定,感觉关键在于那个includes】
OG11上面有一篇非常相近的,麻烦LZ确认一下: After evidence was obtained in the 1920’s that the universe is expanding, it became reasonable to ask: will the universe continue to expand indefinitely, or is there enough mass in it for the mutual attraction of its constituents to bring this expansion to a halt? It can be calculated that the critical density of matter needed to brake the expansion and “close” the universe is equivalent to three hydrogen atoms per cubic meter. But the density of the observable universe—luminous matter in the form of galaxies—comes to only a fraction of this. If the expansion of the universe is to stop, there must be enough invisible matter in the universe to exceed the luminous matter in density by a factor of roughly 70. Our contribution to the search for this “missing matter” has been to study the rotational velocity of galaxies at various distances from their center of rotation. It has been known for some time that outside the bright nucleus of a typical spiral galaxy luminosity falls off rapidly with distance from the center. If luminosity were a true indicator of mass, most of the mass would be concentrated toward the center. Outside the nucleus the rotational velocity would decrease geometrically with distance from the center, in conformity with Kepler’s law. Instead we have found that the rotational velocity in spiral galaxies either remains constant with increasing distance from the center or increases slightly. This unexpected result indicates that the falloff in luminous mass with distance from the center is balanced by an increase in nonluminous mass. Our findings suggest that as much as 90 percent of the mass of the universe is not radiating at any wavelength with enough intensity to be detected on the Earth. Such dark matter could be in the form of extremely dim stars of low mass, of large planets like Jupiter, or of black holes, either small or massive. While it has not yet been determined whether this mass is sufficient to “close” the universe, some physicists consider it significant that estimates are converging on the critical value.