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[GRE模拟] GRE经典题库:GRE试题6

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发表于 2012-8-15 12:40:43 | 显示全部楼层 |阅读模式
17. The author focuses primarily on " X" J: S9 ]0 Q' o- N

4 W; p$ [5 Z# T  (A) presenting two competing scientific theories concerning solar ) e" p3 C2 u5 C5 s- R0 _; h

- V' |% Z& _% R, W8 W  activity and evaluating geological evidence often cited to support them
8 L; x* j3 b, b( A / L8 K; K9 i9 m! R; b4 w
  (B) giving a brief overview of some recent scientifrc developments : w3 G& O/ t) }0 e8 Q; L6 }
$ q# }( t: ~% o  x3 a
  in s'olar physics and assessing their impact on future climatological research 3 e3 {: [- @1 A- R

8 d9 @5 n8 T/ X7 Q% S/ D* Y+ _  (C) discussing the difficulties involved in linkinl: ter- restrial * n* c: w- {9 c/ A, F4 E

5 g# s1 x8 }, I0 Z# D$ R4 ~  phenomena with solar activity and indicating how resolving that issue
; t% M3 y/ O7 L% L3 E
0 h9 S& ^! o: V: P  could have an impact on our understanding of solar physics 7 \4 ^+ Z8 p# D* u

* |! m# e$ E3 ]( t9 F  (D) pointing out the futility of a certain line of sci- entific inquiry 6 p. u$ V( M& p2 S  F
4 [$ M) N/ C+ f7 T
  into the terrestrial effects of solar activity and recommendine ita
9 d$ W( D: L2 I) c4 R) e4 L- J 0 Y: H- K" ]' e# M# J& n
  aban- donment in favor of purely physics-oriented research . K  y; P8 u5 f; k8 f
5 T2 H- p6 D8 {! E" b
  (E) outlinine the specific reasons why a problem in solar physics has 0 ~% p% q/ u: J. V9 x; V' x

# _9 q5 ~- }3 |& q! P  not yet been solved and faulting the overly theoretical approach of modern " o( f+ P$ z* A, ^( Q
' v% a/ T0 d4 g. c% L$ I+ D* D
  physicists. 6 z$ _2 z( O7 x  ~0 d* {
0 @2 ^2 T3 \" D( C, p( L
  18. Which of th.e following statements about the two models of solar " |0 a! w; F" D# `* Q

% }4 t' ?1 q, I' c& Y+ N8 E1 u  activity. as they are described in lines 37-55, is accurate? - _2 _4 q; s$ j% l  F6 H6 \! e
( Q0 s& D* S0 o7 D) \; L
  (A) In both modgls cyclical solar activity is regarded as a long-lived 7 s. t! \) A) u5 D1 U7 s

; A+ H. P0 T  E# d# @  feature of the Sun, persisting with little change over billions of years.
- C, y# a% C2 Z # ~, b5 H: f$ {4 q" @( d8 I. g
  (B) Tn both models the solar-activity cycle is hypothesized as being 9 j) _! W3 Y) {4 v4 h
7 W0 b" y# y3 f
  dependent on the large-scale solar magnetic field.
( O" I# ]# _6 N* _3 p* F8 c . j5 D6 j" c$ [+ h. s# {; V, @
  (C) Tn one model the Sun's magnetic fieid is thought to play a role in
4 G: V9 ~' V$ u* y& L! w
( e; [4 g: {! x; Q1 p  causing solar activ- ity, whereas in the other model it is not. : B7 ]* K5 p2 W; w& s8 B

. p' A9 V& T8 M7 K  (D) In one model solar activity is presumed to be unrelated to terrestrial
  K, x. `  Z* k1 [; Y
( q1 M9 t/ M5 n: C" I! V- L. s3 p  phenomena. whereas in the other model solar activity is thought to have
; ]: {7 Y% c% W9 P# }
# }: g. {, c  _! y3 x  observable effects on the Earth. 3 K' ~! r) x8 A: ?* h* f6 a1 _) O( e

, T& h2 K% ~  V1 f  (E) In one model cycles of solar activity with peri- odicities longer than ; D/ u- A9 a* ~# S5 \, l! H4 t

' l; L- ?! t3 x" V) G  a few decades are con- sidered to be impossible, whereas in the other model
' @4 s+ ]+ x2 b! z( x% B' p! Q% F' C , U9 N# q7 S' v8 `7 S; a+ L! Z
  such cycles are predicted.
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