GRE閲讀理解具體的做題步驟

雖然GRE考試的閲讀理解部分是比較難的，只要我們掌握具體的一些做題步驟還是可以拿到高分的。一起來看看小編為大家整理收集了GRE考試閲讀理解題具體的做題步驟吧，歡迎大家閲讀!

　　GRE閲讀理解5大做題步驟

第一步：讀原文

GRE閲讀的基本做題方法，就是先讀原文再看題目，看過題目後再根據題目定位回原文，所以讀原文是做一篇閲讀的第一步。有些讀者已經養成了先讀題目再看原文的閲讀習慣，其實，做題的順序要因閲讀特點和出題方式而異，GRE閲讀題目的出題順序和原文幾乎沒有任何聯繫，也就是説第一道題可能考了原文的末尾，而最後一道題可能考的是原文的開始，故先讀題目再讀原文對做題沒有任何幫助，反而有可能擾亂讀者理解原文內在的邏輯結構。

第二步：讀原文的同時對重點、考點做標記

做標記是指在讀文章的時候用簡單的符號記錄所讀重點內容，這應該和讀GRE閲讀文章同步進行，標記可以輕輕做在試卷邊緣，也可以另外寫在草稿紙上。所標記的主要目的是為了讀完選項之後能快速、準確的定位，這個步驟要求讀者熟悉常考考點，對應做標記的內容爛熟於胸，這樣才能不費時間的給自己下一步的定位作準標記。

第三步：讀題幹、選項

讀GRE閲讀題乾的過程也是個找題幹特徵的過程，看看題幹所述和自己所做標記的內容有沒有聯繫，如果有，則可以直接定位，故定位最主要的基礎是題干與標記之間的聯繫。有時候題幹可能沒有可以捕捉的特徵，這時讀者不妨從選項下手，選項中也時常會有明顯的特徵反映出它與原文中的重點內容之間的相關性。

第四步：定位

定位指的是確定考題針對GRE閲讀原文中什麼位置的內容發問，通常通過題乾和選項的特徵詞來找，判斷了原文所述的位置之後，就可以找原文和答案之間的對應關係了，絕大多數題目都可以通過找題乾和選項的特徵詞準確的定位到原文某處。

第五步：排除干擾選項後按照文字對應原則選答案

GRE考試的備選答案都是五個，通常很少有考題能讓讀者非常直接的判斷出正確答案，總有1-2個迷惑性比較大的選項，所以，考生不妨先豎讀各選相，排除一些明顯錯誤的選項，然後再對剩下的進行細緻的比較，通過原文和選項之間的文字對應關係，進行選擇。

　　GRE閲讀理解備考技巧

1.解剖文章的首段

GRE考試中閲讀部分需要考生積極主動地解讀文章的第1段，閲讀時儘量記住作者提出的問題(現象或觀點)，和一些關於文章內容的概念和詞彙，如這篇文章講的.是生物化學，日本企業文化還是黑人運動。文章的論題是什麼，作者想説什麼?

2.分析作者思路

在腦子裏或者在草稿紙上畫一個新GRE閲讀文章的結構思路題。各個段落的目的是什麼，主題又是什麼-再次提醒，考察的是你的答題能力而非閲讀能力。你不必完全掌握整篇GRE閲讀理解文章，瞭解文章中的每一個細節(其實，你也沒有那麼多時間)。相反，你應該只讀文章段落的第1句，而快速瀏覽其餘部分。當你“讀”完這篇文章時，你就能對文章的結構思路有總體的把握。

3.語氣詞過渡詞要重點留意

在快速閲讀文章時，特別留意段落開頭或者結尾可能出現的語氣詞和過渡詞。這樣做有助於你對作者思路的把握，從而快速掌握文章大意。

4.總結文章大意

在回答問題前，花幾秒鐘總結一下文章的思路和主題。

5.開始答題

根據你對文章的整體思路來答題。將問題(或選項)定位到文章中具體的某個段落甚至具體的句子。這裏，你可以比第3個步驟更仔細。

　　GRE閲讀理解練習題

Hotter and more massive than the Sun, stars called “stragglers” are puzzling to astronomers because such rapidly burning stars would not be expected to persist in ancient star clusters. Some researchers believe that the typical blue stragglers formed when two ancient, lower-mass stars collide and merge form more massive, hotter star. Peter Leonard theorizes alternatively that in low density globular clusters, where mergers between single stars occur too infrequently to account for the observed quantity of blue stragglers, these stragglers are created instead by a group of stars. He suggests that a pair of stars already orbiting each other presents a larger target for a third star or another pair. Once this new grouping forms, close encounters between the stars could prompt any two to merge as a blue straggler. Leonard’s model predicts that each blue straggler has a distant orbiting companion—as appears true of many blue stragglers in the M67 cluster of the Milky Way galaxy.

1. The reference to a “larger target” serves primarily to suggest why a

A. blue straggler would be more likely to collide and merge with another star than would be a lower-mass star

B. pair of stars would be more likely to encounter other stars than would the typical blue straggler

C. pair of stars would be more likely to interact with other stars than would a single star

D. blue straggler would be more likely to interact with a pair of stars than it would with a third star

E. third star would be more likely to encounter a pair than it would to encounter a blue straggler

2. Information presented in the passage suggests which of the following about blue stragglers?

A. They originate from stars that are hotter and more massive than the Sun.

B. They are burning more rapidly than other types of stars observed in ancient star clusters.

C. They are older than most other types of stars within the same star cluster.

D. They are less numerous in low-density globular clusters than are pairs of stars.

E. They generally originate from the oldest stars among those found in ancient star clusters.

3. The passage cites which of the following as evidence undermining the theory presented in the second sentence?

A. A discrepancy between the number of mergers between single stars in certain low-density globular clusters and that in other low-density globular clusters

B. A discrepancy between the heat and mass of blue stragglers formed by one type of process and the heat and mass of blue stragglers formed by another type of process

C. A discrepancy between the frequency of star mergers in low-density globular clusters and those in high-density globular clusters

D. A discrepancy between the amount of heat and mass of ancient single stars and that of blue stragglers

E. A discrepancy between the number of mergers between single stars in certain star clusters and the number of blue stragglers in those clusters

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