下面为大家推荐的是关于SAT阅读文章模拟题，包括了文章和后面的问题，以及正确答案。澳际小编提醒考生，备考SAT阅读考试一定要多做一些模拟题和真题，这样才能在更短的时间内适应SAT阅读考试的形式，下面是详细内容。

　　Virtually everything astronomers known about objects

　　outside the solar system is based on the detection of

　　photons-quanta of electromagnetic radiation. Yet there

　　is another form of radiation that permeates the universe:

　　(5) neutrinos. With (as its name implies) no electric charge,

　　and negligible mass, the neutrino interacts with other

　　particles so rarely that a neutrino can cross the entire

　　universe, even traversing substantial aggregations of

　　matter, without being absorbed or even dlected. Neu-

　　(10)trinos can thus escape from regions of space where light

　　and other kinds of electromagnetic radiationare blocked

　　by matter. Furthermore, neutrinos carry with them

　　information about the site and circumstances of their

　　production: therore, the detection of cosmic neutrinos

　　(15)could provide new information about a wide variety of

　　cosmic phenomena and about the history of the uni-

　　verse.

　　But how can scientists detect a particle that interacts

　　so infrequently with other matter? Twenty-five years

　　(20)passed between Pauli’s hypothesis that the neutrino

　　existed and its actual detection: since then virtually all

　　research with neutrinos has been with neutrinos created

　　artificially in large particle accelerators and studied

　　under neutrino microscopes. But a neutrino telescope,

　　(25) capable of detecting cosmic neutrinos, is difficult to co-

　　nstruct. No apparatus can detect neutrinos unless it is

　　extremely massive, because great mass is synonymous

　　with huge numbers of nucleons (neutrons and protons),

　　and the more massive the detector, the greater the pro-

　　(30) bability of one of its nucleon’s reacting with a neutrino.

　　In addition, the apparatus must be sufficiently shielded

　　from the interfering fects of other particles.

　　Fortunately, a group of astrophysicists has proposed

　　a means of detecting cosmic neutrinos by harnessing the

　　(35) mass of the ocean. Named DUMAND, for Deep Under-

　　water Muon and Neutrino Detector, the project calls for

　　placing an array of light sensors at a depth of five kilo-

　　meters under the ocean surface. The detecting medium is

　　the seawater itself: when a neutrino interacts with a

　　(40)particle in an atom of seawater. the result is a cascade of

　　electrically charged particles and a flash of light that can

　　be detected by the sensors. The five kilometers of sea-

　　water above the sensors will shield them from the interf-

　　ering fects of other high-energy particles raining down

　　(45) through the atmosphere.

　　The strongest motivation for the DUMAND project

　　is that it will exploit an important source of information

　　about the universe. The extension of astronomy from

　　visible light to radio waves to x-rays and gamma rays

　　(50) never failed to lead to the discovery of unusualobjects

　　such as radio galaxies, quasars, and pulsars. Each of

　　these discoveries came as a surprise. Neutrino astronomy

　　will doubtless bring its own share of surprises.

　　1. Which of the following titles best summarizes the passage as a whole?

　　(A) At the Threshold of Neutrino Astronomy

　　(B) Neutrinos and the History of the Universe

　　(C) The Creation and Study of Neutrinos

　　(D) The DUMAND System and How It Works

　　(E) The Properties of the Neutrino

　　2. With which of the following statements regarding neutrino astronomy would the author be most likely to agree?

　　(A) Neutrino astronomy will supersede all present forms of astronomy.

　　(B) Neutrino astronomy will be abandoned if the DUMAND project fails.

　　(C) Neutrino astronomy can be expected to lead to major breakthroughs in astronomy.

　　(D) Neutrino astronomy will disclose phenomena that will be more surprising than past discoveries.

　　(E) Neutrino astronomy will always be characterized by a large time lag between hypothesis and experimental confirmation.

　　3. In the last paragraph, the author describes the development of astronomy in order to

　　(A) suggest that the potential findings of neutrino astronomy can be seen as part of a series of astronomical successes

　　(B) illustrate the role of surprise in scientific discovery

　　(C) demonstrate the fectiveness of the DUMAND apparatus in detecting neutrinos

　　(D) name some cosmic phenomena that neutrino astronomy will illuminate

　　(E) contrast the motivation of earlier astronomers with that of the astrophysicists working on the DUMAND project

　　4.According to the passage, one advantage that neutrinos have for studies in astronomy is that they

　　(A) have been detected for the last twenty-five years

　　(B) possess a variable electric charge

　　(C) are usually extremely massive

　　(D) carry information about their history with them

　　(E) are very similar to other electromagnetic particles

　　5. According to the passage, the primary use of the apparatus mentioned in lines 24-32 would be to

　　(A) increase the mass of a neutrino

　　(B) interpret the information neutrinos carry with them

　　(C) study the internal structure of a neutrino

　　(D) see neutrinos in distant regions of space

　　(E) detect the presence of cosmic neutrinos

　　6. The passage states that interactions between neutrinos and other matter are

　　(A) rare

　　(B) artificial

　　(C) undetectable

　　(D) unpredictable

　　(E) hazardous

　　7. The passage mentions which of the following as a reason that neutrinos are hard to detect?

　　(A) Their pervasiveness in the universe

　　(B) Their ability to escape from different regions of space

　　(C) Their inability to penetrate dense matter

　　(D) The similarity of their structure to that of nucleons

　　(E) The infrequency of their interaction with other matter

　　8. According to the passage, the interaction of a neutrino with other matter can produce

　　(A) particles that are neutral and massive

　　(B) a form of radiation that permeates the universe

　　(C) inaccurate information about the site and

　　circumstances of the neutrino’s production

　　(D) charged particles and light

　　(E) a situation in which light and other forms of electromagnetic radiation are blocked

　　9. According to the passage, one of the methods used to establish the properties of neutrinos was

　　(A) detection of photons

　　(B) observation of the interaction of neutrinos with gamma rays

　　(C) observation of neutrinos that were artificially created

　　(D) measurement of neutrinos that interacted with particles of seawater

　　(E) experiments with electromagnetic radiation

　　Correct Answers：ACADEAEDC

　　以上就是这一例SAT阅读文章模拟题的全部内容，包括了9道题目。大家可以在备考自己的SAT阅读考试的时候，用此来加以适当的练习，如果能有时间进行限制，就会更有作用。

SAT阅读文章模拟题一篇模拟题题目及答案

　　下面为大家推荐的是关于SAT阅读文章模拟题，包括了文章和后面的问题，以及正确答案。澳际小编提醒考生，备考SAT阅读考试一定要多做一些模拟题和真题，这样才能在更短的时间内适应SAT阅读考试的形式，下面是详细内容。

　　Virtually everything astronomers known about objects

　　outside the solar system is based on the detection of

　　photons-quanta of electromagnetic radiation. Yet there

　　is another form of radiation that permeates the universe:

　　(5) neutrinos. With (as its name implies) no electric charge,

　　and negligible mass, the neutrino interacts with other

　　particles so rarely that a neutrino can cross the entire

　　universe, even traversing substantial aggregations of

　　matter, without being absorbed or even dlected. Neu-

　　(10)trinos can thus escape from regions of space where light

　　and other kinds of electromagnetic radiationare blocked

　　by matter. Furthermore, neutrinos carry with them

　　information about the site and circumstances of their

　　production: therore, the detection of cosmic neutrinos

　　(15)could provide new information about a wide variety of

　　cosmic phenomena and about the history of the uni-

　　verse.

　　But how can scientists detect a particle that interacts

　　so infrequently with other matter? Twenty-five years

　　(20)passed between Pauli’s hypothesis that the neutrino

　　existed and its actual detection: since then virtually all

　　research with neutrinos has been with neutrinos created

　　artificially in large particle accelerators and studied

　　under neutrino microscopes. But a neutrino telescope,

　　(25) capable of detecting cosmic neutrinos, is difficult to co-

　　nstruct. No apparatus can detect neutrinos unless it is

　　extremely massive, because great mass is synonymous

　　with huge numbers of nucleons (neutrons and protons),

　　and the more massive the detector, the greater the pro-

　　(30) bability of one of its nucleon’s reacting with a neutrino.

　　In addition, the apparatus must be sufficiently shielded

　　from the interfering fects of other particles.

　　Fortunately, a group of astrophysicists has proposed

　　a means of detecting cosmic neutrinos by harnessing the

　　(35) mass of the ocean. Named DUMAND, for Deep Under-

　　water Muon and Neutrino Detector, the project calls for

　　placing an array of light sensors at a depth of five kilo-

　　meters under the ocean surface. The detecting medium is

　　the seawater itself: when a neutrino interacts with a

　　(40)particle in an atom of seawater. the result is a cascade of

　　electrically charged particles and a flash of light that can

　　be detected by the sensors. The five kilometers of sea-

　　water above the sensors will shield them from the interf-

　　ering fects of other high-energy particles raining down

　　(45) through the atmosphere.

　　The strongest motivation for the DUMAND project

　　is that it will exploit an important source of information

　　about the universe. The extension of astronomy from

　　visible light to radio waves to x-rays and gamma rays

　　(50) never failed to lead to the discovery of unusualobjects

　　such as radio galaxies, quasars, and pulsars. Each of

　　these discoveries came as a surprise. Neutrino astronomy

　　will doubtless bring its own share of surprises. 上12下

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