Get Apache Solr 3.1 Cookbook PDF

By Rafal Ku

ISBN-10: 1849512183

ISBN-13: 9781849512183

This booklet is a part of Packt's Cookbook sequence; every one bankruptcy appears at a unique element of operating with Apache Solr. The recipes care for universal difficulties of operating with Solr through the use of easy-to-understand, real-life examples. The publication isn't in any respect a whole Apache Solr reference and also you should still see it as a assisting hand while issues get tough in your trip with Apache Solr. builders who're operating with Apache Solr and wish to understand how to strive against universal difficulties will locate this ebook of serious use. wisdom of Apache Lucene will be an advantage yet isn't required.

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When in space, the purpose of a propulsion system is to change the velocity of a spaceship. In order for a spaceship to work, two things are needed: reaction mass and energy. In space, the spaceship must bring along some mass to accelerate away in order to push itself forward in accordance with Newton’s third law: “For every action there is an equal and opposite re-action”. Such mass is called reaction mass. Reaction mass must be carried along with the spaceship and is irretrievably consumed when used.

According to Aristotle and Plato, the universe was a finite sphere. Its ultimate limit was the “primum mobile”, whose diurnal rotation was conferred upon it by a transcendental God, not part of the universe, a motionless prime mover and first cause. Aristarchus estimated the distance from the Earth to the celestial sphere in about one million miles, which is the present day estimate of the distance between Earth and Saturn in our solar system. The notable exception was Democritus. In the decades around 400 BC, he deduced that our Milky Way is composed of stars that appear to be pinpoints of light because of their enormous distances.

The right angle triangle form by the Sun, Cigny 61 and Earth allowed him to calculate the distance from the star using simple trigonometry. However, most of the stars in the night sky are so far away that it is not possible to measure the line of sight shifts and hence their distance. Measuring the distance to very far away stars became possible through the works of Henrietta Leavitt. At the end of 1890s, Leavitt was working for the Harvard College Observatory. She developed a particular curiosity on Cepheid stars.

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Apache Solr 3.1 Cookbook by Rafal Ku

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