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2016 | OriginalPaper | Buchkapitel

1. Introduction

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Abstract

This introductory chapter discusses the meaning of the words that appear in the book’s title. It then gives a concise description of the historical background in which the techniques introduced in the book were developed. The structure of the book is also presented and commented on. Finally, some possible further readings are suggested.

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Fußnoten
1
In numerical analysis, “precision” is the resolution of the representation of the measured quantity, typically defined by the number of decimal digits; more precisely, resolution is the smallest change in the underlying physical quantity that produces a response in the measurement instrument. It must be noted that in the fields of science and statistics, the word “precision” traditionally has a very different meaning. It refers to repeated measurements of the same quantity and is related to reproducibility and repeatability. It is the degree to which repeated measurements under unchanged conditions provide the same results. On the other hand, the “accuracy” of a measurement is the degree of closeness of the measurement of a quantity to the true value of the quantity.
 
2
Photo by Dicklyon (Own work) [CC BY-SA 3.0 (http://​creativecommons.​org/​licenses/​by-sa/​3.​0)], via Wikimedia Commons.
 
3
Sunspots are temporary phenomena on the photosphere of the Sun that appear visibly as dark spots compared to surrounding regions. They are generated by strong magnetic fields that are created in the interior of the Sun and inhibit convective motions, thus forming areas of reduced surface temperature. Of all solar features, the sunspots are the most easily observed and were thus studied since the invention of the telescope by Galileo in 1609. This invention was based on previous work by Hans Lipperhey, a German spectacle maker, in 1608. Sunspots were first observed telescopically in late 1610 by the English astronomer Thomas Harriot and by the Frisian astronomers Johannes and David Fabricius, who published a description in 1611. The sunspot number series is one of the most popular indexes of solar activity and allowed for observing the well know 11-year period of Solar activity, known as the Schwabe cycle.
 
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Metadaten
Titel
Introduction
verfasst von
Silvia Maria Alessio
Copyright-Jahr
2016
DOI
https://doi.org/10.1007/978-3-319-25468-5_1

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