User:Tony1/Exercises in textual flow: Difference between revisions

Revision as of 07:38, 1 September 2006

Revision as of 12:34, 3 September 2006

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===Exercise 1: paragraphing===

Here’s a fat, grey paragraph that functions aswas the lead ofin ana FAC. It needs to be broken up into, let’s say, four manageable portions. There are a number of ways of dividing it, so we can offer only a suggested solution.

'''Your task''' is to identify three statements withinin the paragraph that appear to take a fresh direction. Check that each of these statements can function as a “theme”—that is, as a logical, cohesive subsidiary topic within the lead. To perform this function, each statement that you identify must be followed by extensions or enhancements of the idea that it introduces. [[Image:SOHO solar flare sun large 20031026 0119 eit 304.png|thumb|right|200px|Large solar flare recorded using UV light]]

<div style="padding:10px; background-color:#E6E6FA">'''The Sun''' is the star at the centre of our solar system. The Earth and other matter (including other planets, asteroids, meteoroids, comets and dust) orbit the Sun, which by itself accounts for more than 99% of the solar system’s mass. Energy from the Sun—in the form of sunlight, supports almost all life on Earth via photosynthesis, and, via heating from insolation—drives the Earth’s climate and weather. About 74% of the Sun’s mass is hydrogen, 25% is helium, and the rest is made up of trace quantities of heavier elements. The Sun is about 4.6 billion years old and is about halfway through its main-sequence evolution, during which nuclear fusion reactions in its core fuse hydrogen into helium. Each second, more than four million tonnes of matter are converted into energy within the Sun’s core, producing neutrinos and solar radiation. In about five billion years, the Sun will evolve into a red giant and then a white dwarf, creating a planetary nebula in the process. The Sun is a magnetically active star; it supports a strong, changing magnetic field that varies from year to year and reverses direction about every 11 years. The Sun’s magnetic field gives rise to many effects that are collectively called solar activity, including sunspots on the surface of the Sun, solar flares, and variations in the solar wind that carry material through the solar system. The effects of solar activity on Earth include auroras at moderate to high latitudes, and the disruption of radio communications and electric power. Solar activity is thought to have played a large role in the formation and evolution of the solar system, and strongly affects the structure of Earth’s outer atmosphere. Although it is the nearest star to Earth and has been intensively studied by scientists, many questions about the Sun remain unanswered; these include why its outer atmosphere has a temperature of over a million degrees K when its visible surface (the photosphere) has a temperature of just 6000 K. Current topics of scientific enquiry include the Sun’s regular cycle of sunspot activity, the physics and origin of solar flares and prominences, the magnetic interaction between the chromosphere and the corona, and the origin of the solar wind.</div>

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When you’ve identified the three statements, have a look at our [[User:Tony1/How to satisfy Criterion 1a: exercises in textual flow#Exercise 1: suggested solution|<b>suggested solution</b>]].

===Exercise 2: sentence length===