Stars/Sun/Heliography/Quiz

Heliography is a lecture focusing on the features of the Sun's surface. It is a lecture as part of the radiation astronomy course on solar astronomy.

You are free to take this quiz based on heliogony at any time.

To improve your score, read and study the lecture, the links contained within, listed under See also, External links, and in the template. This should give you adequate background to get 100 %.

As a "learning by doing" resource, this quiz helps you to assess your knowledge and understanding of the information, and it is a quiz you may take over and over as a learning resource to improve your knowledge, understanding, test-taking skills, and your score.

Suggestion: Have the lecture available in a separate window.

To master the information and use only your memory while taking the quiz, try rewriting the information from more familiar points of view, or be creative with association.

Enjoy learning by doing!

Quiz
{Yes or No, As geography describes the features of the surface of the Earth, heliography describes the surface features of Helios or the Sun, Sol. + Yes - No
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{True or False, The Sun has no specific heliographic feature that allows the direct derivation of longitude and latitude. + TRUE - FALSE
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{Complete the text: The { Carrington (i) } longitude (λ2) is measured from the central meridian as it passes through the { ascending (i) } node of the solar equator at { Greenwich (i) } noon on January 1, 1854 (JD 2398220.0) and rotating with the { sidereal (i) } period of 25.38 Earth days.
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{Yes or No, The surface of the Sun is often described by features observed which are located using heliographic coordinates based on heliographic north and south poles. + Yes - No
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{True or False, Sunspots are holes in the surface of the Sun. + TRUE - FALSE
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{What features occasionally show a heliographic distribution on the surface of the Sun? - granulation or supergranulation + active regions + coronal holes + the north an south heliographic poles + sunspots + latitudinal bands that rotate at different rates
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{Yes or No, The Stonyhurst Disk may be superimposed on an image of the Sun to determine the heliographic coordinates. + Yes - No
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{Complete the text: Match up a heliographic feature of the Sun with a heliographic property: sunspots - L polar coronal holes - M coronal mass ejection - N coronal loops - O flares - P photosphere - Q atmosphere - R 106 temperature region - S chromosphere - T transition region - U corona - V heliosphere - W begin to appear at high latitudes and move toward the equator { L (i) }. hemispherically centered on the solar equator { W (i) }. uniform and independent of latitude and longitude { Q (i) }. intensity tracks with active regions { V (i) }. uniformly active above the photosphere { T (i) }. tracks with flaring { N (i) }. tracks with flares, loops, and active regions { S (i) }. tracks with active regions away from sunspots { O (i) }. differential rotation with latitude { R (i) }. track in active regions with sunspots { P (i) }. appear around the magnetic poles and track with them { M (i) }. forms a kind of nimbus around chromospheric features such as spicules and filaments, and is in constant, chaotic motion, viewed in the ultraviolet { U (i) }.
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{Yes or No, The first longitude (λ1) is measured from the plane of the "central meridian" as it passes through the rotation axis of the Sun and the line connecting the center of the Sun to the observer. + Yes - No
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{Yes or No, The Carrington longitude (λ2) is measured from the central meridian as it passes through the ascending node of the solar equator at Greenwich noon on January 1, 1854 (JD 2398220.0) and rotating with the sidereal period of 25.38 Earth days. + Yes - No
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Hypotheses

 * 1) Phenomena occurring above or below the surface of the Sun alter its appearance.