File:Britannica Dynamo 3.jpg
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[edit]DescriptionBritannica Dynamo 3.jpg |
English: If a conductor is rotated in the gap between the poles of a horse-shoe magnet, and these poles have plane parallel faces opposing one another, not only is the density of the flux in the interpolar gap small, but the direction of movement is not always at right angles to the direction of the lines, which for the most part pass straight across from one opposing face to the other. When the conductor is midway between the poles (i.e. either at its highest or lowest point), it is at this instant sliding along the lines and does not cut them, so that its E.M.F. is zero. Taking this position as the starting-point, as the conductor moves round, its rate of line-cutting increases to a maximum when it has moved through a right angle and is opposite to the centre of a pole-face (as in the figure), from which point onward the rate decreases to zero when it has moved through 180°. Each time the conductor crosses a line drawn symmetrically through the gap between the poles and at right angles to the axis of rotation, the E.M.F. along its length is reversed in direction, since the motion relatively to the direction of the field is reversed. A curve connecting the instantaneous values of the E.M.F. as ordinates with time or degrees of angular movement as abscissae (as shown at the foot), will, if the speed of rotation be uniform, be a sine curve. |
Date | |
Source | Encyclopædia Britannica, 1911 |
Author | Encyclopædia Britannica, Volume 8, Slice 9., available freely at Project Gutenberg |
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This image comes from the 13th edition of the Encyclopædia Britannica or earlier. The copyrights for that book have expired in the United States because the book was first published in the US with the publication occurring before January 1, 1929. As such, this image is in the public domain in the United States. | ![]() |
Public domainPublic domainfalsefalse |
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current | 17:07, 17 February 2011 | ![]() | 178 × 272 (12 KB) | Keith Edkins (talk | contribs) | =={{int:filedesc}}== {{Information |Description={{en|If a conductor is rotated in the gap between the poles of a horse-shoe magnet, and these poles have plane parallel faces opposing one another, not only is the density of the flux in the interpolar gap s |
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