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If you have trouble grabbing the ruler s tiny indent controls, you can use the tab/indent selection control at the left end of the horizontal ruler. Click the (usually) L-shaped control to cycle through the different tabs and indents and stop at the indent control that s giving you problems. With that control selected, you can now set a rst-line or hanging indent by clicking the desired position on the ruler. n

1 = 11

If you want to perform a simple flip, it s generally easier to choose Edit Transform Flip Horizontal or Flip Vertical. Better yet, right-click (Control-click on the Mac) in the image window and choose one of the Flip commands from the shortcut menu. Quite surprisingly, you can choose any of the shortcut menu commands while working in the Free Transform mode.

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the scatter diagrams of the transmitted sequence, the received sequence, and the sequence at the output of the equalizer Ignore the first 2000 transmissions and count the number of erroneous decisions in the remaining decisions (you should take into account the delay introduced by the channel-equalizer system) (b) Repeat the simulations of part (a) using 16-QAM data, for which y = 132 (verify this value) Use p = 0000001 Run the simulation for 30000 symbols and ignore the first 15000 for error calculation These numbers are larger than in the QPSK case of part (a), and the step-size is also significantly smaller, since the equalizer converges at a slower pace now (c) Repeat the simulations of part (b) using the multi-modulus algorithm (MMA) of Prob 11135 (d) Repeat the simulations of part (b) using the following three additional blind adaptive algorithms: (d1) CMA1-2 from hob 111.

Another common situation is to know the distance and angle of a point from either 0,0 or a previous point. In this case, you can use polar coordinates, which can be either absolute or relative. Most commonly, you use relative polar coordinates. Polar coordinates take the form distance<angle. (To type the angle symbol, use the less-than symbol on your keyboard.) If you have Dynamic Input on, set to the default options of relative coordinates, polar coordinates are automatically relative. If you have Dynamic Input off or have set Dynamic Input to absolute coordinates, as described earlier in this chapter, you need to add the @ sign before a relative polar coordinate. If you also have the default option of polar format selected, you first see coordinates in polar format. Enter the distance, press the Tab key, and then enter the angle. You can also type the angle (<) symbol instead of using the Tab key. To switch to Cartesian format, just type a comma between the X and Y coordinates.

In the previous section, we introduced the tcrm vo!wge gain ,

36, where y is now chosen as y = E lsI2/E Is1 in terms of the second moment of the symbol constellation divided by the mean of the magnitude of the symbols For 16-QAM data we find y = 33385 (verify this value) Use = 00001 and increase the SNR level at the input of the equalizer to 60 dB Simulate for 30000 iterations and plot the scatter diagram of the output of the equalizer after ignoring the first 15000 samples (d2) The reduced constellation algorithm (RCA) of Rob 111.

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