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Have you heard that dividing a positive integer by 0 gives you infinity If not, you probably will some day Be skeptical! The first thing you must do to figure out if it s really true is to define infinity That s not easy No meaningful, enduring definition of infinity produced by mathematicians has ever had anything to do with division by 0 Again, look at the problem inside-out If you want to multiply 0 by any positive integer n, you must add 0 to itself (n 1) times No matter how large you make n, you always get 0 when you add it to itself (n 1) times Why should adding 0 to itself forever make any difference It s tempting to suppose that it might, but that doesn t prove that it will In mathematics, we need proof before we can claim something is true!

Therefore, using the lower right 2 2 block, we have that = Using the upper right 2 2 block we have that Qd = 1 0 1 1 1 6

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Manipulating equations Whenever we add or subtract a certain quantity to or from both sides of the equation, we still have a valid equation The same is true if we multiply both sides of an equation by a certain quantity, or divide either side by a certain quantity other than 0 The quantity you add, subtract, or multiply by can be a number, a variable, or a complicated expression, as long as it is the same for the left-hand side of the equation as for the righthand side If you divide both sides of an equation by anything, it s best to stick to nonzero numbers If you divide both sides of an equation by a variable or an expression containing a variable, you can get into trouble, as you ll see in Chap 11 Keep these rules in mind That way, you won t get confused later on when we do something like divide both sides of an equation by 999, or multiply both sides by (a + b) The fact that we can do these things makes solving equations and proving various facts far easier than they would be otherwise

Table 14-3

Here s a challenge!

1 2 1

In terms of the number line and displacements, show what happens when you multiply the integer 1 over and over, endlessly, by 2

10 2 =

Figure 5-3 illustrates this process Because the multiplier is negative, we jump to the opposite side of the number reflector each time we multiply Then the result becomes a new multiplicand Because the

Site Cutler, ME Jim Creek, WA Lualualei, HI LaMoure, ND Aquada, Puerto Rico Keflavik, Iceland Niscemi, Italy Harold E Holt, Australia Rhauderfehn, Germany Rosnay, France St Assie, France Bombay, India Tavolara, Italy Ebino Huyshu, Japan Noviken, Norway Arkhanghelsk, Russia Batumi, Russia Kaliningrad, Russia Matotchkinchar, Russia Vladivostok, Russia Anthorn, United Kingdom JXN UGE UVA UGKZ UFQE UIK GQD ICV HWU FTA NWC ID NAA NLK NPM NML4 NAU NRK Frequency kHz 240 248 214 252 4075 375 399 198 185 151 168 151 2027 234 164 194 146 303 181 150 019 45 150* input pwr 100* input pwr 100* input pwr 100* input pwr 100* input pwr 42 43 100 100 25 1000 500 400 23 Power KW 1000 250 566

1 3 1 2

Start at -1 -4

1 and multiply by 2 over and over We jump back and forth across the number reflector, doubling our distance from it with each jump To avoid clutter, only the even-integer points are shown on the number line

10 2

Most of the VLF signals, such as clicks, pops, and tweeks, can be heard almost at any time of the day or night Whistler occurrence is a function of both thunderstorm occurrence and propagation conditions through the ionosphere The rate is higher at night than during the day because of the diurnal variation in the D-region absorption, which is highest when the Sun is above the horizon At night, the D-layer does not exist since it is ionized by solar ultraviolet rays The whistler rate, or the number of whistlers heard per minute, has a marked dependence on sunspot activity, the rate increasing with the sunspot number Whistlers are heard only when sufficient ionization exists along the path to guide the waves along the Earth s magnetic field This ionization is assumed to be supplied from the Sun during a solar To hear a whistler or other signals such as dawn chorus, you will no doubt have to get away from the power line and industrial noise The listening time for these signals will be from near local midnight to early morning hours

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