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Triangle Definition of sin and cos Consider the triangle ABC below. Let A be called . B HYP (hypotenuse) A OPP (side opposite to the angle ) C ADJ (side adjacent to the angle ) Then sin OPP BC HYP AB cos ADJ AC HYP AB . (SOH CAH TOA) MATH 1310 Ronald Brent © 2016 All rights reserved. Lecture 4A 1 of 25 Special Angles (30°, 45°, 60°) 1 Find sin 45 and cos 45 . 2 2 2 Pythagorean Theorem: s s 1 , or 2 s 1 Hence Choosing s > 0, we have s 1 2 s 45 1 1 . s 2 and s 2 2 sin 45 cos 45 45 s 1 , and so 2 2 2 45 1 1 2 45 1 2 MATH 1310 Ronald Brent © 2016 All rights reserved. Lecture 4A 2 of 25 Example: Find sin 30 , cos 30 , sin 60 , and cos 60 . Begin with a 30 60 90 right triangle with HYP = 1. 60 1 t 30 s 30 1 60 Notice that when flipping the triangle down and consider the larger one, the result is an equilateral 1 triangle, so the vertical side is also 1. This means 2t = 1, or t . Now since 2 s2 t 2 1 , we have MATH 1310 Ronald Brent © 2016 All rights reserved. 1 s2 1 , 4 Lecture 4A 3 of 25 which means s2 3 3 s 4 2 Again, it is clear that s > 0, which implies the triangle looks like: 1 60 1 2 30 3 2 So sin 30 1 2 cos30 3 , 2 while cos 60 1 2 sin 60 3 . 2 MATH 1310 Ronald Brent © 2016 All rights reserved. Lecture 4A 4 of 25 Angles in Radian Measure How big is a radian? Here’s how big: it’s the angle corresponding to an arc length of 1 in a unit circle. Look at the diagram below. A “unit circle” indicates that the radius = 1 unit, and we’ll always put the center at (0,0) for convenience. The angle as drawn is 1 radian, because the arc length “subtended” (cut off) by the angle has length = 1 unit. Length of the arc = 1 unit radian (0,0) MATH 1310 Ronald Brent © 2016 All rights reserved. Lecture 4A 1 unit (1,0) 5 of 25 Relationship Between Degrees and Radians 360 2 radians 360 1 rad = 2 1 Examples: 57 2 rad = rad 0.017 rad . 360 180 a) Convert 30 to radians. 1 180 Note: radians 45 30 30 180 6 . , 60 and 90 . 4 3 2 5 b) Convert radians to degrees. 6 180 MATH 1310 Ronald Brent © 2016 All rights reserved. Lecture 4A 5 5 180 150 . 6 6 6 of 25 You should commit to memory the following conversion chart since these angles will come up again and again. Degrees 360 270 180 Radians 2 3 2 90 60 45 30 2 3 4 6 Consider the unit circle, centered at the origin, with an angle of radians, as shown below. y (cos , sin ) (1,0) MATH 1310 Ronald Brent © 2016 All rights reserved. Lecture 4A x 7 of 25 (Notice that the angle is measured from the positive x-axis, counterclockwise.) The dotted line defining the terminal side (end) of the angle intersects the circle at a point. As the angle changes, so do the coordinates of that point, so each of the coordinates is a function of the angle . These two functions are very important, and so they have their own names. Definition: In the figure below, the first coordinate is called cos (short for cosine of ). The second coordinate is called sin ( short for sine of ). y (cos , sin ) (1,0) MATH 1310 Ronald Brent © 2016 All rights reserved. Lecture 4A x 8 of 25 Remarks: a) Since this point is on the unit circle, its coordinates must satisfy the equation of that circle: x 2 y 2 1 , that is (cos ) 2 (sin ) 2 1 . n n b) To avoid the constant use of brackets, we write cos to mean (cos ) ; similarly, we n n write sin to mean (sin ) . Thus cos2 sin 2 1. c) Since the cycle repeats every time we go around the circle, the sine and cosine functions are periodic with period 2 . MATH 1310 Ronald Brent © 2016 All rights reserved. Lecture 4A 9 of 25 Table of Trig. Values: Since 30 6 radians, 45 4 radians, and 60 3 radians, we can use the previous triangle trig. results and the following picture to fill in the table on the next page. y ( cos , sin ) (0,1) (-1,0) (1,0) x (0,-1) MATH 1310 Ronald Brent © 2016 All rights reserved. Lecture 4A 10 of 25 Angle y sin x cos 0 0 1 1 2 3 2 2 2 2 2 3 3 2 1 2 1 0 0 1 3 2 1 0 2 0 1 6 4 2 MATH 1310 Ronald Brent © 2016 All rights reserved. Lecture 4A 11 of 25 Trig Values at Other Angles: Definition: An Obtuse angle is any angle greater than Example: Find sin Since 2 2 and cos . 3 3 2 120 , the triangle in the 3 figure below is the 30 60 90 y 2 120 3 3 2 60 1 2 2 1 . 3 2 Ronald Brent © 2016 All rights reserved. radians. 1 2 3 Hence, sin 3 2 MATH 1310 2 1 3 , 2 2 triangle shown previously. and cos Lecture 4A x (1,0) 12 of 25 Definition: A negative angle is an angle measured in the clockwise direction. Example: Find sin and cos . 3 3 Since 3 y 60 , the triangle in the figure shown is again the 30 60 90 triangle 1 2 shown above. 60 1 3 1 Hence, sin and cos . 2 3 3 2 MATH 1310 Ronald Brent © 2016 All rights reserved. Lecture 4A x 3 2 (1,0) 13 of 25 Graphs of the sine and cosine functions y (cos , sin ) y sin (1,0) x x The second coordinate, y sin , goes from 0 to 1, and back down to 1, then back up to 1. y cos x Meanwhile, the first coordinate, x cos , goes from 1 down to 1, and back to 1. MATH 1310 Ronald Brent © 2016 All rights reserved. Lecture 4A 14 of 25 Graphs of Sine and Cosine (Sinusoidal) Functions y sin x x y cos x x Notice how these graphs oscillate between 1 and 1. Also, the length, or period, of one full cycle is 2 . MATH 1310 Ronald Brent © 2016 All rights reserved. Lecture 4A 15 of 25 Formal Definitions Any function of the form y k sin( a x ) C or y k cos( a x ) C is called sinusoidal. The Amplitude of a sinusoidal graph is equal to one-half the distance from the top to the bottom of the waves, or the number |k|. The Period of a sinusoidal function is the distance for the graph to go through one full cycle. 2 It is always P . a The Angular (Circular) Frequency of a sinusoidal function, |a|, is the number of complete cycles in a horizontal distance of 2 . The Linear Frequency , f is the reciprocal of the a period, so that f . If x represents time, then f has units of cycles per second. 2 The Phase of a sinusoidal function is what point in its cycle it “starts” at, when x = 0. It represents horizontal shifts in the sinusoidal function. The horizontal line y = C, is called the center line about which the function oscillates. MATH 1310 Ronald Brent © 2016 All rights reserved. Lecture 4A 16 of 25 Example: The graph below is f ( x) 2 sin 2 x 3 . Its amplitude is | k | | 2 | 2 , (NOT the bigger number 5.) The circular frequency is 2, the period is , and the frequency is 1 . The phase is 0, and the center line is y = 3. y 5 4 3 2 1 0 x -1 -2 MATH 1310 Ronald Brent © 2016 All rights reserved. Lecture 4A 17 of 25 Changes in Amplitude: y y 4 sin x 5 y 2 sin x 4 y sin x 3 2 1 0 x -1 -2 -3 -4 -5 MATH 1310 Ronald Brent © 2016 All rights reserved. Lecture 4A 18 of 25 y 1 y sin x 4 2 1 y sin x 2 y sin x 1 0 x -1 -2 MATH 1310 Ronald Brent © 2016 All rights reserved. Lecture 4A 19 of 25 y y sin x 2 y sin x 1 0 x -1 -2 MATH 1310 Ronald Brent © 2016 All rights reserved. Lecture 4A 20 of 25 y y sin x 2 y 13 sin x 1 0 x -1 y 2 sin x MATH 1310 Ronald Brent © 2016 All rights reserved. -2 Lecture 4A 21 of 25 Of course all this vertical amplitude scaling works for the cosine graph also. y y 2 cos x y 5 y 12 cos x 4 5 4 3 3 2 2 1 1 0 x -1 -1 -2 -2 -3 -3 -4 -4 -5 -5 y y 4 cos x y y 12 cos x 5 4 MATH 1310 5 4 3 3 2 2 1 1 0 x 0 -1 -1 -2 -2 -3 -3 -4 -4 -5 Ronald Brent © 2016 All rights reserved. x 0 Lecture 4A -5 x 22 of 25 Changes in Frequency: Going from y = sin x or y = cos x, to y sin ( a x ) and y cos ( a x ) involves horizontal scaling. This affects how many cycles appear over a given interval. As a rule: (a) If a is a positive integer, then the graph of y sin ( a x ) ( y cos ( a x ) ) has a complete oscillations, or cycles, in the interval [0, 2 ] . For a positive, if a > 1 this means more oscillations than y = sin x (y = cos x) and for 0 < a < 1, one has less cycles than y = sin x (y = cos x). (b) If a < 0, the graph is reflected about the y-axis, and then compressed or stretched depending upon the value of |a|. y sin ( a x ) and y a sin x are NOT the same. Note: Test it with a = 2 and x MATH 1310 Ronald Brent © 2016 All rights reserved. 2 . Lecture 4A 23 of 25 Examples: Again, in all of these graphs y sin x is shown as a solid line. y sin 2 x y sin 3 x y 2 Period = 3 2 Period = y 2 1 1 0 x 0 -1 -1 -2 -2 y y = sin ( x/2) 2 Period = 4 1 0 x -1 MATH 1310 Ronald Brent © 2016 All rights reserved. -2 Lecture 4A 24 of 25 x Phase Shifts: Phase shifts involve horizontal translations, of shifts in the x-direction. Examples: y sin x 2 y cos x 2 y y 5 5 4 4 3 3 2 2 1 1 0 x 0 -1 -1 -2 -2 -3 -3 -4 -4 -5 -5 MATH 1310 Ronald Brent © 2016 All rights reserved. Lecture 4A x 25 of 25