Phys1101 - Introductory Physics 1
Phys1101 - Introductory Physics 1
College of Liberal Arts & Sciences

  • Introduction
  • Lecture 01
  • Lecture 02
    • Lecture 2, Part 1: Announcements
    • Lecture 2, Part 2: Units
    • Lecture 2, Part 3: Vector Introduction
    • Lecture 2, Part 4: Adding Vectors Graphically
    • Lecture 2, Part 5: Vector Addition Examples
    • Lecture 2, Part 6: Vector Component Introduction
    • Lecture 2, Part 7: Trigonometry
  • Lecture 03
    • Lecture 3, Part 1: Introduction
    • Lecture 3, Part 2: Where Were We
    • Lecture 3, Part 3: Vector Components in Detail
    • Lecture 3, Part 4: Scalar Component Description
    • Lecture 3, Part 5: Example of Finding Scalar Components
    • Lecture 3, Part 6: Scalar Component Addition
    • Lecture 3, Part 7: Scalar Addition Example
    • Lecture 3, Part 8: Motion Diagrams
  • Lecture 04
    • Lecture 4, Part 1: Introduction
    • Lecture 4, Part 2: Where Were We
    • Lecture 4, Part 3: Location Location Location …
    • Lecture 4, Part 4: How Fast ??? What Direction ???
    • Lecture 4, Part 5: Speeding Up? Slowing Down?
    • Lecture 4, Part 6: What Happens at a Turning Point?
  • Lecture 05
    • Lecture 5, Part 01: Introduction
    • Lecture 5, Part 02: Where Were We
    • Lecture 5, Part 03: Big Picture:  1D Kinematics
    • Lecture 5, Part 04: Kinematic Problem Solving Steps
    • Lecture 5, Part 05: Example 1
    • Lecture 5, Part 06: Example 2
    • Lecture 5, Part 07: Example 3
    • Lecture 5, Part 08: Free Fall
    • Lecture 5, Part 09: Free Fall and Kinematic Equations
    • Lecture 5, Part 10: Example 4
    • Lecture 5, Part 11: Example 5
  • Lecture 06
    • Lecture 6, Part 1: Introduction
    • Lecture 6, Part 2: Where Were We
    • Lecture 6, Part 3: Reading Quiz
    • Lecture 6, Part 4: Graph Basics
    • Lecture 6, Part 5: Practice Makes Perfect…
    • Lecture 6, Part 6: The Tangent Line
  • Lecture 07
    • Lecture 7, Part 1: Introduction
    • Lecture 7, Part 2: Where Were We
    • Lecture 7, Part 3: 2D Motion Diagrams
    • Lecture 7, Part 4: Trajectories
    • Lecture 7, Part 5: Why Work With Components…
    • Lecture 7, Part 6: Key Vectors in 2D
    • Lecture 7, Part 7: Watching 2D Motion
    • Lecture 7, Part 8: Dropping Versus Firing…
  • Lecture 08
    • Lecture 8, Part 1: Introduction
    • Lecture 8, Part 2: Where Were We
    • Lecture 8, Part 3: 2D Kinematic Problems:  The Big Picture
    • Lecture 8, Part 4: 2D Kinematic Problem Solving Steps
    • Lecture 8, Part 5: Example – Part a
    • Lecture 8, Part 6: Example – Part b
    • Lecture 8, Part 7: Your Turn
  • Lecture 09
    • Lecture 9, Part 1: Introduction
    • Lecture 9, Part 2: Where Were We
    • Lecture 9, Part 3: What is Special About Projectile Motion?
    • Lecture 9, Part 4: Example Part a
    • Lecture 9, Part 5: Example Part b
    • Lecture 9, Part 6: Example Part c
    • Lecture 9, Part 7: Your Turn
  • Lecture 10
    • Lecture 10, Part 1: Introduction
    • Lecture 10, Part 2: Where Were We
    • Lecture 10, Part 3: Dynamics:  Why Does Velocity Change?
    • Lecture 10, Part 4: Physical Interpretation of Newton’s Laws
    • Lecture 10, Part 5: What is a Force?
    • Lecture 10, Part 6: Mathematics of Newton’s 2nd Law
  • Lecture 11
    • Lecture 11, Part 1: Introduction
    • Lecture 11, Part 2: Where Were We
    • Lecture 11, Part 3: Free Body Diagram and Vector Nature of Newton’s 2nd Law
    • Lecture 11, Part 4: Common Forces:  Weight
    • Lecture 11, Part 5: Common Forces:  Tension
    • Lecture 11, Part 6: Common Forces:  Normal Force
    • Lecture 11, Part 7: Common Forces:  Friction
    • Lecture 11, Part 8: Problem Solving Steps
    • Lecture 11, Part 9: Example
  • Lecture 12
    • Lecture 12, Part 1: Introduction
    • Lecture 12, Part 2: Where Were We
    • Lecture 12, Part 3: Example 1
    • Lecture 12, Part 4: Example 2
    • Lecture 12, Part 5: Example 3
  • Lecture 13
    • Lecture 13, Part 1: Introduction and Where Were We?
    • Lecture 13, Part 2: Why/When Do We Need Newton’s Third Law?
    • Lecture 13, Part 3: Newton’s 3rd Law
    • Lecture 13, Part 4: Changes To Our Problem-Solving Steps
    • Lecture 13, Part 5: Example 1
    • Lecture 13, Part 6: Ropes and Pulleys
    • Lecture 13, Part 7: Example 2
    • Lecture 13, Part 8: Your Turn
  • Lecture 14
    • Lecture 14, Part 01: Introduction
    • Lecture 14, Part 02: Where Were We ?
    • Lecture 14, Part 03: Uniform Circular Motion:  What You Need To Know
    • Lecture 14, Part 04: Example 1
    • Lecture 14, Part 05: Example 2
    • Lecture 14, Part 06: Example 3
    • Lecture 14, Part 07: Optional Roller Coaster Example
    • Lecture 14, Part 08: Satellite Example
    • Lecture 14, Part 09: The Universal Law of Gravitation
    • Lecture 14, Part 10: Satellite Example Continued
  • Lecture 15
    • Lecture 15, Part 1: Introduction and Where Were We?
    • Lecture 15, Part 2: Energy Conservation:  The Basics
    • Lecture 15, Part 3: How Do You Calculate the Net Work?
    • Lecture 15, Part 4: New Problem Solving Steps
    • Lecture 15, Part 5: Example 1
    • Lecture 15, Part 6: Example 2
    • Lecture 15, Part 7: Last Example
    • Lecture 15, Part 8: Final Quiz Questions…
  • Lecture 16
    • Lecture 16, Part 1: Introduction and Where Were We?
    • Lecture 16, Part 2: Defining Our New “Energy Conservation Starting Equation”
    • Lecture 16, Part 3: Defining Mechanical Energy
    • Lecture 16, Part 4: New Problem Solving Steps
    • Lecture 16, Part 5: First Example
    • Lecture 16, Part 6: Second Example
    • Lecture 16, Part 7: Last Example
    • Lecture 16, Part 8: Redo Example From Last Lecture
  • Lecture 17
    • Lecture 17, Part 1: Lecture
  • Lecture 18
    • Lecture 18, Part 1: Introduction and Where Were We?
    • Lecture 18, Part 2: Momentum Change of a Single Object
    • Lecture 18, Part 3: Conservation of Momentum
  • Lecture 19
    • Lecture 19, Part 1: Introduction and Where Were We?
    • Lecture 19, Part 2: Let’s Start With Another Example
    • Lecture 19, Part 3: Elastic Collisions
    • Lecture 19, Part 4: Remaining Quiz Questions
  • Lecture 20
    • Lecture 20, Part 1: Introduction and Where Were We?
    • Lecture 20, Part 2: Rotational Kinematics:  The Basics
    • Lecture 20, Part 3: Examples
  • Lecture 21
    • Lecture 21, Part 1: Introduction and Where Were We?
    • Lecture 21, Part 2: Describing Motion ALONG the Circular Path…
    • Lecture 21, Part 3: Examples
    • Lecture 21, Part 4: Rolling Motion
  • Lecture 22
    • Lecture 22, Part 1: Introduction and Where Were We?
    • Lecture 22, Part 2: A Net Torque Causes Angular Acceleration
    • Lecture 22, Part 3: Torque Example
    • Lecture 22, Part 4: Equilibrium Example
    • Lecture 22, Part 5: Moment of Inertia
    • Lecture 22, Part 6: Non-Equilibrium Example
    • Lecture 22, Part 7: Another Example
  • Lecture 23
    • Lecture 23, Part 1: Introduction and Where Were We?
    • Lecture 23, Part 2: The Basics of Oscillatory Motion
    • Lecture 23, Part 3: Hooke’s Law
    • Lecture 23, Part 4: Kinematics of Simple Harmonic Motion
    • Lecture 23, Part 5: Example
  • Lecture 24
    • Lecture 24, Part 1: Lecture
  • Lecture 25
    • Lecture 25, Part 1: Introduction
    • Lecture 25, Part 2: The Basics of Wave Motion
    • Lecture 25, Part 3: Motion of a Particle on a Wave
    • Lecture 25, Part 4:  Motion of The Wave Crest
    • Lecture 25, Part 5: Examples
Lecture 25 » Lecture 25, Part 2: The Basics of Wave Motion

Lecture 25, Part 2: The Basics of Wave Motion

https://youtu.be/-SMwe8oTdtw

PHYS 1101: Lecture Twenty-Five, Part Two

Our new material in this lecture has to do with waves. We’re very familiar with them in day-to-day life. From a physics perspective, what’s at the heart of a wave is it’s nothing more than what we call a disturbance that’s moving through what, in physics, we’re going to think of as the medium.

In other words, when you drop a pebble into a pond, and you see these ripples on the surface of the water that spread out around that location where the pebble fell in, the disturbance is that ripple in the water, those circular waves that are spreading out. The medium is the water. It’s the material in which this wave is moving through. We’re going to learn in next lecture about sound. That’s nothing more than a wave that propagates through the medium of air, the air molecules that make up the atmosphere.

In this lecture we’re going to look at waves travelling on strings. And you’ll see one of your quiz questions, I even have you thinking about a wave in the context of people, when you’re sitting in a ball game, and you see a wave spread through the crowd. The wave, the motion of this disturbance you describe as the wave, and the medium would be the people. Okay. These are the key features that are true with any wave.

At the heart of it, there’s no new physics. In essence, at the beginning of every wave I have to have some sort of initial disturbance. Think of this as a source. I have to have something that moves, and because of that motion it exerts a force on, it influences the nearby neighbor in this medium, the neighbor then in turn influences its neighbor, and this propagation of this force, and of this interaction is what gives rise to this overall effect of the disturbance propagating along, or moving along.

Let me show you an animation, or a simulation of a very dramatic type of wave–a tsunami. This animation I’m going to show you was generated by a scientist that studies tsunamis, and he simulated the consequence of a large earthquake that happened in 1960 in Chile that’s down here on this map.

The consequence of that tsunami was this water wave that then propagated through the Pacific Ocean. The disturbance is this jarring of the earth that then pushed against the water, and in this simulation he’s showing how that disturbance then keeps exerting a force on the neighboring water molecules, and in turn that keeps happening, and this propagates.

That was Hawaii that you see just got blasted by it, and eventually it reached over here to Japan. This was a Japanese scientist that did this study, or simulation. For the purposes of this demonstration that he did, he greatly magnified the size of the water here, or this ripple compared to the size of the earth, but that’s just so you could see it well. But it’s a good visual though, of a dramatic type of a wave, a tsunami.

It’s the same physics, though. It starts with some disturbance that generates an initial kick, or a force exerted in this medium, in this case, the water. That force then ends up being passed, or exerted on neighbor, to neighbor, to neighbor, and that’s what continues on and builds up to just be this wave, the disturbance. Let’s look at an animation that’s offered through your textbook where we can study the basic features of a wave more carefully, and we can vary some of the parameters.

You can look at this simulation yourself. If you go through WebAssign, into the online version of the textbook, you’ll notice for chapter 16 there’s a simulation section there, and there’s one simulation for this chapter called, it’s just labeled, “C 16.1 Traveling Waves.” That’s the animation I’m going to show you now.

What we have here is a plunger that’s acting on a source. This plunger, when I hit go, does nothing more than move up and down. This disturbance, this initial source here of course, exerts a force on this string, which is attached to this plunger. That string, of course, each segment you can picture is attached to a neighboring segment, which attached to a neighboring segment, and so on. And there are real contact forces between all those segments, and it’s that contact force that gives rise to the propagation of this. Let me reset this and play it for you.

You see, it starts with the plunger going up and down. As a consequence each segment of the string right beside the plunger has to go up and down, but you see, as that effect propagates down the string, it gives rise to this visual effect of something moving to the right. So here I have a snapshot that I’ve taken of that scenario that you just watched.

Now, the thing that jumps out the most at you, I think, as you watch it, is this visual picture of these crests moving to the right. That’s one kind of motion that’s characteristic of a wave. That’s what you really saw in the animation of the tsunami, right? Your eye was drawn to watching the crest of the wave as it moved along the ocean. A separate kind of motion that happens at the same time is to focus on a single segment in this medium. Imagine a red spot that’s painted onto one little section of this string and to look at the motion of this segment.

So this spot that’s attached to the string, we’re going to have to appreciate that it has very different motion than what your eye really watches and sees, which is the crests that move to the right.

So we’re going to break this up into first focusing on a careful analysis of a single spot in the medium, in this case on the string, and watch the motion of that red spot, and let’s think about what it’s doing. Then we’re going to look at the next type of motion, which is that of the wave itself, where we can simplify it to picture we’re following the crest of a wave.

What’s the behavior of that crest, and what sets that characteristic motion? What determines it? Step one, though, let’s focus on the motion of this red spot.

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