The Physics of the Oceanic Tides
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The Double Tidal Bulge
The Double Tidal Bulge If you look at any explanation of tides the force is indeed real. Try driving same for all points on the Earth. Try you will see a diagram that looks fast around a tight bend and tell me this analogy: take something round something like fig.1 which shows the you can’t feel a force pushing you to like a roll of sticky tape, put it on the tides represented as two bulges of the side. You are in the rotating desk and move it in small circles (not water – one directly under the Moon frame of reference hence the force rotating it, just moving the whole and another on the opposite side of can be felt. thing it in a circular manner). You will the Earth. Most people appreciate see that every point on the object that tides are caused by gravitational 3. In the discussion about what moves in a circle of equal radius and forces and so can understand the causes the two bulges of water you the same speed. moon-side bulge; however the must completely ignore the rotation second bulge is often a cause of of the Earth on its axis (the 24 hr Now let’s look at the gravitation pull confusion. This article attempts to daily rotation). Any talk of rotation experienced by objects on the Earth explain why there are two bulges. refers to the 27.3 day rotation of the due to the Moon. The magnitude and Earth and Moon about their common direction of this force will be different centre of mass. -
Of Universal Gravitation and of the Theory of Relativity
ASTRONOMICAL APPLICATIONS OF THE LAW OF UNIVERSAL GRAVITATION AND OF THE THEORY OF RELATIVITY By HUGH OSCAR PEEBLES Bachelor of Science The University of Texas Austin, Texas 1955 Submitted to the faculty of the Graduate School of the Oklahoma State University in partial fulfillment of the requirements for the degree of MASTER OF SCIENCE August, 1960 ASTRONOMICAL APPLICATIONS OF THE LAW OF UNIVERSAL GRAVITATION AND OF THE THEORY OF RELATIVITY Report Approved: Dean of the Graduate School ii ACKNOWLEDGEMENT I express my deep appreciation to Dr. Leon w. Schroeder, Associate Professor of Physics, for his counsel, his criticisms, and his interest in the preparation of this study. My appre ciation is also extended to Dr. James H. Zant, Professor of Mathematics, for his guidance in the development of my graduate program. iii TABLE OF CONTENTS Chapter Page I. INTRODUCTION. 1 II. THE EARTH-MOON T"EST OF THE LAW OF GRAVITATION 4 III. DERIVATION OF KEPLER'S LAWS OF PLAN.ET.ARY MOTION FROM THE LAW OF UNIVERSAL GRAVITATION. • • • • • • • • • 9 The First Law-Law of Elliptical Paths • • • • • 10 The Second Law-Law of Equal Areas • • • • • • • 15 The Third Law-Harmonic Law • • • • • • • 19 IV. DETERMINATION OF THE MASSES OF ASTRONOMICAL BODIES. 20 V. ELEMENTARY THEORY OF TIDES. • • • • • • • • • • • • 26 VI. ELEMENTARY THEORY OF THE EQUATORIAL BULGE OF PLANETS 33 VII. THE DISCOVERY OF NEW PLANETS. • • • • • • • • • 36 VIII. ASTRONOMICAL TESTS OF THE THEORY OF RELATIVITY. 40 BIBLIOGRAPHY . 45 iv LIST OF FIGURES Figure Page 1. Fall of the Uoon Toward the Earth • • • • • • • • • • 6 2. Newton's Calculation of the Earth's Gravitational Ef- fect on the Moon. -
Lecture Notes in Physical Oceanography
LECTURE NOTES IN PHYSICAL OCEANOGRAPHY ODD HENRIK SÆLEN EYVIND AAS 1976 2012 CONTENTS FOREWORD INTRODUCTION 1 EXTENT OF THE OCEANS AND THEIR DIVISIONS 1.1 Distribution of Water and Land..........................................................................1 1.2 Depth Measurements............................................................................................3 1.3 General Features of the Ocean Floor..................................................................5 2 CHEMICAL PROPERTIES OF SEAWATER 2.1 Chemical Composition..........................................................................................1 2.2 Gases in Seawater..................................................................................................4 3 PHYSICAL PROPERTIES OF SEAWATER 3.1 Density and Freezing Point...................................................................................1 3.2 Temperature..........................................................................................................3 3.3 Compressibility......................................................................................................5 3.4 Specific and Latent Heats.....................................................................................5 3.5 Light in the Sea......................................................................................................6 3.6 Sound in the Sea..................................................................................................11 4 INFLUENCE OF ATMOSPHERE ON THE SEA 4.1 Major Wind -
Chapter 5 Water Levels and Flow
253 CHAPTER 5 WATER LEVELS AND FLOW 1. INTRODUCTION The purpose of this chapter is to provide the hydrographer and technical reader the fundamental information required to understand and apply water levels, derived water level products and datums, and water currents to carry out field operations in support of hydrographic surveying and mapping activities. The hydrographer is concerned not only with the elevation of the sea surface, which is affected significantly by tides, but also with the elevation of lake and river surfaces, where tidal phenomena may have little effect. The term ‘tide’ is traditionally accepted and widely used by hydrographers in connection with the instrumentation used to measure the elevation of the water surface, though the term ‘water level’ would be more technically correct. The term ‘current’ similarly is accepted in many areas in connection with tidal currents; however water currents are greatly affected by much more than the tide producing forces. The term ‘flow’ is often used instead of currents. Tidal forces play such a significant role in completing most hydrographic surveys that tide producing forces and fundamental tidal variations are only described in general with appropriate technical references in this chapter. It is important for the hydrographer to understand why tide, water level and water current characteristics vary both over time and spatially so that they are taken fully into account for survey planning and operations which will lead to successful production of accurate surveys and charts. Because procedures and approaches to measuring and applying water levels, tides and currents vary depending upon the country, this chapter covers general principles using documented examples as appropriate for illustration. -
Tides and the Climate: Some Speculations
FEBRUARY 2007 MUNK AND BILLS 135 Tides and the Climate: Some Speculations WALTER MUNK Scripps Institution of Oceanography, La Jolla, California BRUCE BILLS Scripps Institution of Oceanography, La Jolla, California, and NASA Goddard Space Flight Center, Greenbelt, Maryland (Manuscript received 18 May 2005, in final form 12 January 2006) ABSTRACT The important role of tides in the mixing of the pelagic oceans has been established by recent experiments and analyses. The tide potential is modulated by long-period orbital modulations. Previously, Loder and Garrett found evidence for the 18.6-yr lunar nodal cycle in the sea surface temperatures of shallow seas. In this paper, the possible role of the 41 000-yr variation of the obliquity of the ecliptic is considered. The obliquity modulation of tidal mixing by a few percent and the associated modulation in the meridional overturning circulation (MOC) may play a role comparable to the obliquity modulation of the incoming solar radiation (insolation), a cornerstone of the Milankovic´ theory of ice ages. This speculation involves even more than the usual number of uncertainties found in climate speculations. 1. Introduction et al. 2000). The Hawaii Ocean-Mixing Experiment (HOME), a major experiment along the Hawaiian Is- An early association of tides and climate was based land chain dedicated to tidal mixing, confirmed an en- on energetics. Cold, dense water formed in the North hanced mixing at spring tides and quantified the scat- Atlantic would fill up the global oceans in a few thou- tering of tidal energy from barotropic into baroclinic sand years were it not for downward mixing from the modes over suitable topography. -
A Survey on Tidal Analysis and Forecasting Methods
Science of Tsunami Hazards A SURVEY ON TIDAL ANALYSIS AND FORECASTING METHODS FOR TSUNAMI DETECTION Sergio Consoli(1),* European Commission Joint Research Centre, Institute for the Protection and Security of the Citizen, Via Enrico Fermi 2749, TP 680, 21027 Ispra (VA), Italy Diego Reforgiato Recupero National Research Council (CNR), Institute of Cognitive Sciences and Technologies, Via Gaifami 18 - 95028 Catania, Italy R2M Solution, Via Monte S. Agata 16, 95100 Catania, Italy. Vanni Zavarella European Commission Joint Research Centre, Institute for the Protection and Security of the Citizen, Via Enrico Fermi 2749, TP 680, 21027 Ispra (VA), Italy Submitted on December 2013 ABSTRACT Accurate analysis and forecasting of tidal level are very important tasks for human activities in oceanic and coastal areas. They can be crucial in catastrophic situations like occurrences of Tsunamis in order to provide a rapid alerting to the human population involved and to save lives. Conventional tidal forecasting methods are based on harmonic analysis using the least squares method to determine harmonic parameters. However, a large number of parameters and long-term measured data are required for precise tidal level predictions with harmonic analysis. Furthermore, traditional harmonic methods rely on models based on the analysis of astronomical components and they can be inadequate when the contribution of non-astronomical components, such as the weather, is significant. Other alternative approaches have been developed in the literature in order to deal with these situations and provide predictions with the desired accuracy, with respect also to the length of the available tidal record. These methods include standard high or band pass filtering techniques, although the relatively deterministic character and large amplitude of tidal signals make special techniques, like artificial neural networks and wavelets transform analysis methods, more effective. -
Equilibrium Model of Tides Highly Idealized, but Very Instructive, View of Tides
Tides Outline • Equilibrium Theory of Tides — diurnal, semidiurnal and mixed semidiurnal tides — spring and neap tides • Dynamic Theory of Tides — rotary tidal motion — larger tidal ranges in coastal versus open-ocean regions • Special Cases — Forcing ocean water into a narrow embayment — Tidal forcing that is in resonance with the tide wave Equilibrium Model of Tides Highly Idealized, but very instructive, View of Tides • Tide wave treated as a deep-water wave in equilibrium with lunar/solar forcing • No interference of tide wave propagation by continents Tidal Patterns for Various Locations 1 Looking Down on Top of the Earth The Earth’s Rotation Under the Tidal Bulge Produces the Rise moon and Fall of Tides over an Approximately 24h hour period Note: This is describing the ‘hypothetical’ condition of a 100% water planet Tidal Day = 24h + 50min It takes 50 minutes for the earth to rotate 12 degrees of longitude Earth & Moon Orbit Around Sun 2 R b a P Fa = Gravity Force on a small mass m at point a from the gravitational attraction between the small mass and the moon of mass M Fa = Centrifugal Force on a due to rotation about the center of mass of the two mass system using similar arguments The Main Point: Force at and point a and b are equal and opposite. It can be shown that the upward (normal the the earth’s surface) tidal force on a parcel of water produced by the moon’s gravitational attraction is small (1 part in 9 million) compared to the downward gravitation force on that parcel of water caused by earth’s on gravitational attraction. -
Ay 7B – Spring 2012 Section Worksheet 3 Tidal Forces
Ay 7b – Spring 2012 Section Worksheet 3 Tidal Forces 1. Tides on Earth On February 1st, there was a full Moon over a beautiful beach in Pago Pago. Below is a plot of the water level over the course of that day for the beautiful beach. Figure 1: Phase of tides on the beach on February 1st (a) Sketch a similar plot of the water level for February 15th. Nothing fancy here, but be sure to explain how you came up with the maximum and minimum heights and at what times they occur in your plot. On February 1st, there was a full the Moon over the beautiful beaches of Pago Pago. The Earth, Moon, and Sun were co-linear. When this is the case, the tidal forces from the Sun and the Moon are both acting in the same direction creating large tidal bulges. This would explain why the plot for February 1st showed a fairly dramatic difference (∼8 ft) in water level between high and low tides. Two weeks later, a New Moon would be in the sky once again making the Earth, Moon, and Sun co-linear. As a result, the tides will be at roughly the same times and heights (give or take an hour or so). (b) Imagine that the Moon suddenly disappeared. (Don’t fret about the beauty of the beach. It’s still pretty without the moon.) Then how would the water level change? How often would tides happen? (For the level of water change, calculate the ratio of the height of tides between when moon exists and when moon doesn’t exist.) Sketch a plot of the water level on the figure. -
Waves and Tides the Preceding Sections Have Dealt with the Types Of
CHAPTER XIV Waves and Tides .......................................................................................................... Introduction The preceding sections have dealt with the types of motion in the ocean that bring about transport of water massesin a definite direction during a considerable length of time. They have also dealt with the random motion, the turbulence, which is superimposed upon the general flow. Besidesthese types, one has also to consider the oscillating motion characteristic of waves. In general, this motion manifests itself to the observer more by the riseand fall of the sea surface than by the motion of the individual water particles. Waves have attracted attention since before the beginning of recorded history, and in recent years they have been the subject of extensive theoretical studies. Surveys of our knowledge as to the character of ocean waves have been presented by Cornish (1912, 1934), Krtimmel (1911), Patton and Mariner (1932) and by Defant (1929). Lamb (1932) has discussed the hydrodynamic theories of waves, and Thorade (1931) has given a comprehensive review of the theoretical studies of ocean waves and has compiled a long list of literature covering the period from 1687 to 1930. Our understanding of the waves of the ocean, how they are formed and how they travel, is as yet by no means complete. The reason is, in the first place, that actual observations at sea are so difficult that the characteristicsof the waves cannot easily be determined. In the second place, the theories that serve to bring the observed sequence of events in nature into intimate connection with experience gained by other methods of study are still incomplete, particularly because most theories are based on classicalhydrodynamics, which deal with wave motion in an idealized fluid. -
Thompson/Ocean 420/Winter 2005 Tide Dynamics 1
Thompson/Ocean 420/Winter 2005 Tide Dynamics 1 Tide Dynamics Dynamic Theory of Tides. In the equilibrium theory of tides, we assumed that the shape of the sea surface was always in equilibrium with the forcing, even though the forcing moves relative to the Earth as the Earth rotates underneath it. From this Earth-centric reference frame, in order for the sea surface to “keep up” with the forcing, the sea level bulges need to move laterally through the ocean. The signal propagates as a surface gravity wave (influenced by rotation) and the speed of that propagation is limited by the shallow water wave speed, C = gH , which at the equator is only about half the speed at which the forcing moves. In other t = 0 words, if the system were in moon equilibrium at a time t = 0, then by the time the Earth had rotated through an angle , the bulge would lag the equilibrium position by an angle /2. Laplace first rearranged the rotating shallow water equations into the system that underlies the tides, now known as the Laplace tidal equations. The horizontal forces are: acceleration + Coriolis force = pressure gradient force + tractive force. As we discussed, the tide producing forces are a tiny fraction of the total magnitude of gravity, and so the vertical balance (for the long wavelength appropriate to tidal forcing) remains hydrostatic. Therefore, the relevant force, the tractive force, is the projection of the tide producing force onto the local horizontal direction. The equations are the same as those that govern rotating surface gravity waves and Kelvin waves. -
Tides Education Standards, Grades 9-12 Overview Physical Science Life Science
Standards Addressed National Science Lesson 10: Tides Education Standards, Grades 9-12 Overview Physical science Life science Lesson 10 describes the basic causes of tides and defines Ocean Literacy the fundamental terminology scientists use to categorize Principles and characterize tides. Students observe tidal charts and The Earth has one big describe reasons tides are important to humans and ocean with many marine life. In the activity, students research creatures of features the intertidal zone and describe the types of physical and behavioral adaptations that allow organisms to thrive in DCPS, High School this harsh environment. Earth Science ES.5.3. Identify and explain Lesson Objectives the mechanisms that cause and modify the production of tides, such as the Students will: gravitational attraction of the 1. Identify the gravitational effects of the sun and the moon, the sun, and coastal moon on the Earth as the primary determinants of topography tides 2. Differentiate spring and neap tides 3. Define the intertidal zone and describe adaptations of common organisms that live in these zones Lesson Contents 1. Teaching Lesson 10 a. Introduction b. Lecture Notes c. Additional Resources 2. Teacher’s Edition: Creatures of the Intertidal 3. Student Activity: Creatures of the Intertidal 4. Student Handout 5. Mock Bowl Quiz 1 | P a g e Teaching Lesson 10 Lesson 10 Lesson Outline1 I. Introduction To introduce the students to the concept of tides, lead them through a brief presentation of NOAA tide prediction data (slide 3). Ask students if they have ever heard of tides and if they can define them. A tide is the periodic rise and fall of a body of water due to gravitational interactions between the sun, moon and Earth. -
Astronomy 518 Astrometry Lecture
Astronomy 518 Astrometry Lecture Astrometry: the branch of astronomy concerned with the measurement of the positions of celestial bodies on the celestial sphere, conditions such as precession, nutation, and proper motion that cause the positions to change with time, and corrections to the positions due to distortions in the optics, atmosphere refraction, and aberration caused by the Earth’s motion. Coordinate Systems • There are different kinds of coordinate systems used in astronomy. The common ones use a coordinate grid projected onto the celestial sphere. These coordinate systems are characterized by a fundamental circle, a secondary great circle, a zero point on the secondary circle, and one of the poles of this circle. • Common Coordinate Systems Used in Astronomy – Horizon – Equatorial – Ecliptic – Galactic The Celestial Sphere The celestial sphere contains any number of large circles called great circles. A great circle is the intersection on the surface of a sphere of any plane passing through the center of the sphere. Any great circle intersecting the celestial poles is called an hour circle. Latitude and Longitude • The fundamental plane is the Earth’s equator • Meridians (longitude lines) are great circles which connect the north pole to the south pole. • The zero point for these lines is the prime meridian which runs through Greenwich, England. PrimePrime meridianmeridian Latitude: is a point’s angular distance above or below the equator. It ranges from 90° north (positive) to 90 ° south (negative). • Longitude is a point’s angular position east or west of the prime meridian in units ranging from 0 at the prime meridian to 0° to 180° east (+) or west (-).