Normal Modes ß ß Normal modes of a string Normal modes of a sphere Þ Þ Spherical harmonics Radial variation � � Þ Þ ß Fundamental modes Overtone modes Torsional modes Spheroidal modes Observations of normal modes Þ Þ Overview 2004 Sumatra earthquake
Normal Modes of a String The boundaries make the modes! No boundaries, no discrete modes! (an infinitely long string would have continuous modes at all frequencies)
Propagating and Standing Waves Point source at position 8. Displacement of the string at time 1. 5.
Normal Modes of a Sphere (1) r: radial q: colatitude f: longitude
Generated by the great June 9, 1994 deep focus Bolivia earthquake. Recorded at Pasadena, California.
Spherical harmonics
Spherical harmonics
Spherical harmonics
Miaki Ishii
Radial Variations, Fundamental and Overtone Modes
Free oscillations of the earth (online animations) ß http: //lucien. saviot. free. fr/terre/index. en. html
For torsional mode, the number of nodal planes = l - 1
For torsional mode, the number of nodal planes = l - 1
For torsional mode, the number of nodal planes = l - 1
For spheriodal mode, the number of nodal planes = l
For spheriodal mode, the number of nodal planes = l
Observation of Normal Modes 1882 – Lamb – fundamental mode of Earth (as steel ball), 78 minutes 1911 – Love – included self-gravitation – fundamental mode period of 60 minutes 1952 – Kamchatka EQ is first to reveal Earth’s normal modes 1960 – Chile earthquake reveals over 40 modes
Free oscillation observed after the 2004 Sumatra earthquake
2004 Sumata Earthquake
Chandler wobble Earth is not perfect ellipsoid Predicted by Leonhard Euler Observed by
Summary ß ß Normal modes of a string Normal modes of a sphere Þ Þ Spherical harmonics Radial variation � � Þ Þ ß Torsional modes Spheroidal modes Observations of normal modes Þ Þ ¢ Fundamental modes Overtone modes Overview The 2004 Sumatra earthquake The Chandler Wobble