## Classical ElectrodynamicsProblems after each chapter |

### From inside the book

Results 1-3 of 77

Page 220

E

Nu'e ' sin 2r + sin ( i + r ) cos ( i - r ) u sin 2i u ' M sin 2i sin 2r E. " tan ( i E. sin 2r +

и tan ( i + r ) M sin 2i μ ' Again the results on the right apply for ui ' = M. For ...

E

**PARALLEL**TO PLANE OF INCIDENCE E. ' = 2 ( 7.60 ) иє sin 2i 2 cos i sin r EONu'e ' sin 2r + sin ( i + r ) cos ( i - r ) u sin 2i u ' M sin 2i sin 2r E. " tan ( i E. sin 2r +

и tan ( i + r ) M sin 2i μ ' Again the results on the right apply for ui ' = M. For ...

Page 331

where we have introduced a vectorial Alfvén velocity : B. ( 10.70 ) 4πρ The wave

equation ( 10.69 ) for v , is somewhat involved , but it allows simple solutions for

waves propagating

where we have introduced a vectorial Alfvén velocity : B. ( 10.70 ) 4πρ The wave

equation ( 10.69 ) for v , is somewhat involved , but it allows simple solutions for

waves propagating

**parallel**or perpendicular to the magnetic field direction .Page 476

comparable

component is negligible ( of order 1/72 ) compared to that from the perpendicular

...

**parallel**to and perpendicular to the velocity . But we have just seen that forcomparable

**parallel**and perpendicular forces the radiation from the**parallel**component is negligible ( of order 1/72 ) compared to that from the perpendicular

...

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### Contents

Introduction to Electrostatics | 1 |

References and suggested reading | 23 |

Multipoles Electrostatics of Macroscopic Media | 98 |

Copyright | |

6 other sections not shown

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