文件名称:EMFII-lecturenotes
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Electromagnetic theory is essentially a study of some particular field. We define a field
as a function which specifies a particular quantity everywhere in a region. If the quantity is a scalar (or vector), the field is said to be scalar (or vector) field. Examples of
scalar fields include temperature distribution in a building, sound intensity in a theater and
electric potential in a region. The gravitational force on a body in space, the velocity of
raindrops in the atmosphere and the velocity of fluid particles in a fluid motion are
examples of vector fields.
as a function which specifies a particular quantity everywhere in a region. If the quantity is a scalar (or vector), the field is said to be scalar (or vector) field. Examples of
scalar fields include temperature distribution in a building, sound intensity in a theater and
electric potential in a region. The gravitational force on a body in space, the velocity of
raindrops in the atmosphere and the velocity of fluid particles in a fluid motion are
examples of vector fields.
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下载文件列表
EMFII lecturenotes/Chapter 1.doc
EMFII lecturenotes/Chapter 1.pdf
EMFII lecturenotes/Chapter 2.doc
EMFII lecturenotes/Chapter 2.pdf
EMFII lecturenotes/Chapter 3.pdf
EMFII lecturenotes/Chapter 4.pdf
EMFII lecturenotes/Chapter 5.pdf
EMFII lecturenotes
EMFII lecturenotes/Chapter 1.pdf
EMFII lecturenotes/Chapter 2.doc
EMFII lecturenotes/Chapter 2.pdf
EMFII lecturenotes/Chapter 3.pdf
EMFII lecturenotes/Chapter 4.pdf
EMFII lecturenotes/Chapter 5.pdf
EMFII lecturenotes
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