ECE 6382 Fall 2020 David R Jackson Notes

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ECE 6382 Fall 2020 David R. Jackson Notes 21 Modified Bessel Functions and Kelvin

ECE 6382 Fall 2020 David R. Jackson Notes 21 Modified Bessel Functions and Kelvin Functions Notes are from D. R. Wilton, Dept. of ECE 1

Modified Bessel Functions Modified Bessel differential equation: This comes from the Bessel differential equation:

Modified Bessel Functions Modified Bessel differential equation: This comes from the Bessel differential equation: The modified Bessel functions are Bessel functions of imaginary argument. 2

Modified Bessel Function of the First Kind Definition: (I is a real function of

Modified Bessel Function of the First Kind Definition: (I is a real function of x. ) To see this, use the Frobenius solution for J : Frobenius series solution for I : 3

Second Solution of Modified Bessel Equation For n, the modified Bessel function of the

Second Solution of Modified Bessel Equation For n, the modified Bessel function of the 2 nd kind is defined as: For = n (an integer): 4

Relations Between Bessel and Modified Bessel Functions The modified Bessel functions are related to

Relations Between Bessel and Modified Bessel Functions The modified Bessel functions are related to the regular Bessel functions as Note: The added factors in front ensure that the functions are real. *comes from: 5

Small Argument Approximations For small arguments we have: 6

Small Argument Approximations For small arguments we have: 6

Large Argument Approximations For large arguments we have: 7

Large Argument Approximations For large arguments we have: 7

Plots of Modified Bessel Functions for Real Arguments I 0 I 1 I 2

Plots of Modified Bessel Functions for Real Arguments I 0 I 1 I 2 The In functions increase exponentially. They are finite at x = 0. 8

Plots of Modified Bessel Functions for Real Arguments K 1 K 2 K 0

Plots of Modified Bessel Functions for Real Arguments K 1 K 2 K 0 The Kn functions decrease exponentially. The are infinite at x = 0. 9

Recurrence Relations Some recurrence relations are: 10

Recurrence Relations Some recurrence relations are: 10

Wronskian A Wronskian identity is: 11

Wronskian A Wronskian identity is: 11

Kelvin Functions The Kelvin functions are defined as Note: These are important for studying

Kelvin Functions The Kelvin functions are defined as Note: These are important for studying the fields inside of a conducting wire. 12

Kelvin Functions (cont. ) The Ber functions increase exponentially. They are finite at x

Kelvin Functions (cont. ) The Ber functions increase exponentially. They are finite at x = 0. Ber 0 Ber 1 Ber 2 13

Kelvin Functions (cont. ) The Bei functions increase exponentially. They are finite at x

Kelvin Functions (cont. ) The Bei functions increase exponentially. They are finite at x = 0. Bei 1 Bei 2 Bei 0 14

Kelvin Functions (cont. ) Normalizing makes it more obvious that the Ber and Bei

Kelvin Functions (cont. ) Normalizing makes it more obvious that the Ber and Bei functions increase exponentially and also oscillate. x 15

Kelvin Functions (cont. ) Normalizing makes it more obvious that the Ber and Bei

Kelvin Functions (cont. ) Normalizing makes it more obvious that the Ber and Bei functions increase exponentially and also oscillate. x 16

Kelvin Functions (cont. ) The Ker functions decay exponentially. They are infinite at x

Kelvin Functions (cont. ) The Ker functions decay exponentially. They are infinite at x = 0. Ker 0 Ker 1 17

Kelvin Functions (cont. ) The Kei functions decay exponentially. They are infinite at x

Kelvin Functions (cont. ) The Kei functions decay exponentially. They are infinite at x = 0. Kei 1 18

Kelvin Functions (cont. ) Normalizing makes it more obvious that the Ker and Kei

Kelvin Functions (cont. ) Normalizing makes it more obvious that the Ker and Kei functions decrease exponentially and also oscillate. 19

Kelvin Functions (cont. ) Normalizing makes it more obvious that the Ker and Kei

Kelvin Functions (cont. ) Normalizing makes it more obvious that the Ker and Kei functions decrease exponentially and also oscillate. 20