1-3 Appendix A

The elements of the diffusion matrix, D, are given by

(A1)Dαα=∑n=−∞∞∫0∞k⊥dk⊥Dααnk⊥(A2)Dαp=Dpα=∑n=−∞∞∫0∞k⊥dk⊥Dαpnk⊥(A3)Dpp=∑n=−∞∞∫0∞k⊥dk⊥Dppnk⊥

For each harmonic resonance number n and k⊥, the pitch-angle diffusion coefficient Dααnk⊥ is given by

(A4)Dααnk⊥=limV→∞qσ24πV[nΩσ/(γω)−sin2⁡αcos⁡α]2|Θnk|2|v∥−∂ω∂k∥||k∥

The right-hand side of equation (A4) is evaluated at the resonant parallel wave number k∥ and frequency ω that satisfies the resonance condition

(A5)ω−k∥v∥=nΩσ/γ

The value of Θnk is given by

(A6)Θnk=v∥v⊥Ek,∥Jn+Ek,LJn−1+Ek,RJn+12

where Jn is the n-th order Bessel function with argument k⊥p⊥/(mσΩσ), and the Fourier transform of the wave electric field has been written in terms of its parallel Ek,∥, left-hand Ek,L, and right-hand Ek,R, components, with

(A7)Ek,L=12(Ek,x+iEk,y)(A8)Ek,R=12(Ek,x−iEk,y)

From equations A7 and A8, we can easily solve for Ek,x and Ek,y:

(add)Ek,x=12(Ek,L+Ek,R),Ek,y=1i2(Ek,L−Ek,R)

Using cold plasma theory, Ek,L and Ek,R can be rewritten in terms of Ek,∥, the refractive index μ, the wave-normal angle ψ, and the Stix parameters R,L,S,D, and P [Lyons, 1974b], to give

(A9)Ek,L=(μ2sin2⁡ψ−Pμ2sin⁡ψcos⁡ψ)(1−D(μ2−S))Ek,∥2(A10)Ek,R=(μ2sin2⁡ψ−Pμ2sin⁡ψcos⁡ψ)(1+D(μ2−S))Ek,∥2

The Stix parameters are defined as:

(add)R=1−∑σωpσ2ω(ω−Ωσ)L=1−∑σωpσ2ω(ω+Ωσ)P=1−∑σωpσ2ω2S=R+L2D=R−L2

The Maxwell-Faraday equation in Fourier space is:

(add)k×Ek=ωBk→|Ek,⊥|=c|Bk|

and

(add)|Ek|2=|Ek,∥|2+|Ek,⊥|2=|Ek,x|2+|Ek,y|2

Thus, Ek,∥ can be written as a function of the magnitude of the Fourier transform of the wave magnetic field at each k, namely |Bk|:

(A11)|Ek,∥|2=c2|Bk|2μ2⋅[(R−L2(μ2−S))2(μ2sin2⁡ψ−Pμ2sin⁡ψcos⁡ψ)2+(Pμ2sin⁡ψ)2]−1

Combining these results gives

(A12)|Θnk|2=c2|Bk|2μ2|Φn,k|2

with

(A13)|Φn,k|2={[(μ2−Lμ2−S)Jn+1+(μ2−Rμ2−S)Jn−1](μ2sin2⁡ψ−P2μ2)+cot⁡αsin⁡ψcos⁡ψJn}2(R−L2(μ2−S))2(P−μ2sin2⁡ψμ2)2+(Pcos⁡ψμ2)2

We assume that the wave magnetic field can be described by [Lyons, 1974b]

(A14)|Bk|2=VN(ω)B2(ω)g(ψ)

with

(A15)N(ω)=12π2∫XminXmaxg(X)|J(k⊥,k∥ω,X)|k⊥dX

Here B2(ω) is the wave magnetic field intensity squared per unit frequency and g(X) gives the variation of wave magnetic field energy with wave normal angle,

(add)g(X)={exp⁡[−(X−XmXw)2]Xmin≤X≤Xmax0otherwise,with X=tan⁡(ψ)

Using the cold plasma dispersion relation D(k,ω,X)=0, and the Jacobian J(k∥,k⊥ω,X), A15 can be rewritten to obtain the equation (see 1-3 Appendix B):

(add)N(ω)=12π2∫XminXmaxg(X)k2(1+X2)32∂D∂ω[∂D∂k]−1XdX

Combining equations (A1)–(A3), (A4), and (A12) and transforming the integrals from k⊥ to X leads to the final form of the diffusion coefficients' expression:

Dαα=∑n=nlnh∫XminXmaxXdXDααnXDαp=Dpα=∑n=nlnh∫XminXmaxXdXDαpnXDpp=∑n=nlnh∫XminXmaxXdXDppnX

with

DααnX=∑iqσ2ωi24π(1+X2)N(ωi)[nΩσ/(γωi)−sin2⁡αcos⁡α]2⋅B2(ωi)g(X)|Φn,k|2|v∥−∂ω∂k∥||k||iDαpnX=DααnX[sin⁡αcos⁡αnΩσ/(γωi)−sin2⁡α]k||iDppnX=DααnX[sin⁡αcos⁡αnΩσ/(γωi)−sin2⁡α]k||i2