【发布时间】:2022-01-22 01:40:41
【问题描述】:
我写了一个程序来计算流体静力太阳大气的等离子体β:
B_0 = 0.02 # base magnetic field [T]
p_0 = 0.015 # base pressure [J/m^-3]
h_D = 7.5E7 # dipole depth [m]
R_☉ = 6.96E8 # solar radius [m]
M_☉ = 1.9891E30 # solar mass [kg]
G = 6.673E-11 # gravitational constant [m^3 kg^-1 s^-2]
μ = 0.61 # mean molecular weight of solar corona
m_H = 1.6726E-27 # mass of H particle [kg]
μ_0 = (4*pi)*10^(-7) # permeability [H/m]
k = 1.3806E-23 # boltzmann constant [J/K]
T = 1E6 # temperature [K]
g = (G*M_☉)/(R_☉^2)
lambda_p = (k*T)/(μ*m_H*g) # coronal scale height for 1MK [m]
p(h) = p_0*exp(-h/lambda_p)
B(h) = B_0*(1 + (h/h_D))^(-3)
beta = p(h)/(B(h)^2 / (2*μ_0) )
我对使用迭代/数值方法不是很熟悉,想知道是否有办法在beta = 1 时确定h 的值?
【问题讨论】:
标签: julia