[1] import astropy.units as u import matplotlib.pyplot as plt import numpy as np from astropy.constants import h, m_e, k_B from astropy.constants import u as atomicu def Saha (T,Z_i,Z_ii,E_ionize,P_e): N_iitoi = N_iitoi = N_iitoi.decompose() return (N_iitoi) 2*k_B*T*Z_ii/(P_e*Z_i)*(2*np.pi*m_e*k_B*T/h**2)**(3/2)*np.exp(-E_ionize/(k_B*T)) [3] def Boltzmann_H(T, low, high): g_low = 2*low**2 g_high = 2*high**2 E_low = -13.6/low**2*u.eV E_high = -13.6/high**2*u.ev exponent = −1* (E_high-E_low)/(k_B*T) exponent = exponent.decompose() N_htol = g_high/g_low*np.exp(exponent) N_htol = N_htol.decompose() return (N_htol)
[1] import astropy.units as u import matplotlib.pyplot as plt import numpy as np from astropy.constants import h, m_e, k_B from astropy.constants import u as atomicu def Saha (T,Z_i,Z_ii,E_ionize,P_e): N_iitoi = N_iitoi = N_iitoi.decompose() return (N_iitoi) 2*k_B*T*Z_ii/(P_e*Z_i)*(2*np.pi*m_e*k_B*T/h**2)**(3/2)*np.exp(-E_ionize/(k_B*T)) [3] def Boltzmann_H(T, low, high): g_low = 2*low**2 g_high = 2*high**2 E_low = -13.6/low**2*u.eV E_high = -13.6/high**2*u.ev exponent = −1* (E_high-E_low)/(k_B*T) exponent = exponent.decompose() N_htol = g_high/g_low*np.exp(exponent) N_htol = N_htol.decompose() return (N_htol)
Computer Networking: A Top-Down Approach (7th Edition)
7th Edition
ISBN:9780133594140
Author:James Kurose, Keith Ross
Publisher:James Kurose, Keith Ross
Chapter1: Computer Networks And The Internet
Section: Chapter Questions
Problem R1RQ: What is the difference between a host and an end system? List several different types of end...
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Answer in Python. Given this code to start with (definitions for the Saha and Boltzmann Equations), I must: use the Saha equation (defined in the second code block) to find the temperature of the partial ionization zone for a certain gas.
(Hint: The Saha function will return answers for the Saha equation for gases of arbitrary composition)
![[1] import astropy.units as u
import matplotlib.pyplot as plt
import numpy as np
from astropy.constants import h, m_e, k_B
from astropy.constants import u as atomicu
def Saha (T,Z_i,Z_ii,E_ionize,P_e):
N_iitoi = 2*k_B*T*Z_ii/(P_e*Z_i)*(2*np.pi*m_e*k_B*T/h**2)**(3/2)*np.exp(-E_ionize/(k_B*T))
N_iitoi = N_iitoi.decompose()
return (N_iitoi)
[3] def Boltzmann_H(T,low, high):
g_low
2*low**2
g_high 2*high**2
E low =
=
-13.6/low**2*u.eV
E_high = -13.6/high**2*u.eV
exponent = -1* (E_high-E_low)/(k_B*T)
exponent = exponent.decompose()
N htol g_high/g_low*np.exp(exponent)
N_htol N_htol.decompose()
return (N_htol)](/v2/_next/image?url=https%3A%2F%2Fcontent.bartleby.com%2Fqna-images%2Fquestion%2Fe3c23c7f-c566-42d4-a739-9c42cf68404f%2F50aefa86-46e0-4963-8844-9bccab99e8b5%2Feuuseoc_processed.png&w=3840&q=75)
Transcribed Image Text:[1] import astropy.units as u
import matplotlib.pyplot as plt
import numpy as np
from astropy.constants import h, m_e, k_B
from astropy.constants import u as atomicu
def Saha (T,Z_i,Z_ii,E_ionize,P_e):
N_iitoi = 2*k_B*T*Z_ii/(P_e*Z_i)*(2*np.pi*m_e*k_B*T/h**2)**(3/2)*np.exp(-E_ionize/(k_B*T))
N_iitoi = N_iitoi.decompose()
return (N_iitoi)
[3] def Boltzmann_H(T,low, high):
g_low
2*low**2
g_high 2*high**2
E low =
=
-13.6/low**2*u.eV
E_high = -13.6/high**2*u.eV
exponent = -1* (E_high-E_low)/(k_B*T)
exponent = exponent.decompose()
N htol g_high/g_low*np.exp(exponent)
N_htol N_htol.decompose()
return (N_htol)
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