File:Twilight illumination by sun altitude luxes 2 r 1.svg

From Wikimedia Commons, the free media repository
Jump to navigation Jump to search

Original file (SVG file, nominally 1,247 × 771 pixels, file size: 57 KB)

Captions

Captions

Illumination of twilight by sun altitude degrees

Summary

[edit]
Description
English: Illumination of twilight by sun altitude degrees
Date
Source Own work
Author Merikanto

Python source code

based on data from R "moonlit" package

https://github.com/msmielak/moonlit

Original source of data

        1. Twilight illumination from empirical data https://www.jstor.org/stable/44612241
        1. Sun Position and Twilight Times for Driver Visibility Assessment; Duane D.
        2. MacInnis, Peter B. Williamson and Geoffrey P. Nielsen; SAE Transactions;
        3. Vol. 104, Section 6: JOURNAL OF PASSENGER CARS: Part 1 (1995), pp. 759-783
        1. Values calulated from the paper for angles -18 to 5 degrees, by 0.25 degree, imported to R and spline function applied

Python3 polyfit code

    1. illumination of twilight
    2. python3 source code
    3. 19.8.2023 0000.0000

import math import numpy as np import matplotlib.pyplot as plt

    1. uses data from
    2. https://github.com/msmielak/moonlit
        1. Twilight illumination from empirical data https://www.jstor.org/stable/44612241
        1. Sun Position and Twilight Times for Driver Visibility Assessment; Duane D.
        2. MacInnis, Peter B. Williamson and Geoffrey P. Nielsen; SAE Transactions;
        3. Vol. 104, Section 6: JOURNAL OF PASSENGER CARS: Part 1 (1995), pp. 759-783
        1. Values calulated from the paper for angles -18 to 5 degrees, by 0.25 degree, imported to R and spline function applied

sun_altitudes0=np.array([5,4.75,4.5,4.25,4,3.75,3.5,3.25,3,2.75,2.5,2.25,2,1.75,1.5,1.25,1,0.75,0.5,0.25,0,-0.25,-0.5,-0.75,-1,-1.25,-1.5,-1.75,-2,-2.25,-2.5,-2.75,-3,-3.25,-3.5,-3.75,-4,-4.25,-4.5,-4.75,-5,-5.25,-5.5,-5.75,-6,-6.25,-6.5,-6.75,-7,-7.25,-7.5,-7.75,-8,-8.25,-8.5,-8.75,-9,-9.25,-9.5,-9.75,-10,-10.25,-10.5,-10.75,-11,-11.25,-11.5,-11.75,-12,-12.25,-12.5,-12.75,-13,-13.25,-13.5,-13.75,-14,-14.25,-14.5,-14.75,-15,-15.25,-15.5,-15.75,-16,-16.25,-16.5,-16.75,-17,-17.25,-17.5,-17.75,-18]) sun_illuminations0=np.array([4499.368645,4251.166227,4010.398231,3776.215801,3547.994929,3325.316934,3107.949504,2895.827638,2689.034018,2487.778469,2292.376367,2103.225979,1920.784922,1745.546056,1578.01326,1418.677674,1267.99505,1126.364901,994.1121318,871.4718063,758.577575,655.4541802,562.0142693,478.0595544,404.556034,338.5269901,281.0455199,231.5470057,189.3612856,153.7599131,123.995336,99.33178815,79.06826738,62.55436811,49.1999767,38.47993901,29.93480689,23.16869331,17.84514167,13.68176809,10.44428227,7.911259933,5.993606008,4.527348005,3.411591605,2.566090598,1.927671576,1.447053311,1.086102387,0.815522737,0.612949604,0.461403805,0.348056383,0.263253638,0.199755997,0.152149406,0.116393841,0.089479462,0.069166322,0.053788354,0.04210643,0.033198579,0.026378238,0.02113351,0.017082103,0.01393796,0.01148655,0.009566583,0.008056477,0.006931022,0.00596833,0.00519104,0.004556611,0.004033257,0.003596965,0.003229411,0.002916468,0.002647147,0.002412827,0.002206692,0.002023321,0.001858385,0.001708419,0.001570657,0.001442901,0.001323428,0.001210913,0.001104369,0.001003101,0.000906659,0.000814804,0.000727464,0.000644703])

sun_altitudes1=sun_altitudes0[::-1] sun_illuminations1=sun_illuminations0[::-1] log_sun_illuminations2=np.log10(sun_illuminations0[::-1])

fit1=np.polyfit(sun_altitudes1,log_sun_illuminations2,6) poly1=np.poly1d(fit1)

altitudes2=np.linspace(-18,5,230)

  1. altitudes2=np.linspace(-18,90,900+180)

log_illums2=poly1(altitudes2)

  1. print(log_illums2)

fig = plt.figure() ax = fig.gca() ax.set_xticks(np.arange(-21, 6, 3)) ax.set_yticks(np.arange(-4, 4,0.5))

plt.xlabel("Altitude of Sun, degrees", size=18) plt.ylabel("Log10 of illumination lx", size=18)

plt.yticks(fontsize=18) plt.xticks(fontsize=18)

plt.suptitle("Illumination of twilight, luxes", fontsize=22) plt.title("From empirical data", fontsize=18)

  1. plt.plot(alts1, logillums1, linewidth=6, color="#ff7f00")
  2. plt.plot(x2,y2,linewidth=6, color="#ff7f00" )
  1. plt.plot(altitude, log10_lux, linestyle=":", linewidth=4, color="#ffff00")

plt.plot(altitudes2, log_illums2,color="#ff7f00", linewidth=6 ) plt.scatter(sun_altitudes1, log_sun_illuminations2, marker='+', color="red")

plt.grid()

plt.axvline(x = 0, color = '#FFFF00', label = 'Sunset') plt.axvline(x = -6, color = '#7f7f00', label = 'Civil twilight ends') plt.axvline(x = -12, color = '#3f3f00', label = 'Nautical twilight ends') plt.axvline(x = -18, color = '#1f1f00', label = 'Astronomical twilight ends')

plt.text(-5, 0, "Civil twilight", size=17) plt.text(-11.5, -1, "Nautical twilight", size=17) plt.text(-17.5, -2, "Astronomical twi.", size=17)

plt.show()


Licensing

[edit]
I, the copyright holder of this work, hereby publish it under the following license:
w:en:Creative Commons
attribution share alike
This file is licensed under the Creative Commons Attribution-Share Alike 4.0 International license.
You are free:
  • to share – to copy, distribute and transmit the work
  • to remix – to adapt the work
Under the following conditions:
  • attribution – You must give appropriate credit, provide a link to the license, and indicate if changes were made. You may do so in any reasonable manner, but not in any way that suggests the licensor endorses you or your use.
  • share alike – If you remix, transform, or build upon the material, you must distribute your contributions under the same or compatible license as the original.

File history

Click on a date/time to view the file as it appeared at that time.

Date/TimeThumbnailDimensionsUserComment
current12:20, 19 August 2023Thumbnail for version as of 12:20, 19 August 20231,247 × 771 (57 KB)Merikanto (talk | contribs)Uploaded own work with UploadWizard

There are no pages that use this file.

Metadata