File:Sunspots seen by azimutal observer during day.gif

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Sunspots_seen_by_azimutal_observer_during_day.gif (480 × 480 pixels, file size: 252 KB, MIME type: image/gif, looped, 30 frames, 3.0 s)

Captions

Captions

Due to earth roration aziumutal observer see a rotation of image plane during a day.

Summary

[edit]
Description
English: Earth rotation is responsible for rotation of image plane when observed by azimutal mounted telescope or simply observed by looking at sun (through protecting glass). The image simulates the rotation from morning till evening. Rotation angle was calculated according (thanks to Rolf Hempel, 2024):

Tubas (talk) from math import sin, cos, asin, acos, radians, degrees, pi

def equatorial_to_azimuth(rect, decl, sideral_time, latitude):

   """
   Convert equatorial coordinates in azimuthal ones.
   :param rect: Right ascension of the object (in radians)
   :param decl: Declination of the object (in radians)
   :param sideral_time: Sideral time (in radians)
   :param latitude: Geographical latitude of the observer
   :return: azimuth, height, position angle with:
            azimuth: equatorial azimuth angle of the object (in radians)
            height: equatorial height of the object (in radians)
            position angle: rotation of northern direction relative to vertical at the object
                            (in radians), positive in clockwise direction
   """
   h = asin(sin(latitude) * sin(decl) + cos(latitude) * cos(decl) * cos(rect - sideral_time))
   dir_from_south = (rect - sideral_time + 2. * pi) / (2. * pi) % 1.
   if dir_from_south > 0.5:
       P = acos((sin(latitude) - sin(h) * sin(decl)) / (cos(h) * cos(decl)))
       az = 2. * pi - acos(
           -cos(P) * cos(rect - sideral_time) + sin(P) * sin(rect - sideral_time) * sin(decl))
   else:
       P = - acos((sin(latitude) - sin(h) * sin(decl)) / (cos(h) * cos(decl)))
       az = acos(
           -cos(P) * cos(rect - sideral_time) + sin(P) * sin(rect - sideral_time) * sin(decl))
   return az, h, P

if __name__ == '__main__':

   rect = radians(180.)
   decl = radians(0.)
   latitude = radians(50.)
   sideral_time = radians(90.)
   azimuth, height, position_angle = equatorial_to_azimuth(rect, decl, sideral_time, latitude)
   print("Azimuth: " + str(degrees(azimuth)) + ", height: " + str(
       degrees(height)) + ", Rotation of north relative to vertical: " + str(degrees(position_angle)))

Tubas (talk)

The image is based on photo taken by Rolf Hempel, see: File:Hempel 2024-08-24 08-14-10MESZ Sonne.jpg, animation done by Tubas
Date
Source Source: Rolf Hempel (2024)
Author Rolf Hempel (2024)

Licensing

[edit]
w:en:Creative Commons
attribution
This file is licensed under the Creative Commons Attribution 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.

File history

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Date/TimeThumbnailDimensionsUserComment
current08:25, 18 September 2024Thumbnail for version as of 08:25, 18 September 2024480 × 480 (252 KB)Tubas (talk | contribs)Uploaded a work by Rolf Hempel (2024) from Source: Rolf Hempel (2024) with UploadWizard

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