Experiment

Sunspot Orientation Comparison

At the same UTC moment, does the same sunspot pattern rotate with observer location the way globe-Earth viewing geometry predicts?

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Materials Needed

  • Sunspot Observer tool or real solar images captured at the same UTC time
  • two or three observer locations, ideally northern hemisphere, near-equator, and southern hemisphere
  • shared UTC clock or timestamp agreement
  • safe solar telescope setup with a proper full-aperture solar filter if you are capturing your own images
  • screenshots, sketches, or notes for side-by-side comparison

Setup Steps

  1. Pick one UTC timestamp and keep it fixed for every observer or generated view.
  2. Choose at least two locations at different latitudes, and preferably three: north, near-equator, and south.
  3. Use the same real sunspot snapshot or the same generated SVG baseline pattern for every location.
  4. Place the results side by side without changing the underlying spot pattern or relabeling the disk.
  5. Compare how the solar disk and spot pattern rotate from one location to the next.

Expected Calculation

spot pattern=same at one UTC instant
x=cos(lat) × sin(CMD)
y=sin(lat)
disk roll=parallactic-angle frame rotation by latitude

The same solar pattern should stay internally consistent while the apparent disk orientation changes with observer frame. Northern and southern hemisphere views can differ strongly, often approaching a half-turn, while near-equatorial views sit between them.

Graphic

This visual shows the core geometry the experiment is testing before the real-world observation is made.

Same Sun, same UTC moment, different observer latitude.The spot pattern stays the same while the apparent orientation rotates.northNorthern latitudenorthNear equatornorthSouthern latitudeCompare the same timestamp and the same identified spot groups. Orientation changes by location.

What to Observe

  • The same major spot groups remain identifiable from panel to panel instead of turning into different patterns.
  • What changes is the orientation of the disk and spot layout, not the identity of the pattern itself.
  • Northern and southern observers can see the same pattern rotated in noticeably different directions at the same UTC moment.
  • A near-equatorial observer usually lands between those two orientations rather than matching either extreme.

Interpretation

Same object, same time, different location leading to different apparent orientation is what you expect when observers stand on different parts of a curved Earth and view the same Sun from different local frames. This is best used as side-by-side supporting evidence together with real timestamps and repeatable comparisons.

Sources

Evidence Card

Claim

At the same UTC moment, does the same sunspot pattern rotate with observer location the way globe-Earth viewing geometry predicts?

Model Used

The experiment’s stated geometry or physical model with fixed inputs across comparisons.

Formula

spot pattern=same at one UTC instant
x=cos(lat) × sin(CMD)
y=sin(lat)
disk roll=parallactic-angle frame rotation by latitude

Last Verified

2026-06-30

Assumptions

  • The protocol holds location, height, and distance inputs fixed while comparing observation to prediction.
  • A single ambiguous photo is not enough; repeatable measurements matter.
  • Primary-source references carry more weight than generic summaries.

What Would Falsify This Page

A repeatable observation that matched the competing model better than this experiment’s stated prediction would count against this page.

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