Spontaneous Emissions
Random observations from excited states
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Eddington Experiment

I have chronicled my efforts to reproduce the work of Sir Arthur Eddington in confirming the predictions of Einstein’ General Relativity Theory.  Here are some entry points.

Intro to the Modern Eddington Experiment

Intro to celestial coordinates 

The overall step by step plan to measure star deflections

Step EE-1, Detect the star locations in a photograph

Step EE-2: Transform to reference coordinates

Step EE-3: Finding the best fit

Eclipse Day!

Comparing Before and During images, step EE-4

Analyzing Eclipse Day Results

Discussion

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    • And now for something completely different.
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    • Comparing Before and During images, step EE-4
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  • The “Modern Eddington Experiment”: Spontaneous Emissions

    And now for something completely different.

    Sometimes, when I try to describe to others what I do as a color scientist, I am asked if I can fix their photos.  Usually it is to make their printer look more like their monitor, but a few years ago it was a friend asking about how to correct his underwater pictures while scuba […]

    Eddington epilogue

    I was lucky to have ended up at this observing location with such excellent weather. When planning to view total eclipses, I am advised to arrange for other activities as well; the eclipse itself is subject to fickle viewing conditions (my one prior total solar eclipse effort was thwarted, but the travel experience was rewarding […]

    Discussion

    It is a bit disappointing to be unable to show a clear gravitational signal, even with all of the successful exposures that were taken, but I recognized the difficulty of this measurement early on. In addition to the variables I anticipated, there are some additional uncertainties that I now recognize. Here is my updated list […]

    Analyzing Eclipse Day Results

    I was able to obtain 35 photos during totality that were candidates to locate stars in the field. The exposures ranged from 1/60 to 2 seconds, but it became clear after applying the detection procedure starPos.m, that only the longest exposures, 1 and 2 seconds, would yield detected stars. The inner regions of the corona […]

    Comparing Before and During images, step EE-4

    This was written prior to eclipse day as I was contemplating how to compare the two image sets.  I include it here to keep the thought sequence intact.   When we apply steps EE-1, 2, and 3 to both the before images and the during images, we will have a set of radial distances to […]

Spontaneous Emissions
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