SOLAR ECLIPSE

The image I included in the section titled "The Theoretical Aspect of Alice Law" in the book might have caught your attention. That image is truly extraordinary, revealing all the beauty and secrets of (c+v)(c-v) Mathematics. I can only obtain such images with the help of animations that use intensive mathematical calculations. Here, I will show you the animation of that image.

I recommend familiarizing yourself with (c+v)(c-v) Mathematics before watching this animation and even leaving this animation for the later stages of your exploration. Otherwise, what you see might challenge you. When I ran this animation for the first time, I was greatly surprised by what I saw.

SOLAR ECLIPSE I
The observer is advancing along their own trajectory. There is a Sun and a Moon on their path. In the animation, we will observe moment by moment how the observer perceives the Sun and the Moon.

Information about the flow of the animation:
As we press the play button, the observer begins to move along their trajectory, and at the same time, signals start coming from the Sun and the Moon towards the observer.
As the signals reach the observer, we see that the Image Objects of the Sun and Moon, influenced by Dimension Shift, are formed. The animation shows the Image Objects only with their outer outlines. Therefore, the Image Objects are hollow. Around the middle of the animation, the Moon's mass begins to shadow some of the signals coming from the Sun, preventing them from reaching the observer. As a result, the observer begins to see the solar eclipse.
The red areas in the Sun's Image Object show the parts corresponding to the signals that are shadowed by the Moon.
Over time, the Moon's shadowing ends, and as the solar eclipse for the observer also nears its end, the animation concludes.

SOLAR ECLIPSE II
This animation was created using the Bitmap technique. The Bitmap technique cannot show continuous animation. Therefore, in this animation, we only obtain a single frame corresponding to a specific moment. The animation presents the Dimension Shift in the Image Objects of the Sun and Moon in full detail. When the Electromagnetic Wave Packet reaches the observer (end of animation), the observer perceives the Image Objects of the Sun and Moon.

SOLAR ECLIPSE III
In this animation, the Continuous technique and Bitmap technique are used together. After starting the animation, watch it until the end.