Lunar Eclipse due to Electromagnetic Acceleration

According to the Flat Earth Theory's celestial model of Electromagnetic Acceleration the Lunar Eclipse occurs when the Moon travels out of bounds of the Sun's area of light. As result of the geometry of the Sun's curving rays the Lunar Eclipse can only occur on a Full Moon. The Lunar Eclipse can occur two to five times a year.

Lunar Phase Overview
When one observes the phases of the Moon they are seeing the Moon's day and night, a shadow created from the Sun illuminating half of the spherical Moon at any one time. As depicted in the previous section, due to EA we are always observing the nearside (or underside) of the Moon.

The curved rays of the Sun results in the phases upon the Moon's surface. The plane of the Moon's route is at an inclination to the plane of the Sun's ecliptic, with its highest side opposite from the Sun. When the Moon is far from the Sun and higher than it, the Full Moon occurs. When the Moon is closer to the Sun and lower than it, the New Moon occurs1. The Moon moves at a slightly slower rate than the Sun across the sky, causing the range of phases. The time between two Full Moons, or between successive occurrences of the same phase, is about 29.53 days (29 days, 12 hours, 44 minutes) on average.

Sample large-scale Sun ray diagram (side view):





Cause of Lunar Eclipse
Ass seen in the above, both the Moon and Sun follow similar paths near the ecliptic. On large scales light is curving upwards, as per Flat Earth's celestial model of Electromagnetic Acceleration. The Earth's presence limits the extent of the parabolic rays and blocks the light at the boundary from progressing outwards beyond a certain range. The Lunar Eclipse occurs on an occasion when the Moon is on the opposite side of the ecliptic from the Sun and its diurnal path wanders "out of bounds," intersecting the daylight boundary at the edges. Hence according to EA it is found that, after all, the shadow on the Moon during the Lunar Eclipse is the shadow of the Earth.

The scheme described above will follow a certain geometrical pattern. It can be predicted that the Lunar Eclipse will occur when:


 * - The Moon is Full
 * - The Moon is on opposite extremes of the Earth from the Sun
 * - The Moon and Sun are near their greatest latitudinal displacement from each other

Another consequence will be that the Lunar Eclipse will turn red, since the outer-most rays of the Sun create parabolic arcs which dip down and pass through the atmosphere of the Earth. When the Sun's light is horizontal against the atmosphere the light will turn red, as seen when the sky turns red during sunsets. It is also apparent that, since the Sun and Moon are on opposite extremes of the ecliptic during the Lunar Eclipse, the path which intersects the atmosphere will be through an area near the North Pole. If this geometry is true, it follows that conditions at the North Pole may affect the appearance of the Lunar Eclipse. And indeed, astronomers have noted an anomaly where during periods of high auroral activity the Lunar Eclipse has been seen to be very bright.

Curved Shadow
One of the original proofs for the rotundity of the world was the shape of the shadow on the Moon during a Lunar Eclipse. Aristotle reasoned that only a round earth could cause a round shadow. Since the shadow is round on the Moon, the Earth must also be round. Although a seemingly reasonable statement on the face of things, this is not necessarily the case. Since the surface of the Moon is that of a small convexly curved sphere, a flat or slightly concave shadow can display as convexly curved upon the Moon.

In a dark room place a flashlight onto a ledge, shining at a sphere eleven feet away. Use a book or folder to block the path of light, observing how the shadow behaves on the sphere.



We see that a shadow on a sphere curves on its own, due to the convexity of the sphere. Under FE-EA explanation for the Lunar Eclipse the shadow at the boundary is only slightly concave, as compared to the smaller convex surface of the Moon.

Lunar Eclipse Comparison
Compare the warping of the shadow in the above example to the shadow on the real Moon during a Lunar Eclipse:



Less than 180 degrees
Interestingly, during the eclipse the shadow seen does not travel straight across the Moon's face, but appears to turn mid-stride, making a 110 - 120 degree angle across its surface.

Under the EA model:



Lunar Eclipse Examples
In the below examples of the Lunar Eclipse notice that the shadow does not go straight across the Moon's face, but seems to make a turn mid-way through.







https://lrtimelapse.com/news/lunar-eclipse-2015-timelapse/ (Archive)



Griffith Observatory Runtime: 1m

Other videos

https://youtu.be/j1nVsCcKHwI

Additional:

http://www.astrosurf.com/cidadao/animations.htm http://www.oceanlight.com/spotlight.php?img=29411 https://www.youtube.com/watch?v=ziCVOhDsQzE - Lunar Eclipse, moon orientation non-corrected (az mount) https://en.m.wikipedia.org/wiki/Wikipedia:Featured_picture_candidates/Lunar_eclipse_time_lapse_still_image - near land, better orientation

Bright Lunar Eclipse
Under the FE-EA explanation it is seen that when the Sun and Moon are on opposite sides from each other the dipping rays must pass through the auroral zone on their way to the Moon. The Lunar Eclipse turns red due to the rays at the boundary edge passing horizontally through the atmolayer near the Earth's surface on their parabolic course. On occasion the Lunar Eclipse will be seen to be significantly brighter. It has been remarked by European astronomers that there is an association with the presence of the Aurora and bright occurrences of the Lunar Eclipse.

See the following remarks:

Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Nov 1845 - Jun 1847

[https://books.google.com/books?id=S7xAAAAAYAAJ&lpg=RA3-PA132&pg=RA3-PA132#v=onepage&q&f=false Remarkable Appearances during the total Eclipse of the Moon on March 19. 1848.] (Archive)

Extract of a Letter from Mr. Forster, Bruges.

Nature
Nature, Volume 16, p.287

OUR ASTRONOMICAL COLUMN (Archive)

The Observatory
The Observatory, A Montly Review of Astronomy - Vol. XXVI, 1903

Bright Lunar Eclipses (Archive)