I captured images once a minute before, during and after the total eclipse with a MallinCam DS10c camera inserted into my MCR-80ED refractor telescope on my SkyProdigy mount. I was inside where it was warm using Remote Video Astronomy to control the mount & camera and view the image live on my monitor.
After awhile the moon began to brighten…
If you compare the first image of the moon before the eclipse began and look through the images to the last one after it was over, the image of the moon appears rotated later in the evening. This is not due to the moon’s spin (once/month), but is due to the “field rotation” effect when using an Alt-Az mount.
I had thought about using an equatorial mount for viewing and recording the lunar eclipse to avoid any field rotation. The good news is the orientation of the moon would have remained the same in the captured image throughout the evening. But as the moon changes from being viewed to the east to being viewed to the west, a “meridian flip” occurs. The bad news is that to keep tracking the object past the meridian position with an equatorial mount, at some point you must stop tracking the object, flip your telescope from pointing east to point toward the west, and then resume tracking.
With an Alt-Az mount the telescope just keeps tracking the moon as it moves from east to west with no meridian flip to deal with. However, its view of the sky will rotate within the field of view. In fact, an Alt-Az mount “sees” the sky just like you do when you look up. If you had looked at the moon toward the east before the eclipse began and noted where a particular bright crater was located (like Tycho), and then looked again where the bright crater was located after the eclipse was over, you would realize the image of the moon that you now see has rotated somewhat. So an Alt-Az mount actually reproduces your point of view of the skies as you would see it looking up.