It's just ... well ... a lot darker.
Shooting long-exposure slide film is a good way to confirm this (no colour adjustment possible).
Moonlight is has a slightly lower (that is, optically "warmer") colour temperature -- 4100K rather than 5000K.
Contrast with "daylight" vs. "tungsten" film colour balance: 5500K vs. 3200K.
https://physics.stackexchange.com/questions/244922/why-does-...
http://www.apogeephoto.com/white-balance-and-color-temperatu...
Or shooting long exposure with a digital camera that does not automatically adjust the color balance. E.g. take the raw data from the sensor, instead of a camera-generated JPEG.
(Much of my experimental night photography was conducted ... some time ago.)
Working with film was, um, exciting? Not sure if that's the right word. Anyway, mistakes were final. I remember deliberating on the settings for a really long time before pushing the button.
Thanks for sharing though! I wasn't able to experience the full eclipse so I love seeing others experience it.
To my eyes, close to totality (on either side) the light was a bit redshifted. Not much, but a little. The change seemed symmetrical before and after.
I've imaged the whole event. Looking at the disk of the Sun, the color is not the same everywhere. The edge definitely loses energy in the blue end of the spectrum - I believe for the same reason why blue light is dispersed more, compared to red, in Earth's atmosphere. So near totality, when you receive light only from the edge of the photosphere, it's normal that the spectral composition looks different.
And yes, there's a huge difference between any perceivable percentage away from totality, and totality itself. We're talking fractions of a second making a difference between direct viewing vs rapidly going blind.