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Hi,
I think these are good questions. As you know, the greyline is enhanced propagation associated with paths along the dawn/dusk region. I’m not entirely sure how you would compare the propagation around the circular eclipse shadow with that greyline propagation along a long, linear path. Still, there may be some way to make useful comparisons and test some of our understanding of greyline. A useful and recent reference to start with when studying greyline is the Lo et al. (2022) study: https://doi.org/10.3390/atmos13081340
The equatorial ionospheric anomaly are enhanced regions of ionization just north and south of the geomagnetic equator due to something called the fountain effect. See https://doi.org/10.26464/epp2018025. While traversing North America, the eclipse will not be close to the EIA and will likely not be affected by it. However, towards the end of the eclipse the shadow will be over South America and will go in/near the EIA. Early model runs by Joe Huba suggest that the eclipse going through the EIA may produce ionospheric bubbles/irregularities that would not otherwise be there. But, more modeling and observational testing need to occur.
73 Nathaniel W2NAF
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Have a nice day!
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