'Oumuamua observation times, modeled vector error, and solar flux (under construction)

 

Tumbling motion of 1I/'Oumuamua reveals body's violent past

Michal Drahus, Piotr Guzik, Waclaw Waniak, Barbara Handzlik, Sebastian Kurowski, Siyi Xu
https://arxiv.org/abs/1712.00437

Light curves were extracted from Drahus et al. 2017, and plotted onto GOES solar X-ray flux charts at coincident intervals, showing that the phases are roughly identical. Extra gravitational effects attributed to prior collision history frozen-in to the orbital motion of the error-prone observation period of 1I/ 'Oumuamua, which was in all periods directly coherent to the maximal CME front density for coupled slow and fast forward-reverse magnetic shock fronts, which produce refraction and dispersion errors, may in fact have generated artifacts that contributesld to the apparent luminosity, eccentricity of orbit, and morphology of the body itself, as a function of its rotation irregularities. 

This degeneracy is characteristic for uncorrected scalar orbit models, which are notorious for eccentricity estimation. As all three potential interstellar interlopers observed to date (August, 2026) were observed during maximal CME-induced foreground errors during peak flare/CME activity and/or interplanetary shock convergence at approximately the same annual intervals, diffractive/refractive observation error (emergent multivector gratings) and/or solar/IMF driving of motion must be considered. Interestingly, if so, evidence for any extrasolar origin of these bodies vanishes, and Kuiper-Oort models are valid. Error normalization values are in fact an eigenensemble that, when subtracted/deconvolved from motion/morphology/composition spectra/luminosity, show invariance. 

The Drahus et al. 2017 rotation phases are virtually identical to DCT Fourier power spectral components of their coincident solar flux indices:

Foreground and baseline error for terrestrial observations is locked with phase components of geostationary observation of X-ray flux, which occurs during maximal sun-Earth connectivity periods, and is a regime that is certain to accompany foreground dispersion artifacts and diffractive degeneracy between key orbital parameters for a diffuse/faint object without stable prior sky localization reference.