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- W2772207962 abstract "We consider scattering of electromagnetic waves from a distant source by the gravitational field of the sun, taking the sun oblateness into account. It turns out that the sun oblateness is of a great importance in formation of the diffraction pattern in the infrared-visible and shorter wavelength range of the electromagnetic spectrum. Depending on the source orientation, spatial scales of the pattern increase by orders of magnitude and the maximal intensity magnification by solar gravitational lens decreases up to about two-three orders of magnitude in comparison with the spherically symmetric model. The sun gravitational lens produces an astroid caustic whose transversal size can reach several hundred meters, which is comparable with sizes of images of objects to be observed in prospective missions towards the focal line of the solar gravitational lens." @default.
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- W2772207962 date "2017-12-06" @default.
- W2772207962 modified "2023-09-27" @default.
- W2772207962 title "Diffraction Pattern of Solar Gravitational Lens" @default.
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