dc.rights.license | CC-BY-NC-ND | |
dc.contributor.advisor | Vasconselos, Ivan | |
dc.contributor.author | Savenije, V. | |
dc.date.accessioned | 2018-08-27T17:01:00Z | |
dc.date.available | 2018-08-27T17:01:00Z | |
dc.date.issued | 2018 | |
dc.identifier.uri | https://studenttheses.uu.nl/handle/20.500.12932/30607 | |
dc.description.abstract | The structure of asteroids remains ill-unknown due to few effective methods
to accurately image their interior. In this paper, using a synthetic model of
an asteroid, radar imaging by migration of slant stacked data is studied. The
basis for this method relies on beamforming in the electric wave?eld due to the
interference of pointsource responses. This method, here referred to as waveform
Synthetic Aperture Radar (SAR) imaging, is evaluated for migration at both
the source- and receiver-side, but results are very comparable. Waveform SAR
is compared to imaging with zero-offset data as well as multi-offset data, the
latter only acquirable by using more than one satellite in practice. Waveform
SAR shows better image quality than zero-offset data migration when the target
is coarsely spatially sampled by data points. This is because the image using
waveform SAR is more accurate per shot, due to ampli?cation of signal near
the true location of scatterers. | |
dc.description.sponsorship | Utrecht University | |
dc.format.extent | 2037065 | |
dc.format.mimetype | application/pdf | |
dc.language.iso | en | |
dc.title | The effect radar imaging of astroids by migration
of slant stacked data | |
dc.type.content | Master Thesis | |
dc.rights.accessrights | Open Access | |
dc.subject.keywords | seismic, imaging, SAR, asteroids, slant stacking | |
dc.subject.courseuu | Earth Structure and Dynamics | |