Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/32573
DC Field | Value | Language |
---|---|---|
dc.contributor.author | HOPE, Douglas | en_US |
dc.contributor.author | JEFFERIES, Stuart | en_US |
dc.contributor.author | LI CAUSI, Gianluca | en_US |
dc.contributor.author | STANGALINI, MARCO | en_US |
dc.contributor.author | PEDICHINI, Fernando | en_US |
dc.contributor.author | MATTIOLI, Massimiliano | en_US |
dc.contributor.author | ANTONIUCCI, Simone | en_US |
dc.contributor.author | TESTA, Vincenzo | en_US |
dc.contributor.author | PIAZZESI, ROBERTO | en_US |
dc.date.accessioned | 2022-09-15T09:30:24Z | - |
dc.date.available | 2022-09-15T09:30:24Z | - |
dc.date.issued | 2019 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/32573 | - |
dc.description.abstract | The monitoring and protection of satellites is a crucial component of national security and space traffic management. Characterizing the local space environment around important satellites, such as persistence surveillance platforms and communication satellites, requires an ability to robustly detect, identify and classify any objects or debris in proximity to the satellite that may pose a threat. Accomplishing this task requires using large aperture (>3m) ground-based telescopes. However, image blur caused by the finite aperture size of the telescope and dynamic atmospheric blur will cause the observed reflected solar illumination of the satellite to be smeared out across the image, effectively obscuring the presence of any faint object in proximity to the spacecraft. <P />Overcoming this problem of detecting a faint source embedded in the noise of another source, commonly referred to as the problem of identifying closely spaced objects (CSOs), requires both high-resolution and high-contrast imaging. The significant technical barrier that must be overcome is the building of a high-fidelity model of the turbulence in the atmosphere. One step in overcoming this barrier is the use of a large aperture telescope equipped with an adaptive optics (AO) system with a temporal response matched to the Greenwood frequency of the site. However, even with such a system, the limited spatial sampling of the wave front by the wave-front-sensor limits the measurement of the high frequencies in the wave front, thus limiting the effectiveness of the AO correction and thus yielding an image with a resolution lower than that of the diffraction limit of the telescope. This residual blur represents an accumulation of uncorrected faint speckle structure in the PSF which can obscure the presence of any objects or debris near the primary satellite. <P />Removing this residual blur in the AO-restored imagery requires the use of advanced multi-frame blind deconvolution (MFBD) algorithms. The basis of MFBD is to solve for a single static object scene and a set of PSFs that change in a temporal fashion that is consistent with turbulence induced errors in the wave front. Typically, the number of PSFs that must be estimated for MFBD is on the order of several hundred (1-2 seconds of image data) as a low-earth orbiting (LEO) object changes pose significantly enough on longer time scales that the assumption of a static object scene is violated, thus causing MFBD to produce erroneous non-physical results. For the CSO problem at a geostationary orbit the object will remain static on much longer time scales, and this will allow MFBD to use a much larger volume of data (5-10 minutes), and thus obtain a higher resolution image of the primary satellite over the AO compensated image. Further, we will demonstrate the effects of how a high fidelity PSF model can dramatically improve the background in the image via the proper modeling of the uncorrected speckle structure in the PSF. This will lead to an ability to perform high contrast imaging, which allows the use of MFBD restoration on data where brightness between the satellite and companion will cover a dynamic range on the order of 104. <P />Scaling the MFBD problem with data volume (from several thousand to several million variables) represents a formidable computational and minimization challenge, that we study using a sequence of high frame rate (1 kHz) images acquired with the SHARK-VIS forerunner at the Large Binocular Telescope (8.4m aperture). We demonstrate the importance of leveraging temporal correlations in the turbulence, that is encoded into Fourier spectra of the imagery by the optical system, to obtain high quality starting guesses for the wave fronts used in the large scale MFBD. We then demonstrate how an improvement in the fidelity of a PSF model from MFBD can improve the use of Recurrence Quantification Analysis (RQA) to statistically discriminate between the signal of the faint satellite companion and the speckle noise in the imagery. | en_US |
dc.language.iso | eng | en_US |
dc.title | High-Resolution Imaging of Closely Space Objects with High Contrast Ratios | en_US |
dc.type | Conference paper | - |
dc.identifier.url | https://amostech.com/ | en_US |
dc.identifier.url | https://amostech.com/proceedings/ | en_US |
dc.relation.medium | ELETTRONICO | en_US |
dc.relation.firstpage | 3 | en_US |
dc.type.referee | REF_0 | en_US |
dc.description.numberofauthors | 9 | en_US |
dc.description.international | sì | en_US |
dc.contributor.country | ITA | en_US |
dc.contributor.country | USA | en_US |
dc.relation.ispartofbook | AMOS Advanced Maui Optical and Space Surveillance Technologies Conference 2019 Conference Proceedings | en_US |
dc.relation.conferencename | Advanced Maui Optical and Space Surveillance Technologies Conference | en_US |
dc.relation.conferenceplace | Wailea, Maui, Hawaii | en_US |
dc.relation.conferencedate | September 17-20, 2019 | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.type.miur | 273 Contributo in Atti di convegno | - |
dc.identifier.adsbibcode | 2019amos.confE...3H | en_US |
dc.relation.ercsector | ERC sectors::Physical Sciences and Engineering::PE6 Computer Science and Informatics: Informatics and information systems, computer science, scientific computing, intelligent systems::PE6_12 Scientific computing, simulation and modelling tools | en_US |
dc.description.apc | no | en_US |
dc.description.oa | 1 – prodotto con file in versione Open Access (allegare il file al passo 5-Carica) | en_US |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.fulltext | With Fulltext | - |
item.grantfulltext | reserved | - |
item.languageiso639-1 | en | - |
item.openairetype | Conference paper | - |
item.cerifentitytype | Publications | - |
crisitem.author.dept | O.A. Roma | - |
crisitem.author.dept | O.A. Roma | - |
crisitem.author.dept | O.A. Roma | - |
crisitem.author.dept | O.A. Roma | - |
crisitem.author.dept | O.A. Roma | - |
crisitem.author.dept | O.A. Roma | - |
crisitem.author.orcid | 0000-0001-9539-2112 | - |
crisitem.author.orcid | 0000-0002-5365-7546 | - |
crisitem.author.orcid | 0000-0002-0983-8040 | - |
crisitem.author.orcid | 0000-0002-5790-3994 | - |
crisitem.author.orcid | 0000-0002-0666-3847 | - |
crisitem.author.orcid | 0000-0003-1033-1340 | - |
crisitem.author.orcid | 0000-0002-2264-8698 | - |
Appears in Collections: | 3.01 Contributi in Atti di convegno |
Files in This Item:
File | Description | Size | Format | Existing users please |
---|---|---|---|---|
Hope.pdf | [Administrators only] | 6.97 MB | Adobe PDF |
Page view(s)
73
checked on Sep 11, 2024
Download(s)
6
checked on Sep 11, 2024
Google ScholarTM
Check
Items in DSpace are published in Open Access, unless otherwise indicated.