FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2954405531> ?p ?o ?g. }

• W2954405531 endingPage "849" @default.
• W2954405531 startingPage "831" @default.
• W2954405531 abstract "The far-infrared (FIR) is one of the few wavelength ranges where no astronomical data with sub-arcsec resolution exist yet. Neither of the medium-term satellite projects like SPICA, Millimetron or OST will resolve this malady. Information at high spatial and spectral resolution in the FIR, taken from atomic fine-structure lines, highly excited CO, and especially from water lines would, however, open the door for transformative science. This calls for interferometric concepts. We present first results of our feasibility study IRASSI (Infrared Astronomy Satellite Swarm Interferometry) for a FIR space interferometer. Extending on the principal concept of the ESPRIT study, it features heterodyne interferometry within a swarm of 5 satellite elements. The satellites can drift in and out within a range of several hundred meters, thereby achieving spatial resolutions of <0.1 over the whole wavelength range of 1-6 THz. Precise knowledge on the baselines will be ensured by metrology methods employing laser-based optical frequency combs, for which preliminary ground-based tests have been designed by us. We first show how the science requirements translate into operational and design parameters. We have put much emphasis on the navigational aspects of such a free-flying satellite swarm operating in relatively close vicinity. We hence present work on the formation geometry, the relative dynamics of the swarm, and aspects of our investigation towards attitude estimation. Furthermore, we discuss issues regarding the real-time capability of the autonomous relative positioning system, which is an important aspect for IRASSI where, due to the large raw data rates expected, the interferometric correlation has to be done onboard. We also address questions regarding the spacecraft architecture and how a thermomechanical model is used to study the effect of thermal perturbations on the spacecraft. (abridged)" @default.
• W2954405531 created "2019-07-12" @default.
• W2954405531 creator A5000327350 @default.
• W2954405531 creator A5000688029 @default.
• W2954405531 creator A5001673611 @default.
• W2954405531 creator A5001931712 @default.
• W2954405531 creator A5009888511 @default.
• W2954405531 creator A5019174548 @default.
• W2954405531 creator A5024430051 @default.
• W2954405531 creator A5030471986 @default.
• W2954405531 creator A5035452425 @default.
• W2954405531 creator A5047210815 @default.
• W2954405531 creator A5051039868 @default.
• W2954405531 creator A5055101741 @default.
• W2954405531 creator A5072904000 @default.
• W2954405531 creator A5084577830 @default.
• W2954405531 date "2020-01-01" @default.
• W2954405531 modified "2023-10-08" @default.
• W2954405531 title "InfraRed Astronomy Satellite Swarm Interferometry (IRASSI): Overview and study results" @default.
• W2954405531 cites W1267957734 @default.
• W2954405531 cites W1765032695 @default.
• W2954405531 cites W1825682289 @default.
• W2954405531 cites W1845448257 @default.
• W2954405531 cites W1968450423 @default.
• W2954405531 cites W1991108342 @default.
• W2954405531 cites W2002923246 @default.
• W2954405531 cites W2016600321 @default.
• W2954405531 cites W2022002212 @default.
• W2954405531 cites W2023058018 @default.
• W2954405531 cites W2034016787 @default.
• W2954405531 cites W2035538351 @default.
• W2954405531 cites W2063784852 @default.
• W2954405531 cites W2078700897 @default.
• W2954405531 cites W2079396829 @default.
• W2954405531 cites W2082108368 @default.
• W2954405531 cites W2108853098 @default.
• W2954405531 cites W2128308786 @default.
• W2954405531 cites W2131823000 @default.
• W2954405531 cites W2134541573 @default.
• W2954405531 cites W2143759881 @default.
• W2954405531 cites W2150754529 @default.
• W2954405531 cites W2173074330 @default.
• W2954405531 cites W2497285852 @default.
• W2954405531 cites W2520214598 @default.
• W2954405531 cites W2574356407 @default.
• W2954405531 cites W2768565736 @default.
• W2954405531 cites W2790594495 @default.
• W2954405531 cites W2801733100 @default.
• W2954405531 cites W2851542641 @default.
• W2954405531 cites W2963859707 @default.
• W2954405531 cites W3102132298 @default.
• W2954405531 cites W3102179097 @default.
• W2954405531 cites W3103332967 @default.
• W2954405531 cites W3104821242 @default.
• W2954405531 cites W3106080585 @default.
• W2954405531 cites W3130986434 @default.
• W2954405531 cites W3140276830 @default.
• W2954405531 cites W4293003757 @default.
• W2954405531 cites W952783030 @default.
• W2954405531 doi "https://doi.org/10.1016/j.asr.2019.06.022" @default.
• W2954405531 hasPublicationYear "2020" @default.
• W2954405531 type Work @default.
• W2954405531 sameAs 2954405531 @default.
• W2954405531 citedByCount "13" @default.
• W2954405531 countsByYear W29544055312019 @default.
• W2954405531 countsByYear W29544055312020 @default.
• W2954405531 countsByYear W29544055312021 @default.
• W2954405531 countsByYear W29544055312023 @default.
• W2954405531 crossrefType "journal-article" @default.
• W2954405531 hasAuthorship W2954405531A5000327350 @default.
• W2954405531 hasAuthorship W2954405531A5000688029 @default.
• W2954405531 hasAuthorship W2954405531A5001673611 @default.
• W2954405531 hasAuthorship W2954405531A5001931712 @default.
• W2954405531 hasAuthorship W2954405531A5009888511 @default.
• W2954405531 hasAuthorship W2954405531A5019174548 @default.
• W2954405531 hasAuthorship W2954405531A5024430051 @default.
• W2954405531 hasAuthorship W2954405531A5030471986 @default.
• W2954405531 hasAuthorship W2954405531A5035452425 @default.
• W2954405531 hasAuthorship W2954405531A5047210815 @default.
• W2954405531 hasAuthorship W2954405531A5051039868 @default.
• W2954405531 hasAuthorship W2954405531A5055101741 @default.
• W2954405531 hasAuthorship W2954405531A5072904000 @default.
• W2954405531 hasAuthorship W2954405531A5084577830 @default.
• W2954405531 hasBestOaLocation W29544055312 @default.
• W2954405531 hasConcept C120665830 @default.
• W2954405531 hasConcept C121332964 @default.
• W2954405531 hasConcept C127313418 @default.
• W2954405531 hasConcept C1276947 @default.
• W2954405531 hasConcept C154945302 @default.
• W2954405531 hasConcept C166689943 @default.
• W2954405531 hasConcept C181335050 @default.
• W2954405531 hasConcept C19269812 @default.
• W2954405531 hasConcept C2777460106 @default.
• W2954405531 hasConcept C41008148 @default.
• W2954405531 hasConcept C62649853 @default.
• W2954405531 hasConceptScore W2954405531C120665830 @default.
• W2954405531 hasConceptScore W2954405531C121332964 @default.
• W2954405531 hasConceptScore W2954405531C127313418 @default.

• next