Development of a strontium optical lattice clock for the SOC mission on the ISS

Publikation: Nicht-textuelle MedienAudiovisuelle VeröffentlichungForschungPeer-Review

Autoren

  • S. Origlia
  • S. Schiller
  • M. S. Pramod
  • L. Smith
  • Y. Singh
  • W. He
  • S. Viswam
  • D. Świerad
  • Thomas J.R. Hughes
  • K. Bongs
  • Uwe Sterr
  • Christian Lisdat
  • S. Vogt
  • S. Bize
  • J. Lodewyck
  • R. Le Targat
  • D. Holleville
  • B. Venon
  • Patrick Gill
  • G. Barwood
  • I. R. Hill
  • Y. Ovchinnikov
  • André Philipp Kulosa
  • Wolfgang Ertmer
  • Ernst Maria Rasel
  • J. Stuhler
  • W. Kaenders

Externe Organisationen

  • Universitätsklinikum Düsseldorf
  • University of Birmingham
  • University of Texas at Austin
  • Universität Hamburg
  • Physikalisch-Technische Bundesanstalt (PTB)
  • Observatoire de Paris (OBSPARIS)
  • National Physical Laboratory
  • Universität Konstanz
  • Universität Stuttgart
  • Toptica Photonics GmbH
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Details

OriginalspracheEnglisch
Herausgeber (Verlag)SPIE
PublikationsstatusVeröffentlicht - 29 Apr. 2016
VeranstaltungQuantum Optics - Brussels, Belgien
Dauer: 5 Apr. 20167 Apr. 2016

Abstract

The ESA mission "Space Optical Clock" project aims at operating an optical lattice clock on the ISS in approximately 2023. The scientific goals of the mission are to perform tests of fundamental physics, to enable space-assisted relativistic geodesy and to intercompare optical clocks on the ground using microwave and optical links. The performance goal of the space clock is less than 1 × 10 -17uncertainty and 1 × 10 -15τ -1/2 instability. Within an EU-FP7-funded project, a strontium optical lattice clock demonstrator has been developed. Goal performances are instability below 1 × 10 -15τ -1/2 and fractional inaccuracy 5 × 10 -17. For the design of the clock, techniques and approaches suitable for later space application are used, such as modular design, diode lasers, low power consumption subunits, and compact dimensions. The Sr clock apparatus is fully operational, and the clock transition in 88Sr was observed with linewidth as small as 9 Hz.

ASJC Scopus Sachgebiete

Zitieren

Development of a strontium optical lattice clock for the SOC mission on the ISS. Origlia, S. (Autor*in); Schiller, S. (Autor*in); Pramod, M. S. (Autor*in) et al.. 2016. SPIEVeranstaltung: null, Brussels, Belgien.

Publikation: Nicht-textuelle MedienAudiovisuelle VeröffentlichungForschungPeer-Review

Origlia, S, Schiller, S, Pramod, MS, Smith, L, Singh, Y, He, W, Viswam, S, Świerad, D, Hughes, TJR, Bongs, K, Sterr, U, Lisdat, C, Vogt, S, Bize, S, Lodewyck, J, Le Targat, R, Holleville, D, Venon, B, Gill, P, Barwood, G, Hill, IR, Ovchinnikov, Y, Kulosa, AP, Ertmer, W, Rasel, EM, Stuhler, J & Kaenders, W, Development of a strontium optical lattice clock for the SOC mission on the ISS, 2016, Audiovisuelle Veröffentlichung, SPIE. https://doi.org/10.1117/12.2229473
Origlia, S., Schiller, S., Pramod, M. S., Smith, L., Singh, Y., He, W., Viswam, S., Świerad, D., Hughes, T. J. R., Bongs, K., Sterr, U., Lisdat, C., Vogt, S., Bize, S., Lodewyck, J., Le Targat, R., Holleville, D., Venon, B., Gill, P., ... Kaenders, W. (2016). Development of a strontium optical lattice clock for the SOC mission on the ISS. Audiovisuelle Veröffentlichung, SPIE. https://doi.org/10.1117/12.2229473
Origlia S, Schiller S, Pramod MS, Smith L, Singh Y, He W et al.. Development of a strontium optical lattice clock for the SOC mission on the ISS SPIE. 2016. doi: 10.1117/12.2229473
Origlia, S. (Autor*in) ; Schiller, S. (Autor*in) ; Pramod, M. S. (Autor*in) et al.. / Development of a strontium optical lattice clock for the SOC mission on the ISS. [Audiovisuelle Veröffentlichung].
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abstract = "The ESA mission {"}Space Optical Clock{"} project aims at operating an optical lattice clock on the ISS in approximately 2023. The scientific goals of the mission are to perform tests of fundamental physics, to enable space-assisted relativistic geodesy and to intercompare optical clocks on the ground using microwave and optical links. The performance goal of the space clock is less than 1 × 10 -17uncertainty and 1 × 10 -15τ -1/2 instability. Within an EU-FP7-funded project, a strontium optical lattice clock demonstrator has been developed. Goal performances are instability below 1 × 10 -15τ -1/2 and fractional inaccuracy 5 × 10 -17. For the design of the clock, techniques and approaches suitable for later space application are used, such as modular design, diode lasers, low power consumption subunits, and compact dimensions. The Sr clock apparatus is fully operational, and the clock transition in 88Sr was observed with linewidth as small as 9 Hz. ",
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AU - Origlia, S.

AU - Schiller, S.

AU - Pramod, M. S.

AU - Smith, L.

AU - Singh, Y.

AU - He, W.

AU - Viswam, S.

AU - Świerad, D.

AU - Hughes, Thomas J.R.

AU - Bongs, K.

AU - Sterr, Uwe

AU - Lisdat, Christian

AU - Vogt, S.

AU - Bize, S.

AU - Lodewyck, J.

AU - Le Targat, R.

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AU - Venon, B.

AU - Gill, Patrick

AU - Barwood, G.

AU - Hill, I. R.

AU - Ovchinnikov, Y.

AU - Kulosa, André Philipp

AU - Ertmer, Wolfgang

AU - Rasel, Ernst Maria

AU - Stuhler, J.

AU - Kaenders, W.

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PY - 2016/4/29

Y1 - 2016/4/29

N2 - The ESA mission "Space Optical Clock" project aims at operating an optical lattice clock on the ISS in approximately 2023. The scientific goals of the mission are to perform tests of fundamental physics, to enable space-assisted relativistic geodesy and to intercompare optical clocks on the ground using microwave and optical links. The performance goal of the space clock is less than 1 × 10 -17uncertainty and 1 × 10 -15τ -1/2 instability. Within an EU-FP7-funded project, a strontium optical lattice clock demonstrator has been developed. Goal performances are instability below 1 × 10 -15τ -1/2 and fractional inaccuracy 5 × 10 -17. For the design of the clock, techniques and approaches suitable for later space application are used, such as modular design, diode lasers, low power consumption subunits, and compact dimensions. The Sr clock apparatus is fully operational, and the clock transition in 88Sr was observed with linewidth as small as 9 Hz.

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