The Current Stage of Development of the Receiving Complex of the Millimetron Space Observatory
Artikel i vetenskaplig tidskrift, 2012

We present an overview of the state of the onboard receiving complex of the Millimetron space observatory in the development phase of its preliminary design. The basic parameters of the onboard equipment planned to create and required for astrophysical observations are considered. A review of coherent and incoherent detectors, which are central to each receiver of the observatory, is given. Their characteristics and limiting parameters feasible at the present level of technology are reported.

telescope

noise

electrothermal feedback

mixer

wavelengths

circuits

detector

cold-electron bolometer

Författare

A. V. Smirnov

Pn Lebedev Physics Institute, Russian Academy of Sciences

Lomonosov Moscow State University

A. M. Baryshev

SRON Netherlands Institute for Space Research

P. de Bernardis

Universita degli Studi di Roma La Sapienza

V. F. Vdovin

Pn Lebedev Physics Institute, Russian Academy of Sciences

Lobachevsky State University of Nizhni Novgorod

Institute of Applied Physics, Russian Academy of Sciences

G. N. Gol'tsman

Pn Lebedev Physics Institute, Russian Academy of Sciences

Lomonosov Moscow State University

N. S. Kardashev

Pn Lebedev Physics Institute, Russian Academy of Sciences

Leonid Kuzmin

Chalmers, Mikroteknologi och nanovetenskap (MC2), Kvantkomponentfysik

V. P. Koshelets

V. A. kotel'Nikov Institute for Radioengineering and Electronics

A. N. Vystavkin

V. A. kotel'Nikov Institute for Radioengineering and Electronics

Y. V. Lobanov

Lomonosov Moscow State University

S. A. Ryabchun

Lomonosov Moscow State University

M. I. Finkel

Lomonosov Moscow State University

Pn Lebedev Physics Institute, Russian Academy of Sciences

D. R. Khokhlov

Lomonosov Moscow State University

Radiophysics and Quantum Electronics (English Translation of Izvestiya Vysshikh Uchebnykh Zavedenii, Radiofizika)

0033-8443 (ISSN) 1573-9120 (eISSN)

Vol. 54 8-9 557-568

Ämneskategorier (SSIF 2011)

Fysik

DOI

10.1007/s11141-012-9314-z

Mer information

Skapat

2017-10-06