Zobrazeno 1 - 4
of 4
pro vyhledávání: '"T deGraauw"'
Publikováno v:
International Journal of Infrared and Millimeter Waves, 17(1), 91-104
We describe heterodyne mixing experiments with NbCN/Nb quasi-particle tunnel junctions at submillimeter wavelengths. In this wavelength range junctions with niobium nitride as superconducting material are promising because of the high gap voltage, ab
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c79898417acf44b3f31ba9573cfce6ea
https://doi.org/10.1007/bf02088185
https://doi.org/10.1007/bf02088185
Autor:
Rs Booth, T Degraauw
Publikováno v:
Iau symposia, 415-420
ISSUE=148;STARTPAGE=415;ENDPAGE=420;ISSN=0074-1809;TITLE=Iau symposia
ISSUE=148;STARTPAGE=415;ENDPAGE=420;ISSN=0074-1809;TITLE=Iau symposia
In this short review we describe recent new observations of millimetre transitions of molecules in selected regions of the Magellanic Clouds. The observations were made using the Swedish-ESO Submillimetre Telescope, SEST, (Booth et al. 1989), the rel
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a8903afc6f40e465ac378bb151efb1f8
https://doi.org/10.1017/s0074180900201046
https://doi.org/10.1017/s0074180900201046
Publikováno v:
Superconductor Science and Technology. 4:683-685
An array of four Nb-Al-Al2O3-Nb SIS junctions in series is used as the mixing element in a waveguide mixer at 345 GHz. The area of one junction is 4 mu m2 and its normal state resistance is about 12 Omega , yielding at 345 GHz, omega RC approximately
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::dfa238ad69d5e3ee341d5ad4de305209
https://doi.org/10.1088/0953-2048/4/11/036
https://doi.org/10.1088/0953-2048/4/11/036
Autor:
[No Value] Pottasch, Fred Lahuis, Boxhoorn, T deGraauw, Patrick W. Morris, Helmut Feuchtgruber, D. A. Beintema, L. B. F. M. Waters, Pam vanHoof
Publikováno v:
Planetary Nebulae ISBN: 9780792348931
Infrared spectra of NGC 7027 and NGC 6543 ranging from 2.4 μm to 45 μm were obtained with the Short Wavelength Spectrometer on board the Infrared Space Observatory. A first analysis of these spectra, with the aid of photo-ionization models, is pres
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::27ae6581c2b86f5985829b054afcc7ba
https://doi.org/10.1007/978-94-011-5244-0_52
https://doi.org/10.1007/978-94-011-5244-0_52
