Far-infrared observations of the galactic Cygnus region and Mars with a 60 cm diameter balloon-borne telescope
Abstract We have introduced secondary-mirror chopping in our balloon-borne far-infrared 60 cm Ø telescope equipped with He-cooled filters and a composite silicon bolometer with an NEP of 1.3 10−14 W/Hz1/2 for imaging, radiometry and spectroscopy of the Cygnus region at the wavelengths 80 μm, 130 μm...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
1991 |
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| Umfang: |
12 |
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| Reproduktion: |
Springer Online Journal Archives 1860-2002 |
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| Übergeordnetes Werk: |
in: International journal of infrared and millimeter waves - 1980, 12(1991) vom: Jan., Seite 33-44 |
| Übergeordnetes Werk: |
volume:12 ; year:1991 ; month:01 ; pages:33-44 ; extent:12 |
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NLEJ197363393 |
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| 245 | 1 | 0 | |a Far-infrared observations of the galactic Cygnus region and Mars with a 60 cm diameter balloon-borne telescope |
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| 520 | |a Abstract We have introduced secondary-mirror chopping in our balloon-borne far-infrared 60 cm Ø telescope equipped with He-cooled filters and a composite silicon bolometer with an NEP of 1.3 10−14 W/Hz1/2 for imaging, radiometry and spectroscopy of the Cygnus region at the wavelengths 80 μm, 130 μm and 310 μm. The modified system was flown on September 26/27, 1990 with a 380'000m3 hydrogen balloon at the CNES station at Aire/Adour, France. Observations were performed at a platform height of 39 km during 5 hrs. We made successful measurements on the complexes DR21 and S106 of the Cygnus region as well as on Mars at the wavelengths mentioned. | ||
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| 700 | 1 | |a Holenstein, A. |4 oth | |
| 700 | 1 | |a Schenker, G. |4 oth | |
| 700 | 1 | |a Kneubühl, F. K. |4 oth | |
| 700 | 1 | |a Huguenin, D. |4 oth | |
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(DE-627)NLEJ197363393 DE-627 ger DE-627 rakwb eng Far-infrared observations of the galactic Cygnus region and Mars with a 60 cm diameter balloon-borne telescope 1991 12 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Abstract We have introduced secondary-mirror chopping in our balloon-borne far-infrared 60 cm Ø telescope equipped with He-cooled filters and a composite silicon bolometer with an NEP of 1.3 10−14 W/Hz1/2 for imaging, radiometry and spectroscopy of the Cygnus region at the wavelengths 80 μm, 130 μm and 310 μm. The modified system was flown on September 26/27, 1990 with a 380'000m3 hydrogen balloon at the CNES station at Aire/Adour, France. Observations were performed at a platform height of 39 km during 5 hrs. We made successful measurements on the complexes DR21 and S106 of the Cygnus region as well as on Mars at the wavelengths mentioned. Springer Online Journal Archives 1860-2002 Holenstein, A. oth Schenker, G. oth Kneubühl, F. K. oth Huguenin, D. oth in International journal of infrared and millimeter waves 1980 12(1991) vom: Jan., Seite 33-44 (DE-627)NLEJ188988874 (DE-600)2016007-0 1572-9559 nnns volume:12 year:1991 month:01 pages:33-44 extent:12 http://dx.doi.org/10.1007/BF01041881 GBV_USEFLAG_U ZDB-1-SOJ GBV_NL_ARTICLE AR 12 1991 1 33-44 12 |
| spelling |
(DE-627)NLEJ197363393 DE-627 ger DE-627 rakwb eng Far-infrared observations of the galactic Cygnus region and Mars with a 60 cm diameter balloon-borne telescope 1991 12 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Abstract We have introduced secondary-mirror chopping in our balloon-borne far-infrared 60 cm Ø telescope equipped with He-cooled filters and a composite silicon bolometer with an NEP of 1.3 10−14 W/Hz1/2 for imaging, radiometry and spectroscopy of the Cygnus region at the wavelengths 80 μm, 130 μm and 310 μm. The modified system was flown on September 26/27, 1990 with a 380'000m3 hydrogen balloon at the CNES station at Aire/Adour, France. Observations were performed at a platform height of 39 km during 5 hrs. We made successful measurements on the complexes DR21 and S106 of the Cygnus region as well as on Mars at the wavelengths mentioned. Springer Online Journal Archives 1860-2002 Holenstein, A. oth Schenker, G. oth Kneubühl, F. K. oth Huguenin, D. oth in International journal of infrared and millimeter waves 1980 12(1991) vom: Jan., Seite 33-44 (DE-627)NLEJ188988874 (DE-600)2016007-0 1572-9559 nnns volume:12 year:1991 month:01 pages:33-44 extent:12 http://dx.doi.org/10.1007/BF01041881 GBV_USEFLAG_U ZDB-1-SOJ GBV_NL_ARTICLE AR 12 1991 1 33-44 12 |
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(DE-627)NLEJ197363393 DE-627 ger DE-627 rakwb eng Far-infrared observations of the galactic Cygnus region and Mars with a 60 cm diameter balloon-borne telescope 1991 12 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Abstract We have introduced secondary-mirror chopping in our balloon-borne far-infrared 60 cm Ø telescope equipped with He-cooled filters and a composite silicon bolometer with an NEP of 1.3 10−14 W/Hz1/2 for imaging, radiometry and spectroscopy of the Cygnus region at the wavelengths 80 μm, 130 μm and 310 μm. The modified system was flown on September 26/27, 1990 with a 380'000m3 hydrogen balloon at the CNES station at Aire/Adour, France. Observations were performed at a platform height of 39 km during 5 hrs. We made successful measurements on the complexes DR21 and S106 of the Cygnus region as well as on Mars at the wavelengths mentioned. Springer Online Journal Archives 1860-2002 Holenstein, A. oth Schenker, G. oth Kneubühl, F. K. oth Huguenin, D. oth in International journal of infrared and millimeter waves 1980 12(1991) vom: Jan., Seite 33-44 (DE-627)NLEJ188988874 (DE-600)2016007-0 1572-9559 nnns volume:12 year:1991 month:01 pages:33-44 extent:12 http://dx.doi.org/10.1007/BF01041881 GBV_USEFLAG_U ZDB-1-SOJ GBV_NL_ARTICLE AR 12 1991 1 33-44 12 |
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(DE-627)NLEJ197363393 DE-627 ger DE-627 rakwb eng Far-infrared observations of the galactic Cygnus region and Mars with a 60 cm diameter balloon-borne telescope 1991 12 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Abstract We have introduced secondary-mirror chopping in our balloon-borne far-infrared 60 cm Ø telescope equipped with He-cooled filters and a composite silicon bolometer with an NEP of 1.3 10−14 W/Hz1/2 for imaging, radiometry and spectroscopy of the Cygnus region at the wavelengths 80 μm, 130 μm and 310 μm. The modified system was flown on September 26/27, 1990 with a 380'000m3 hydrogen balloon at the CNES station at Aire/Adour, France. Observations were performed at a platform height of 39 km during 5 hrs. We made successful measurements on the complexes DR21 and S106 of the Cygnus region as well as on Mars at the wavelengths mentioned. Springer Online Journal Archives 1860-2002 Holenstein, A. oth Schenker, G. oth Kneubühl, F. K. oth Huguenin, D. oth in International journal of infrared and millimeter waves 1980 12(1991) vom: Jan., Seite 33-44 (DE-627)NLEJ188988874 (DE-600)2016007-0 1572-9559 nnns volume:12 year:1991 month:01 pages:33-44 extent:12 http://dx.doi.org/10.1007/BF01041881 GBV_USEFLAG_U ZDB-1-SOJ GBV_NL_ARTICLE AR 12 1991 1 33-44 12 |
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(DE-627)NLEJ197363393 DE-627 ger DE-627 rakwb eng Far-infrared observations of the galactic Cygnus region and Mars with a 60 cm diameter balloon-borne telescope 1991 12 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Abstract We have introduced secondary-mirror chopping in our balloon-borne far-infrared 60 cm Ø telescope equipped with He-cooled filters and a composite silicon bolometer with an NEP of 1.3 10−14 W/Hz1/2 for imaging, radiometry and spectroscopy of the Cygnus region at the wavelengths 80 μm, 130 μm and 310 μm. The modified system was flown on September 26/27, 1990 with a 380'000m3 hydrogen balloon at the CNES station at Aire/Adour, France. Observations were performed at a platform height of 39 km during 5 hrs. We made successful measurements on the complexes DR21 and S106 of the Cygnus region as well as on Mars at the wavelengths mentioned. Springer Online Journal Archives 1860-2002 Holenstein, A. oth Schenker, G. oth Kneubühl, F. K. oth Huguenin, D. oth in International journal of infrared and millimeter waves 1980 12(1991) vom: Jan., Seite 33-44 (DE-627)NLEJ188988874 (DE-600)2016007-0 1572-9559 nnns volume:12 year:1991 month:01 pages:33-44 extent:12 http://dx.doi.org/10.1007/BF01041881 GBV_USEFLAG_U ZDB-1-SOJ GBV_NL_ARTICLE AR 12 1991 1 33-44 12 |
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Far-infrared observations of the galactic Cygnus region and Mars with a 60 cm diameter balloon-borne telescope |
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Abstract We have introduced secondary-mirror chopping in our balloon-borne far-infrared 60 cm Ø telescope equipped with He-cooled filters and a composite silicon bolometer with an NEP of 1.3 10−14 W/Hz1/2 for imaging, radiometry and spectroscopy of the Cygnus region at the wavelengths 80 μm, 130 μm and 310 μm. The modified system was flown on September 26/27, 1990 with a 380'000m3 hydrogen balloon at the CNES station at Aire/Adour, France. Observations were performed at a platform height of 39 km during 5 hrs. We made successful measurements on the complexes DR21 and S106 of the Cygnus region as well as on Mars at the wavelengths mentioned. |
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Abstract We have introduced secondary-mirror chopping in our balloon-borne far-infrared 60 cm Ø telescope equipped with He-cooled filters and a composite silicon bolometer with an NEP of 1.3 10−14 W/Hz1/2 for imaging, radiometry and spectroscopy of the Cygnus region at the wavelengths 80 μm, 130 μm and 310 μm. The modified system was flown on September 26/27, 1990 with a 380'000m3 hydrogen balloon at the CNES station at Aire/Adour, France. Observations were performed at a platform height of 39 km during 5 hrs. We made successful measurements on the complexes DR21 and S106 of the Cygnus region as well as on Mars at the wavelengths mentioned. |
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Abstract We have introduced secondary-mirror chopping in our balloon-borne far-infrared 60 cm Ø telescope equipped with He-cooled filters and a composite silicon bolometer with an NEP of 1.3 10−14 W/Hz1/2 for imaging, radiometry and spectroscopy of the Cygnus region at the wavelengths 80 μm, 130 μm and 310 μm. The modified system was flown on September 26/27, 1990 with a 380'000m3 hydrogen balloon at the CNES station at Aire/Adour, France. Observations were performed at a platform height of 39 km during 5 hrs. We made successful measurements on the complexes DR21 and S106 of the Cygnus region as well as on Mars at the wavelengths mentioned. |
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