Diffraction-Limited Imaging with Very Large Telescopes:
Gespeichert in:
| 1. Verfasser: | |
|---|---|
| Format: | Elektronisch E-Book |
| Sprache: | English |
| Veröffentlicht: |
Dordrecht
Springer Netherlands
1989
|
| Schriftenreihe: | NATO ASI Series, Series C: Mathematical and Physical Sciences
274 |
| Schlagworte: | |
| Online-Zugang: | Volltext |
| Beschreibung: | A few years ago, a real break-through happened in observational astronomy: the un derstanding of the effect of atmospheric turbulence on the structure of stellar images, and of ways to overcome this dramatic degradation. This opened a route to diffraction-limited observations with large telescopes in the optical domain. Soon, the first applications of this new technique led to some outstanding astrophysical results, both at visible and infrared wavelengths. Yet, the potential of interferometric observations is not fully foreseeable as the first long-baseline arrays of large optical telescopes are being built or cOIIllnissioned right now. In this respect a comparison with the evolution of radio-astronomy is tempting. From a situation where, in spite of the construction of giant antennas, low angular resolution was prevailing, the introduction of long baseline and very long baseline interferometry and the rapid mastering of sophisticated image reconstruction techniques, have brought on a nearly routine basis high dynamic range images with milliarcseconds resolution. This, of course, has completely changed our views of the radio sky |
| Beschreibung: | 1 Online-Ressource (XVI, 433 p) |
| ISBN: | 9789400923409 9789401075534 |
| ISSN: | 1389-2185 |
| DOI: | 10.1007/978-94-009-2340-9 |
Internformat
MARC
| LEADER | 00000nmm a2200000zcb4500 | ||
|---|---|---|---|
| 001 | BV042415015 | ||
| 003 | DE-604 | ||
| 005 | 20170814 | ||
| 007 | cr|uuu---uuuuu | ||
| 008 | 150316s1989 |||| o||u| ||||||eng d | ||
| 020 | |a 9789400923409 |c Online |9 978-94-009-2340-9 | ||
| 020 | |a 9789401075534 |c Print |9 978-94-010-7553-4 | ||
| 024 | 7 | |a 10.1007/978-94-009-2340-9 |2 doi | |
| 035 | |a (OCoLC)863765382 | ||
| 035 | |a (DE-599)BVBBV042415015 | ||
| 040 | |a DE-604 |b ger |e aacr | ||
| 041 | 0 | |a eng | |
| 049 | |a DE-91 |a DE-83 | ||
| 082 | 0 | |a 520 |2 23 | |
| 084 | |a PHY 906f |2 stub | ||
| 084 | |a PHY 000 |2 stub | ||
| 100 | 1 | |a Alloin, D. M. |e Verfasser |4 aut | |
| 245 | 1 | 0 | |a Diffraction-Limited Imaging with Very Large Telescopes |c edited by D. M. Alloin, J.-M. Mariotti |
| 246 | 1 | 3 | |a Proceedings of the NATO Advanced Study Institute, Cargèse, Corsica, September 13-23, 1988 |
| 264 | 1 | |a Dordrecht |b Springer Netherlands |c 1989 | |
| 300 | |a 1 Online-Ressource (XVI, 433 p) | ||
| 336 | |b txt |2 rdacontent | ||
| 337 | |b c |2 rdamedia | ||
| 338 | |b cr |2 rdacarrier | ||
| 490 | 0 | |a NATO ASI Series, Series C: Mathematical and Physical Sciences |v 274 |x 1389-2185 | |
| 500 | |a A few years ago, a real break-through happened in observational astronomy: the un derstanding of the effect of atmospheric turbulence on the structure of stellar images, and of ways to overcome this dramatic degradation. This opened a route to diffraction-limited observations with large telescopes in the optical domain. Soon, the first applications of this new technique led to some outstanding astrophysical results, both at visible and infrared wavelengths. Yet, the potential of interferometric observations is not fully foreseeable as the first long-baseline arrays of large optical telescopes are being built or cOIIllnissioned right now. In this respect a comparison with the evolution of radio-astronomy is tempting. From a situation where, in spite of the construction of giant antennas, low angular resolution was prevailing, the introduction of long baseline and very long baseline interferometry and the rapid mastering of sophisticated image reconstruction techniques, have brought on a nearly routine basis high dynamic range images with milliarcseconds resolution. This, of course, has completely changed our views of the radio sky | ||
| 650 | 4 | |a Physics | |
| 650 | 4 | |a Astronomy, Observations and Techniques | |
| 650 | 4 | |a Statistics for Engineering, Physics, Computer Science, Chemistry and Earth Sciences | |
| 700 | 1 | |a Mariotti, J.-M. |e Sonstige |4 oth | |
| 856 | 4 | 0 | |u https://doi.org/10.1007/978-94-009-2340-9 |x Verlag |3 Volltext |
| 912 | |a ZDB-2-PHA |a ZDB-2-BAE | ||
| 940 | 1 | |q ZDB-2-PHA_Archive | |
| 999 | |a oai:aleph.bib-bvb.de:BVB01-027850508 | ||
Datensatz im Suchindex
| _version_ | 1804153081536970752 |
|---|---|
| any_adam_object | |
| author | Alloin, D. M. |
| author_facet | Alloin, D. M. |
| author_role | aut |
| author_sort | Alloin, D. M. |
| author_variant | d m a dm dma |
| building | Verbundindex |
| bvnumber | BV042415015 |
| classification_tum | PHY 906f PHY 000 |
| collection | ZDB-2-PHA ZDB-2-BAE |
| ctrlnum | (OCoLC)863765382 (DE-599)BVBBV042415015 |
| dewey-full | 520 |
| dewey-hundreds | 500 - Natural sciences and mathematics |
| dewey-ones | 520 - Astronomy and allied sciences |
| dewey-raw | 520 |
| dewey-search | 520 |
| dewey-sort | 3520 |
| dewey-tens | 520 - Astronomy and allied sciences |
| discipline | Physik |
| doi_str_mv | 10.1007/978-94-009-2340-9 |
| format | Electronic eBook |
| fullrecord | <?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>02721nmm a2200433zcb4500</leader><controlfield tag="001">BV042415015</controlfield><controlfield tag="003">DE-604</controlfield><controlfield tag="005">20170814 </controlfield><controlfield tag="007">cr|uuu---uuuuu</controlfield><controlfield tag="008">150316s1989 |||| o||u| ||||||eng d</controlfield><datafield tag="020" ind1=" " ind2=" "><subfield code="a">9789400923409</subfield><subfield code="c">Online</subfield><subfield code="9">978-94-009-2340-9</subfield></datafield><datafield tag="020" ind1=" " ind2=" "><subfield code="a">9789401075534</subfield><subfield code="c">Print</subfield><subfield code="9">978-94-010-7553-4</subfield></datafield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1007/978-94-009-2340-9</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(OCoLC)863765382</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-599)BVBBV042415015</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-604</subfield><subfield code="b">ger</subfield><subfield code="e">aacr</subfield></datafield><datafield tag="041" ind1="0" ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="049" ind1=" " ind2=" "><subfield code="a">DE-91</subfield><subfield code="a">DE-83</subfield></datafield><datafield tag="082" ind1="0" ind2=" "><subfield code="a">520</subfield><subfield code="2">23</subfield></datafield><datafield tag="084" ind1=" " ind2=" "><subfield code="a">PHY 906f</subfield><subfield code="2">stub</subfield></datafield><datafield tag="084" ind1=" " ind2=" "><subfield code="a">PHY 000</subfield><subfield code="2">stub</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Alloin, D. M.</subfield><subfield code="e">Verfasser</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Diffraction-Limited Imaging with Very Large Telescopes</subfield><subfield code="c">edited by D. M. Alloin, J.-M. Mariotti</subfield></datafield><datafield tag="246" ind1="1" ind2="3"><subfield code="a">Proceedings of the NATO Advanced Study Institute, Cargèse, Corsica, September 13-23, 1988</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="a">Dordrecht</subfield><subfield code="b">Springer Netherlands</subfield><subfield code="c">1989</subfield></datafield><datafield tag="300" ind1=" " ind2=" "><subfield code="a">1 Online-Ressource (XVI, 433 p)</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="b">c</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="b">cr</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="490" ind1="0" ind2=" "><subfield code="a">NATO ASI Series, Series C: Mathematical and Physical Sciences</subfield><subfield code="v">274</subfield><subfield code="x">1389-2185</subfield></datafield><datafield tag="500" ind1=" " ind2=" "><subfield code="a">A few years ago, a real break-through happened in observational astronomy: the un derstanding of the effect of atmospheric turbulence on the structure of stellar images, and of ways to overcome this dramatic degradation. This opened a route to diffraction-limited observations with large telescopes in the optical domain. Soon, the first applications of this new technique led to some outstanding astrophysical results, both at visible and infrared wavelengths. Yet, the potential of interferometric observations is not fully foreseeable as the first long-baseline arrays of large optical telescopes are being built or cOIIllnissioned right now. In this respect a comparison with the evolution of radio-astronomy is tempting. From a situation where, in spite of the construction of giant antennas, low angular resolution was prevailing, the introduction of long baseline and very long baseline interferometry and the rapid mastering of sophisticated image reconstruction techniques, have brought on a nearly routine basis high dynamic range images with milliarcseconds resolution. This, of course, has completely changed our views of the radio sky</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Physics</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Astronomy, Observations and Techniques</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Statistics for Engineering, Physics, Computer Science, Chemistry and Earth Sciences</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Mariotti, J.-M.</subfield><subfield code="e">Sonstige</subfield><subfield code="4">oth</subfield></datafield><datafield tag="856" ind1="4" ind2="0"><subfield code="u">https://doi.org/10.1007/978-94-009-2340-9</subfield><subfield code="x">Verlag</subfield><subfield code="3">Volltext</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">ZDB-2-PHA</subfield><subfield code="a">ZDB-2-BAE</subfield></datafield><datafield tag="940" ind1="1" ind2=" "><subfield code="q">ZDB-2-PHA_Archive</subfield></datafield><datafield tag="999" ind1=" " ind2=" "><subfield code="a">oai:aleph.bib-bvb.de:BVB01-027850508</subfield></datafield></record></collection> |
| id | DE-604.BV042415015 |
| illustrated | Not Illustrated |
| indexdate | 2024-07-10T01:20:56Z |
| institution | BVB |
| isbn | 9789400923409 9789401075534 |
| issn | 1389-2185 |
| language | English |
| oai_aleph_id | oai:aleph.bib-bvb.de:BVB01-027850508 |
| oclc_num | 863765382 |
| open_access_boolean | |
| owner | DE-91 DE-BY-TUM DE-83 |
| owner_facet | DE-91 DE-BY-TUM DE-83 |
| physical | 1 Online-Ressource (XVI, 433 p) |
| psigel | ZDB-2-PHA ZDB-2-BAE ZDB-2-PHA_Archive |
| publishDate | 1989 |
| publishDateSearch | 1989 |
| publishDateSort | 1989 |
| publisher | Springer Netherlands |
| record_format | marc |
| series2 | NATO ASI Series, Series C: Mathematical and Physical Sciences |
| spelling | Alloin, D. M. Verfasser aut Diffraction-Limited Imaging with Very Large Telescopes edited by D. M. Alloin, J.-M. Mariotti Proceedings of the NATO Advanced Study Institute, Cargèse, Corsica, September 13-23, 1988 Dordrecht Springer Netherlands 1989 1 Online-Ressource (XVI, 433 p) txt rdacontent c rdamedia cr rdacarrier NATO ASI Series, Series C: Mathematical and Physical Sciences 274 1389-2185 A few years ago, a real break-through happened in observational astronomy: the un derstanding of the effect of atmospheric turbulence on the structure of stellar images, and of ways to overcome this dramatic degradation. This opened a route to diffraction-limited observations with large telescopes in the optical domain. Soon, the first applications of this new technique led to some outstanding astrophysical results, both at visible and infrared wavelengths. Yet, the potential of interferometric observations is not fully foreseeable as the first long-baseline arrays of large optical telescopes are being built or cOIIllnissioned right now. In this respect a comparison with the evolution of radio-astronomy is tempting. From a situation where, in spite of the construction of giant antennas, low angular resolution was prevailing, the introduction of long baseline and very long baseline interferometry and the rapid mastering of sophisticated image reconstruction techniques, have brought on a nearly routine basis high dynamic range images with milliarcseconds resolution. This, of course, has completely changed our views of the radio sky Physics Astronomy, Observations and Techniques Statistics for Engineering, Physics, Computer Science, Chemistry and Earth Sciences Mariotti, J.-M. Sonstige oth https://doi.org/10.1007/978-94-009-2340-9 Verlag Volltext |
| spellingShingle | Alloin, D. M. Diffraction-Limited Imaging with Very Large Telescopes Physics Astronomy, Observations and Techniques Statistics for Engineering, Physics, Computer Science, Chemistry and Earth Sciences |
| title | Diffraction-Limited Imaging with Very Large Telescopes |
| title_alt | Proceedings of the NATO Advanced Study Institute, Cargèse, Corsica, September 13-23, 1988 |
| title_auth | Diffraction-Limited Imaging with Very Large Telescopes |
| title_exact_search | Diffraction-Limited Imaging with Very Large Telescopes |
| title_full | Diffraction-Limited Imaging with Very Large Telescopes edited by D. M. Alloin, J.-M. Mariotti |
| title_fullStr | Diffraction-Limited Imaging with Very Large Telescopes edited by D. M. Alloin, J.-M. Mariotti |
| title_full_unstemmed | Diffraction-Limited Imaging with Very Large Telescopes edited by D. M. Alloin, J.-M. Mariotti |
| title_short | Diffraction-Limited Imaging with Very Large Telescopes |
| title_sort | diffraction limited imaging with very large telescopes |
| topic | Physics Astronomy, Observations and Techniques Statistics for Engineering, Physics, Computer Science, Chemistry and Earth Sciences |
| topic_facet | Physics Astronomy, Observations and Techniques Statistics for Engineering, Physics, Computer Science, Chemistry and Earth Sciences |
| url | https://doi.org/10.1007/978-94-009-2340-9 |
| work_keys_str_mv | AT alloindm diffractionlimitedimagingwithverylargetelescopes AT mariottijm diffractionlimitedimagingwithverylargetelescopes AT alloindm proceedingsofthenatoadvancedstudyinstitutecargesecorsicaseptember13231988 AT mariottijm proceedingsofthenatoadvancedstudyinstitutecargesecorsicaseptember13231988 |