Venus Aeronomy:
For almost three decades since Mariner 2 flew by the planet in December 1962, Venus has been the subject of intense investigation by both the Soviet and American space programs. Since the intrinsic magnetic field of Venus is exceedingly weak, if it exists at all, we expect many phenomena of the uppe...
Gespeichert in:
| Weitere Verfasser: | |
|---|---|
| Format: | Elektronisch E-Book |
| Sprache: | English |
| Veröffentlicht: |
Dordrecht
Springer Netherlands
1991
|
| Schlagworte: | |
| Online-Zugang: | BTU01 Volltext |
| Zusammenfassung: | For almost three decades since Mariner 2 flew by the planet in December 1962, Venus has been the subject of intense investigation by both the Soviet and American space programs. Since the intrinsic magnetic field of Venus is exceedingly weak, if it exists at all, we expect many phenomena of the upper atmosphere and ionosphere of Venus to differ from their terrestrial counterparts. While flybys and landings of the many Venus missions provided useful data on these phenomena, orbital missions were needed for their detailed investigation. Such orbital missions were provided by the Soviet program with Veneras 9 and 10 in October 1975 and by the United States with the Pioneer Venus Orbiter in December 1978. Originally designed for a prime mission of only 243 days, the Pioneer Venus Orbiter is still functioning over a decade later, providing data nearly - hours a day through one of the most active solar cycles to date. We expect these transmis sions to continue until September 1992 when gravitation perturbations will lower the periapsis of the PVO orbit so that the spacecraft will be lost to the atmosphere. The Venera 9 and 10 and the Pioneer Venus observations have led to an explosion of knowledge about the upper atmosphere and ionosphere of Venus and their interaction with the solar wind. The availability of data over a full solar cycle has |
| Beschreibung: | 1 Online-Ressource (VIII, 489 p) |
| ISBN: | 9789401133005 |
| DOI: | 10.1007/978-94-011-3300-5 |
Internformat
MARC
| LEADER | 00000nmm a2200000zc 4500 | ||
|---|---|---|---|
| 001 | BV045177607 | ||
| 003 | DE-604 | ||
| 005 | 00000000000000.0 | ||
| 007 | cr|uuu---uuuuu | ||
| 008 | 180911s1991 |||| o||u| ||||||eng d | ||
| 020 | |a 9789401133005 |9 978-94-011-3300-5 | ||
| 024 | 7 | |a 10.1007/978-94-011-3300-5 |2 doi | |
| 035 | |a (ZDB-2-EES)978-94-011-3300-5 | ||
| 035 | |a (OCoLC)1053821629 | ||
| 035 | |a (DE-599)BVBBV045177607 | ||
| 040 | |a DE-604 |b ger |e aacr | ||
| 041 | 0 | |a eng | |
| 049 | |a DE-634 | ||
| 082 | 0 | |a 551.5 |2 23 | |
| 245 | 1 | 0 | |a Venus Aeronomy |c edited by C. T. Russell |
| 264 | 1 | |a Dordrecht |b Springer Netherlands |c 1991 | |
| 300 | |a 1 Online-Ressource (VIII, 489 p) | ||
| 336 | |b txt |2 rdacontent | ||
| 337 | |b c |2 rdamedia | ||
| 338 | |b cr |2 rdacarrier | ||
| 520 | |a For almost three decades since Mariner 2 flew by the planet in December 1962, Venus has been the subject of intense investigation by both the Soviet and American space programs. Since the intrinsic magnetic field of Venus is exceedingly weak, if it exists at all, we expect many phenomena of the upper atmosphere and ionosphere of Venus to differ from their terrestrial counterparts. While flybys and landings of the many Venus missions provided useful data on these phenomena, orbital missions were needed for their detailed investigation. Such orbital missions were provided by the Soviet program with Veneras 9 and 10 in October 1975 and by the United States with the Pioneer Venus Orbiter in December 1978. Originally designed for a prime mission of only 243 days, the Pioneer Venus Orbiter is still functioning over a decade later, providing data nearly - hours a day through one of the most active solar cycles to date. We expect these transmis sions to continue until September 1992 when gravitation perturbations will lower the periapsis of the PVO orbit so that the spacecraft will be lost to the atmosphere. The Venera 9 and 10 and the Pioneer Venus observations have led to an explosion of knowledge about the upper atmosphere and ionosphere of Venus and their interaction with the solar wind. The availability of data over a full solar cycle has | ||
| 650 | 4 | |a Earth Sciences | |
| 650 | 4 | |a Atmospheric Sciences | |
| 650 | 4 | |a Planetology | |
| 650 | 4 | |a Astrophysics and Astroparticles | |
| 650 | 4 | |a Earth sciences | |
| 650 | 4 | |a Planetology | |
| 650 | 4 | |a Atmospheric sciences | |
| 650 | 4 | |a Astrophysics | |
| 700 | 1 | |a Russell, C. T. |4 edt | |
| 776 | 0 | 8 | |i Erscheint auch als |n Druck-Ausgabe |z 9789401054577 |
| 856 | 4 | 0 | |u https://doi.org/10.1007/978-94-011-3300-5 |x Verlag |z URL des Erstveröffentlichers |3 Volltext |
| 912 | |a ZDB-2-EES | ||
| 940 | 1 | |q ZDB-2-EES_Archiv | |
| 999 | |a oai:aleph.bib-bvb.de:BVB01-030566837 | ||
| 966 | e | |u https://doi.org/10.1007/978-94-011-3300-5 |l BTU01 |p ZDB-2-EES |q ZDB-2-EES_Archiv |x Verlag |3 Volltext | |
Datensatz im Suchindex
| _version_ | 1804178866800951296 |
|---|---|
| any_adam_object | |
| author2 | Russell, C. T. |
| author2_role | edt |
| author2_variant | c t r ct ctr |
| author_facet | Russell, C. T. |
| building | Verbundindex |
| bvnumber | BV045177607 |
| collection | ZDB-2-EES |
| ctrlnum | (ZDB-2-EES)978-94-011-3300-5 (OCoLC)1053821629 (DE-599)BVBBV045177607 |
| dewey-full | 551.5 |
| dewey-hundreds | 500 - Natural sciences and mathematics |
| dewey-ones | 551 - Geology, hydrology, meteorology |
| dewey-raw | 551.5 |
| dewey-search | 551.5 |
| dewey-sort | 3551.5 |
| dewey-tens | 550 - Earth sciences |
| discipline | Geologie / Paläontologie |
| doi_str_mv | 10.1007/978-94-011-3300-5 |
| format | Electronic eBook |
| fullrecord | <?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>02820nmm a2200457zc 4500</leader><controlfield tag="001">BV045177607</controlfield><controlfield tag="003">DE-604</controlfield><controlfield tag="005">00000000000000.0</controlfield><controlfield tag="007">cr|uuu---uuuuu</controlfield><controlfield tag="008">180911s1991 |||| o||u| ||||||eng d</controlfield><datafield tag="020" ind1=" " ind2=" "><subfield code="a">9789401133005</subfield><subfield code="9">978-94-011-3300-5</subfield></datafield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1007/978-94-011-3300-5</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(ZDB-2-EES)978-94-011-3300-5</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(OCoLC)1053821629</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-599)BVBBV045177607</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-634</subfield></datafield><datafield tag="082" ind1="0" ind2=" "><subfield code="a">551.5</subfield><subfield code="2">23</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Venus Aeronomy</subfield><subfield code="c">edited by C. T. Russell</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="a">Dordrecht</subfield><subfield code="b">Springer Netherlands</subfield><subfield code="c">1991</subfield></datafield><datafield tag="300" ind1=" " ind2=" "><subfield code="a">1 Online-Ressource (VIII, 489 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="520" ind1=" " ind2=" "><subfield code="a">For almost three decades since Mariner 2 flew by the planet in December 1962, Venus has been the subject of intense investigation by both the Soviet and American space programs. Since the intrinsic magnetic field of Venus is exceedingly weak, if it exists at all, we expect many phenomena of the upper atmosphere and ionosphere of Venus to differ from their terrestrial counterparts. While flybys and landings of the many Venus missions provided useful data on these phenomena, orbital missions were needed for their detailed investigation. Such orbital missions were provided by the Soviet program with Veneras 9 and 10 in October 1975 and by the United States with the Pioneer Venus Orbiter in December 1978. Originally designed for a prime mission of only 243 days, the Pioneer Venus Orbiter is still functioning over a decade later, providing data nearly - hours a day through one of the most active solar cycles to date. We expect these transmis sions to continue until September 1992 when gravitation perturbations will lower the periapsis of the PVO orbit so that the spacecraft will be lost to the atmosphere. The Venera 9 and 10 and the Pioneer Venus observations have led to an explosion of knowledge about the upper atmosphere and ionosphere of Venus and their interaction with the solar wind. The availability of data over a full solar cycle has</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Earth Sciences</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Atmospheric Sciences</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Planetology</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Astrophysics and Astroparticles</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Earth sciences</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Planetology</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Atmospheric sciences</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Astrophysics</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Russell, C. T.</subfield><subfield code="4">edt</subfield></datafield><datafield tag="776" ind1="0" ind2="8"><subfield code="i">Erscheint auch als</subfield><subfield code="n">Druck-Ausgabe</subfield><subfield code="z">9789401054577</subfield></datafield><datafield tag="856" ind1="4" ind2="0"><subfield code="u">https://doi.org/10.1007/978-94-011-3300-5</subfield><subfield code="x">Verlag</subfield><subfield code="z">URL des Erstveröffentlichers</subfield><subfield code="3">Volltext</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">ZDB-2-EES</subfield></datafield><datafield tag="940" ind1="1" ind2=" "><subfield code="q">ZDB-2-EES_Archiv</subfield></datafield><datafield tag="999" ind1=" " ind2=" "><subfield code="a">oai:aleph.bib-bvb.de:BVB01-030566837</subfield></datafield><datafield tag="966" ind1="e" ind2=" "><subfield code="u">https://doi.org/10.1007/978-94-011-3300-5</subfield><subfield code="l">BTU01</subfield><subfield code="p">ZDB-2-EES</subfield><subfield code="q">ZDB-2-EES_Archiv</subfield><subfield code="x">Verlag</subfield><subfield code="3">Volltext</subfield></datafield></record></collection> |
| id | DE-604.BV045177607 |
| illustrated | Not Illustrated |
| indexdate | 2024-07-10T08:10:47Z |
| institution | BVB |
| isbn | 9789401133005 |
| language | English |
| oai_aleph_id | oai:aleph.bib-bvb.de:BVB01-030566837 |
| oclc_num | 1053821629 |
| open_access_boolean | |
| owner | DE-634 |
| owner_facet | DE-634 |
| physical | 1 Online-Ressource (VIII, 489 p) |
| psigel | ZDB-2-EES ZDB-2-EES_Archiv ZDB-2-EES ZDB-2-EES_Archiv |
| publishDate | 1991 |
| publishDateSearch | 1991 |
| publishDateSort | 1991 |
| publisher | Springer Netherlands |
| record_format | marc |
| spelling | Venus Aeronomy edited by C. T. Russell Dordrecht Springer Netherlands 1991 1 Online-Ressource (VIII, 489 p) txt rdacontent c rdamedia cr rdacarrier For almost three decades since Mariner 2 flew by the planet in December 1962, Venus has been the subject of intense investigation by both the Soviet and American space programs. Since the intrinsic magnetic field of Venus is exceedingly weak, if it exists at all, we expect many phenomena of the upper atmosphere and ionosphere of Venus to differ from their terrestrial counterparts. While flybys and landings of the many Venus missions provided useful data on these phenomena, orbital missions were needed for their detailed investigation. Such orbital missions were provided by the Soviet program with Veneras 9 and 10 in October 1975 and by the United States with the Pioneer Venus Orbiter in December 1978. Originally designed for a prime mission of only 243 days, the Pioneer Venus Orbiter is still functioning over a decade later, providing data nearly - hours a day through one of the most active solar cycles to date. We expect these transmis sions to continue until September 1992 when gravitation perturbations will lower the periapsis of the PVO orbit so that the spacecraft will be lost to the atmosphere. The Venera 9 and 10 and the Pioneer Venus observations have led to an explosion of knowledge about the upper atmosphere and ionosphere of Venus and their interaction with the solar wind. The availability of data over a full solar cycle has Earth Sciences Atmospheric Sciences Planetology Astrophysics and Astroparticles Earth sciences Atmospheric sciences Astrophysics Russell, C. T. edt Erscheint auch als Druck-Ausgabe 9789401054577 https://doi.org/10.1007/978-94-011-3300-5 Verlag URL des Erstveröffentlichers Volltext |
| spellingShingle | Venus Aeronomy Earth Sciences Atmospheric Sciences Planetology Astrophysics and Astroparticles Earth sciences Atmospheric sciences Astrophysics |
| title | Venus Aeronomy |
| title_auth | Venus Aeronomy |
| title_exact_search | Venus Aeronomy |
| title_full | Venus Aeronomy edited by C. T. Russell |
| title_fullStr | Venus Aeronomy edited by C. T. Russell |
| title_full_unstemmed | Venus Aeronomy edited by C. T. Russell |
| title_short | Venus Aeronomy |
| title_sort | venus aeronomy |
| topic | Earth Sciences Atmospheric Sciences Planetology Astrophysics and Astroparticles Earth sciences Atmospheric sciences Astrophysics |
| topic_facet | Earth Sciences Atmospheric Sciences Planetology Astrophysics and Astroparticles Earth sciences Atmospheric sciences Astrophysics |
| url | https://doi.org/10.1007/978-94-011-3300-5 |
| work_keys_str_mv | AT russellct venusaeronomy |