Radio observations of the planet Jupiter:
Gespeichert in:
| Beteiligte Personen: | , |
|---|---|
| Format: | Buch |
| Sprache: | Englisch |
| Veröffentlicht: |
[Baltimore]
1958
|
| Beschreibung: | Radio observations of Jupiter made in June 1954 and November 1, 1955, to March 13, 1956, are reported. Three aspects of the program are discussed: (1) Correlation of observation with the rotation of Jupiter; (2) Polarization of the radiation; (3) Frequency characteristics. During the period of observation, there were at least three centers of activity on the planet, rotating approximately with the non equatorial regions. No definite correlation of radio noise with visible features was noted. The white spot DE, noted as a possible correlation in 1951 data, was definitely not well correlated with radio noise occurrences in 1955–56. The most active radio region exhibited a rotational period of 9h55m33s, a value consistent with other determinations and also consistent with the suggested long term rotational period, system III. Most of the radio noise bursts were strongly circularly polarized. For the most active region, only bursts of right circular polarization were observed. The radio noise spectrum does not appear to be continuous over the observed set of frequencies. The hypothesis that the narrow angle of visibility is evidence for critical reflection by the ionosphere of Jupiter is not supported by the combined Carnegie and Australian observations |
| Umfang: | Seiten 807 - 824 Illustrationen und graphische Darstellungen |
Internformat
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| 100 | 1 | |a Franklin, Kenneth L. |d 1923-2007 |0 (DE-588)1047455080 |4 aut | |
| 245 | 1 | 0 | |a Radio observations of the planet Jupiter |
| 264 | 1 | |a [Baltimore] |c 1958 | |
| 264 | 3 | |b [Byrd] | |
| 300 | |a Seiten 807 - 824 |b Illustrationen und graphische Darstellungen | ||
| 336 | |b txt |2 rdacontent | ||
| 337 | |b n |2 rdamedia | ||
| 338 | |b nc |2 rdacarrier | ||
| 500 | |a Radio observations of Jupiter made in June 1954 and November 1, 1955, to March 13, 1956, are reported. Three aspects of the program are discussed: (1) Correlation of observation with the rotation of Jupiter; (2) Polarization of the radiation; (3) Frequency characteristics. During the period of observation, there were at least three centers of activity on the planet, rotating approximately with the non equatorial regions. No definite correlation of radio noise with visible features was noted. The white spot DE, noted as a possible correlation in 1951 data, was definitely not well correlated with radio noise occurrences in 1955–56. The most active radio region exhibited a rotational period of 9h55m33s, a value consistent with other determinations and also consistent with the suggested long term rotational period, system III. Most of the radio noise bursts were strongly circularly polarized. For the most active region, only bursts of right circular polarization were observed. The radio noise spectrum does not appear to be continuous over the observed set of frequencies. The hypothesis that the narrow angle of visibility is evidence for critical reflection by the ionosphere of Jupiter is not supported by the combined Carnegie and Australian observations | ||
| 505 | 0 | |a [Baltimore] 1958: [Byrd]. S. 807-824 m. Abb. u. Taf. [Kopft.]<br>S.- Abdr. aus: Journal of geophysical research. 63, 4. | |
| 700 | 1 | |a Burke, Bernard F. |d 1928-2018 |0 (DE-588)112809707 |4 aut | |
| 787 | 0 | 8 | |i Sonderdruck aus |t Journal of geophysical research |c 63,4, S. 807-824 |
| 943 | 1 | |a oai:aleph.bib-bvb.de:BVB01-011551401 | |
| 980 | 4 | |a (DE-12)AK7260164 | |
| 980 | 4 | |a (DE-12)AK03490729 | |
Datensatz im Suchindex
| _version_ | 1818959187284066304 |
|---|---|
| any_adam_object | |
| author | Franklin, Kenneth L. 1923-2007 Burke, Bernard F. 1928-2018 |
| author_GND | (DE-588)1047455080 (DE-588)112809707 |
| author_facet | Franklin, Kenneth L. 1923-2007 Burke, Bernard F. 1928-2018 |
| author_role | aut aut |
| author_sort | Franklin, Kenneth L. 1923-2007 |
| author_variant | k l f kl klf b f b bf bfb |
| building | Verbundindex |
| bvnumber | BV018780666 |
| contents | [Baltimore] 1958: [Byrd]. S. 807-824 m. Abb. u. Taf. [Kopft.]<br>S.- Abdr. aus: Journal of geophysical research. 63, 4. |
| ctrlnum | (OCoLC)641876920 (DE-599)BVBBV018780666 |
| format | Book |
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| id | DE-604.BV018780666 |
| illustrated | Illustrated |
| indexdate | 2024-12-20T11:37:39Z |
| institution | BVB |
| language | English |
| oai_aleph_id | oai:aleph.bib-bvb.de:BVB01-011551401 |
| oclc_num | 641876920 |
| open_access_boolean | |
| owner | DE-12 |
| owner_facet | DE-12 |
| physical | Seiten 807 - 824 Illustrationen und graphische Darstellungen |
| publishDate | 1958 |
| publishDateSearch | 1958 |
| publishDateSort | 1958 |
| record_format | marc |
| spelling | Franklin, Kenneth L. 1923-2007 (DE-588)1047455080 aut Radio observations of the planet Jupiter [Baltimore] 1958 [Byrd] Seiten 807 - 824 Illustrationen und graphische Darstellungen txt rdacontent n rdamedia nc rdacarrier Radio observations of Jupiter made in June 1954 and November 1, 1955, to March 13, 1956, are reported. Three aspects of the program are discussed: (1) Correlation of observation with the rotation of Jupiter; (2) Polarization of the radiation; (3) Frequency characteristics. During the period of observation, there were at least three centers of activity on the planet, rotating approximately with the non equatorial regions. No definite correlation of radio noise with visible features was noted. The white spot DE, noted as a possible correlation in 1951 data, was definitely not well correlated with radio noise occurrences in 1955–56. The most active radio region exhibited a rotational period of 9h55m33s, a value consistent with other determinations and also consistent with the suggested long term rotational period, system III. Most of the radio noise bursts were strongly circularly polarized. For the most active region, only bursts of right circular polarization were observed. The radio noise spectrum does not appear to be continuous over the observed set of frequencies. The hypothesis that the narrow angle of visibility is evidence for critical reflection by the ionosphere of Jupiter is not supported by the combined Carnegie and Australian observations [Baltimore] 1958: [Byrd]. S. 807-824 m. Abb. u. Taf. [Kopft.]<br>S.- Abdr. aus: Journal of geophysical research. 63, 4. Burke, Bernard F. 1928-2018 (DE-588)112809707 aut Sonderdruck aus Journal of geophysical research 63,4, S. 807-824 |
| spellingShingle | Franklin, Kenneth L. 1923-2007 Burke, Bernard F. 1928-2018 Radio observations of the planet Jupiter [Baltimore] 1958: [Byrd]. S. 807-824 m. Abb. u. Taf. [Kopft.]<br>S.- Abdr. aus: Journal of geophysical research. 63, 4. |
| title | Radio observations of the planet Jupiter |
| title_auth | Radio observations of the planet Jupiter |
| title_exact_search | Radio observations of the planet Jupiter |
| title_full | Radio observations of the planet Jupiter |
| title_fullStr | Radio observations of the planet Jupiter |
| title_full_unstemmed | Radio observations of the planet Jupiter |
| title_short | Radio observations of the planet Jupiter |
| title_sort | radio observations of the planet jupiter |
| work_keys_str_mv | AT franklinkennethl radioobservationsoftheplanetjupiter AT burkebernardf radioobservationsoftheplanetjupiter |