The rings of Uranus: Occultation profiles from three observatories
Elliot, J.L. ; Elias, J.H. ; French, R.G. ; Frogel, J.A. ; Liller, W. ; Matthews, K. ; Meech, K.J. ; Mink, D.J. ; Sicardy, B. ; Nicholson, P.D.
Amsterdam : Elsevier
Amsterdam : Elsevier
| ISSN: |
0019-1035
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|---|---|
| Source: |
Elsevier Journal Backfiles on ScienceDirect 1907 - 2002
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| Topics: |
Physics
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| Type of Medium: |
Electronic Resource
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| URL: |
| _version_ | 1798290857524199424 |
|---|---|
| autor | Elliot, J.L. Elias, J.H. French, R.G. Frogel, J.A. Liller, W. Matthews, K. Meech, K.J. Mink, D.J. Sicardy, B. Nicholson, P.D. |
| autorsonst | Elliot, J.L. Elias, J.H. French, R.G. Frogel, J.A. Liller, W. Matthews, K. Meech, K.J. Mink, D.J. Sicardy, B. Nicholson, P.D. |
| book_url | http://dx.doi.org/10.1016/0019-1035(83)90033-7 |
| datenlieferant | nat_lic_papers |
| fussnote | Occultation profiles for the nine confirmed Uranian rings obtained from Las Campanas, the European Southern Observatory, and Cerro Tololo on 15-16 August 1980 are compared. The α ring shows a ''double-dip'' structure; the η ring shows a broad and narrow component (similar to Saturn's F ring); and the ε ring shows six features that appear in the data from all three observatories. Diffraction fringes appear at the edges of several of the occultation profiles. |
| hauptsatz | hsatz_simple |
| identnr | NLZ180402358 |
| issn | 0019-1035 |
| journal_name | Icarus |
| materialart | 1 |
| package_name | Elsevier |
| publikationsort | Amsterdam |
| publisher | Elsevier |
| reference | 56 (1983), S. 202-208 |
| search_space | articles |
| shingle_author_1 | Elliot, J.L. Elias, J.H. French, R.G. Frogel, J.A. Liller, W. Matthews, K. Meech, K.J. Mink, D.J. Sicardy, B. Nicholson, P.D. |
| shingle_author_2 | Elliot, J.L. Elias, J.H. French, R.G. Frogel, J.A. Liller, W. Matthews, K. Meech, K.J. Mink, D.J. Sicardy, B. Nicholson, P.D. |
| shingle_author_3 | Elliot, J.L. Elias, J.H. French, R.G. Frogel, J.A. Liller, W. Matthews, K. Meech, K.J. Mink, D.J. Sicardy, B. Nicholson, P.D. |
| shingle_author_4 | Elliot, J.L. Elias, J.H. French, R.G. Frogel, J.A. Liller, W. Matthews, K. Meech, K.J. Mink, D.J. Sicardy, B. Nicholson, P.D. |
| shingle_catch_all_1 | Elliot, J.L. Elias, J.H. French, R.G. Frogel, J.A. Liller, W. Matthews, K. Meech, K.J. Mink, D.J. Sicardy, B. Nicholson, P.D. The rings of Uranus: Occultation profiles from three observatories 0019-1035 00191035 Elsevier |
| shingle_catch_all_2 | Elliot, J.L. Elias, J.H. French, R.G. Frogel, J.A. Liller, W. Matthews, K. Meech, K.J. Mink, D.J. Sicardy, B. Nicholson, P.D. The rings of Uranus: Occultation profiles from three observatories 0019-1035 00191035 Elsevier |
| shingle_catch_all_3 | Elliot, J.L. Elias, J.H. French, R.G. Frogel, J.A. Liller, W. Matthews, K. Meech, K.J. Mink, D.J. Sicardy, B. Nicholson, P.D. The rings of Uranus: Occultation profiles from three observatories 0019-1035 00191035 Elsevier |
| shingle_catch_all_4 | Elliot, J.L. Elias, J.H. French, R.G. Frogel, J.A. Liller, W. Matthews, K. Meech, K.J. Mink, D.J. Sicardy, B. Nicholson, P.D. The rings of Uranus: Occultation profiles from three observatories 0019-1035 00191035 Elsevier |
| shingle_title_1 | The rings of Uranus: Occultation profiles from three observatories |
| shingle_title_2 | The rings of Uranus: Occultation profiles from three observatories |
| shingle_title_3 | The rings of Uranus: Occultation profiles from three observatories |
| shingle_title_4 | The rings of Uranus: Occultation profiles from three observatories |
| sigel_instance_filter | dkfz geomar wilbert ipn albert fhp |
| source_archive | Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 |
| timestamp | 2024-05-06T08:23:23.940Z |
| titel | The rings of Uranus: Occultation profiles from three observatories |
| titel_suche | The rings of Uranus: Occultation profiles from three observatories Occultation profiles for the nine confirmed Uranian rings obtained from Las Campanas, the European Southern Observatory, and Cerro Tololo on 15-16 August 1980 are compared. The α ring shows a ''double-dip'' structure; the η ring shows a broad and narrow component (similar to Saturn's F ring); and the ε ring shows six features that appear in the data from all three observatories. Diffraction fringes appear at the edges of several of the occultation profiles. |
| topic | U |
| uid | nat_lic_papers_NLZ180402358 |