The South Equatorial Belt of Jupiter, I: Its Life Cycle
The South Equatorial Belt of Jupiter, I: Its Life Cycle
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木星南赤道带,I:它的生命周期
DOI:
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发表时间:
1996
期刊:
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通讯作者:
J. M. Gómez
中科院分区:
文献类型:
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作者:
A. Sánchez‐Lavega;J. M. Gómez
Abstract The South Equatorial Belt (SEB) of Jupiter, located between latitudes ∼10°S and ∼20°S, represents the archetype of a cyclically changing band between the belt and zone stages. A new analysis of the historical records has been performed, using various published observations and additional data in visual wavelengths, which permit characterization of cloud morphology patterns, the zonal and meridional motions, the zonal wind velocities, and the spatial and temporal scales of the variability of the SEB. For uniformity and clarity each phase of the cycle has been denoted with its proper nomenclature based on the traditional one. The following sequential stages can be distinguished: (i) Zone-like, global “fade” aspect (SEBF); (ii) Outbreak of activity with one or more independent sources in different longitudes but fixed latitudes (SEBD0), followed by the development and zonal expansion of a disturbance to planetary scale within the cyclonic band (SEBD); (iii) Propagation of the activity and formation of new disturbances in adjacent regions, tropical (20°S to 26°S, STrZD) and equatorial (5°S to 10°S, EZs activity). This phase, denoted globally as SEBD1 does not always develop after the SEBD; (iv) Normal belt-like stage (SEB), a period during which secondary outbursts simulating in some respects the SEBD can take place (also the STrZD and EZs disturbances can be present); (v) The cycle is completed with a rapid return to the SEBF phase. A new comprehensive list that includes quantitative data and detailed commentaries of all the documented events has been compiled. We propose and discuss possible dynamical scenarios involved in each one of these phases. In an accompanying paper (part II) the recent SEBD phase, whose onset occurred on April 6, 1993, is described in detail. The data presented in that paper describes the most thoroughly documented event to date and is based on our observations in the specral range from 400 to 890 nm, which will serve as a guide for comparisons with simultaneous observations by other teams performed at other wavelengths.