The evolution of spokes in Saturn's B ring |
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| Authors: | Eberhard Grün Gregor E Morfill Richard J Terrile Torrence V Johnson Gerhard Schwehm |
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| Institution: | 1. Lunar and Planetary Institute, Houston, Texas 77058, USA;2. Max-Planck-Institut für Extraterrestrische Physik, 8046 Garching, Federal Republic of Germany;3. Jet Propulsion Laboratory, Pasadena, California 91109, USA;4. Ruhr Universität, Bereich Extraterrestrische Physik, Bochum, Federal Republic of Germany |
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| Abstract: | The optical appearance of spokes was studied in high resolution (?200 km/lp) images obtained by Voyager 2. Spokes are classified into three categories. (1) Extended spokes are seen in the distance interval of 100,000 to 112,000 km from Saturn's center. They have diffuse edges and are slightly wedge shaped. Their width at the base (towards Saturn) is about 20,000 km. Their active times (during which they increase in width) range from 4000 to 12,000 sec. (2) Narrow spokes are found in the distance range 104,000 to 116,000 km, have sharply defined edges, and are narrowest at the corotation distance (112, 300 km). Their typical radial extension and width is 6000 and 2,000 km, respectively. (3) Filamentary spokes are found outside 110,000 km mostly joined with a wider spoke further in. They are typically 3000 km in length and 500 km in width. Their active time is less than 1000 sec. Several narrow spokes were observed during formation along radial lines in the sunlit portion of the ring. The formation time is typically ?5 min for a 6000-km-long spoke. The rate of spoke formation is highest at the morning ansa outside Saturn's shadow. Several spokes have been found where one edge revolves with Keplerian speed whereas the other edge stays radial. Recurrent spoke patterns have been observed at the period of Saturn's rotation. From edge-on views of the ring system, an upper limit for the height of spokes of 80 km is derived. |
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