Unusual nonlinear waves in the Venusian magnetosheath
Within the Venusian magnetosheath, Venus Express has observed the existence of high‐amplitude, nonlinear waves which have been interpreted as large‐scale nonlinear rotational structures within the magnetic field. A number of mechanisms have been proposed that can be used to explain their origin. Ven...
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| Veröffentlicht in: | Journal of Geophysical Research: Space Physics 2011-01, Vol.116 (A1), p.n/a |
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| container_title | Journal of Geophysical Research: Space Physics |
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| creator | Walker, S. N. Balikhin, M. A. Zhang, T. L. Gedalin, M. E. Pope, S. A. Dimmock, A. P. Fedorov, A. O. |
| description | Within the Venusian magnetosheath, Venus Express has observed the existence of high‐amplitude, nonlinear waves which have been interpreted as large‐scale nonlinear rotational structures within the magnetic field. A number of mechanisms have been proposed that can be used to explain their origin. Venus Express data have been searched for other examples of the similar structures. It appears that such structures are quite rare, being observed during only 8 of the dayside magnetosheath crossings among 676 that took place between April 2006 and February 2008. All together, only 50 such waves have been identified during these 8 crossings. The properties of these structures were studied. After considering a number of possible generation mechanisms, it is concluded that the most probable generation mechanism is the Kelvin‐Helmholtz Instability; however, other mechanisms such as shock‐related processes cannot be completely discounted. |
| doi_str_mv | 10.1029/2010JA015916 |
| format | Article |
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It appears that such structures are quite rare, being observed during only 8 of the dayside magnetosheath crossings among 676 that took place between April 2006 and February 2008. All together, only 50 such waves have been identified during these 8 crossings. The properties of these structures were studied. After considering a number of possible generation mechanisms, it is concluded that the most probable generation mechanism is the Kelvin‐Helmholtz Instability; however, other mechanisms such as shock‐related processes cannot be completely discounted.</description><subject>Astronomy</subject><subject>Astrophysics</subject><subject>Comets</subject><subject>Earth sciences</subject><subject>Earth, ocean, space</subject><subject>Exact sciences and technology</subject><subject>Magnetic fields</subject><subject>Magnetism</subject><subject>magnetosheath</subject><subject>Physics</subject><subject>Planetology</subject><subject>Planets</subject><subject>Sun</subject><subject>Venus</subject><issn>0148-0227</issn><issn>2169-9380</issn><issn>2156-2202</issn><issn>2169-9402</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2011</creationdate><recordtype>article</recordtype><sourceid>BENPR</sourceid><recordid>eNpNkE9Lw0AQxRdRsNTe_ABB8Bid3U32z7EUWy1BQWo9LpvNxqamm5pNrP32rrQU5zIM7_dmmIfQNYY7DETeE8AwHwNOJWZnaEBwymJCgJyjAeBExEAIv0Qj79cQKklZAniA0jfX-17XkWtcXTmr22inv62PKhd1KxstbdAr7aKN_nC2a_zK6m51hS5KXXs7OvYhWkwfFpPHOHuZPU3GWWySBEPMc5znFhuRFLmUhjCbUCZICZRpIQpjc1xKWhQ0tRobUhrMgOSMi5zqMNIhujms3bbNV299p9ZN37pwUYUnOeFCpgG6PULaG12XrXam8mrbVhvd7hWhknMhRODogdtVtd2fdAzqLz71Pz41n72OCUgMwRUfXJXv7M_JpdtPxTjlqXp_nimWLpbTLJuFY78zMXHt</recordid><startdate>201101</startdate><enddate>201101</enddate><creator>Walker, S. 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N.</au><au>Balikhin, M. A.</au><au>Zhang, T. L.</au><au>Gedalin, M. E.</au><au>Pope, S. A.</au><au>Dimmock, A. P.</au><au>Fedorov, A. O.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Unusual nonlinear waves in the Venusian magnetosheath</atitle><jtitle>Journal of Geophysical Research: Space Physics</jtitle><addtitle>J. Geophys. Res</addtitle><date>2011-01</date><risdate>2011</risdate><volume>116</volume><issue>A1</issue><epage>n/a</epage><issn>0148-0227</issn><issn>2169-9380</issn><eissn>2156-2202</eissn><eissn>2169-9402</eissn><abstract>Within the Venusian magnetosheath, Venus Express has observed the existence of high‐amplitude, nonlinear waves which have been interpreted as large‐scale nonlinear rotational structures within the magnetic field. A number of mechanisms have been proposed that can be used to explain their origin. Venus Express data have been searched for other examples of the similar structures. 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| source | Wiley Online Library - AutoHoldings Journals; Wiley-Blackwell AGU Digital Library; Wiley Online Library Free Content; Alma/SFX Local Collection |
| subjects | Astronomy Astrophysics Comets Earth sciences Earth, ocean, space Exact sciences and technology Magnetic fields Magnetism magnetosheath Physics Planetology Planets Sun Venus |
| title | Unusual nonlinear waves in the Venusian magnetosheath |
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