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Published byἸούλιος Μανωλάς Modified over 5 years ago
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Prediction for Encounter with Ion Tail of Comet
45P/Honda-Mrkos-Pajdusakova, ~July 6, 2006 (Sofie Spjuth) Green: comet path Yellow: ion tail for various vsw (blue: 400 km/s) Red square: Rosetta For vsw = 400 km/s, Rosetta passed within 0.05 AU from ion tail at ~0.7 AU from comet.
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Problem(-s) And the list is not exhaustive...
Comet tail all to wide Current (from MAG) does not make sense -- radial along tail direction What is this? What should a real comet tail look like?
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Ulysses Encounter with Hyakutake Ion Tail May 1, 1996
Now concluded by Some to be no comet tail at all... Ulysses-comet: > 3 AU Rosetta-comet: 0.7 AU Jones et al., Nature, 2000
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So, are there any real comet tail observations?
Sofie also checked for possible tail crossings for other s/c, including Spaceship Earth PRAO-student Martin Hult checked ACE/IMP-8 data for Sofie’s pre- and postdictions Best event: P/Catalina (2005 JQ5) July 9, (DOY 190)
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Something? + current sheet(?) + heavy ions - but density jump...
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Is this a comet tail crossing?
Minimum variance on B? Models for what to find? Other s/w disturbances -- what do they look like?? What do you know? Any unambiguous signature of a comet tail? Ideas? Comments?
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