Annales Geophysicae
Annales Geophysicae
ANGEO
Articles | Volume 32, issue 11
Articles | Volume 32, issue 11
https://doi.org/10.5194/angeo-32-1441-2014
© Author(s) 2014. This work is distributed under
the Creative Commons Attribution 3.0 License.
https://doi.org/10.5194/angeo-32-1441-2014
© Author(s) 2014. This work is distributed under
the Creative Commons Attribution 3.0 License.
Articles | Volume 32, issue 11
Regular paper
 | Highlight paper
 | 
28 Nov 2014
Regular paper | Highlight paper |  | 28 Nov 2014

A comparison between VEGA 1, 2 and Giotto flybys of comet 1P/Halley: implications for Rosetta

M. Volwerk, K.-H. Glassmeier, M. Delva, D. Schmid, C. Koenders, I. Richter, and K. Szegö

Viewed

Total article views: 3,883 (including HTML, PDF, and XML)
HTML PDF XML Total BibTeX EndNote
2,920 782 181 3,883 99 94
  • HTML: 2,920
  • PDF: 782
  • XML: 181
  • Total: 3,883
  • BibTeX: 99
  • EndNote: 94
Views and downloads (calculated since 28 Nov 2014)
Cumulative views and downloads (calculated since 28 Nov 2014)

Cited

Latest update: 21 Nov 2024
Download
Short summary
We discuss three flybys (within an 8-day time span) of comet 1P/Halley by VEGA 1, 2 and Giotto. Looking at two different plasma phenomena: mirror mode waves and field line draping; we study the differences in SW--comet interaction between these three flybys. We find that on this time scale (comparable to Rosetta's orbits) there is a significant difference, both caused by changing outgassing rate of the comet and changes in the solar wind. We discuss implications for Rosetta RPC observations.
Read more