pi-Puppids 2013: prediction of activity
Fig. 1. Space-temporal projection of pi-Puppids trails parts onto their minimal distance passages (correspondence between colours of the particles and their ejection velocities can be seen here).
Fig. 1. Detailed space-temporal projection of pi-Puppids trails parts onto their minimal distance passages in 2013 (correspondence between colours of the particles and their ejection velocities can be seen here).
No encounters with trails are found. Activity is not expected.
References
1. "Comet's dust 2.0" program by S. Shanov and S. Dubrovsky. [Used for computation of stream particles orbital evolution]
2. Kazuo Kinosita, http://www9.ocn.ne.jp/~comet/index.html [Orbital elements of the comet 26P Grigg-Skjellerup.]
3. Lyytinen E, van Flandern T. "Predicting the strength of Leonid outbursts", 2000, Icarus, P. 158-160.
References
1. "Comet's dust 2.0" program by S. Shanov and S. Dubrovsky. [Used for computation of stream particles orbital evolution]
2. Kazuo Kinosita, http://www9.ocn.ne.jp/~comet/index.html [Orbital elements of the comet 26P Grigg-Skjellerup.]
3. Lyytinen E, van Flandern T. "Predicting the strength of Leonid outbursts", 2000, Icarus, P. 158-160.