Meeting update -- 02/12/2018

  • Laurence Sabin's Visit
    1. Time
    2. Projects 

The main goal would be using the hydrodynamical model that you already published with Bruce and
 add the "magnetic component" to fit our observations.

It would also be interesting to combine this with Martin's (synthetic) polarization maps 
to reflect what we are observing with the SMA, CARMA and ALMA.


A second point, that was raised during the PNe conference Adam and I attended 
last year, is the determination of the minimum field's intensity needed to 

trigger the shaping. This is a very important and rather unknown aspect:  
I am working on the measurement of photospheric magnetic fields, on Post-AGBs and PPNe, and so far the
 (longitudinal) values found are quite low and might not be enough to actually launch any material !!
  1. Current JetClump Module: 2D MHD (Toroidal magnetic field in Clump and Jet ) runs OK. 3D MHD untested.

Comments

No comments.