Z. Meliani | Observatoire de Paris (original) (raw)

Z. Meliani

I am a Associate Astronomer at LUTh, Observatoire de Paris.My current research interests concern fluid code development and numerical simulation

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Papers by Z. Meliani

Monthly Notices of the Royal Astronomical Society, 2012

AIP Conference Proceedings, 2007

In parallel to the development of numerical simulations, analytical solutions for modelling the a... more In parallel to the development of numerical simulations, analytical solutions for modelling the acceleration and the collimation of winds and jets have been proposed. We present here how meridionally self-similar solutions can be used to model the solar wind using Ulysses data at solar minimum. Such solutions may also be adapted to explain the formation core or spine jets in classical and weak TTauri stars (class II and III young stellar jets) as well as relativistic jet cores from AGN. The criterion for collimation explains how the jet evolves towards a wind as the star approaches the main sequence. A similar scenario could explain the winds from Seyfert galaxies by opposition to the powerful jets from Fanaroff Riley sources.

Lecture Notes in Physics, 2009

... Z. Meliani Centre for Plasma Astrophysics, KULeuven, Belgium, Zakaria.Meliani@wis.kuleuven. b... more ... Z. Meliani Centre for Plasma Astrophysics, KULeuven, Belgium, Zakaria.Meliani@wis.kuleuven. be ... 2.3 Wake-Current Sheets A relevant, closely related study is found in local box computations of the solar coronal streamer belt [31]. As sketched in Fig. ...