Nature Communications (Feb 2021)
Laboratory disruption of scaled astrophysical outflows by a misaligned magnetic field
- G. Revet,
- B. Khiar,
- E. Filippov,
- C. Argiroffi,
- J. Béard,
- R. Bonito,
- M. Cerchez,
- S. N. Chen,
- T. Gangolf,
- D. P. Higginson,
- A. Mignone,
- B. Olmi,
- M. Ouillé,
- S. N. Ryazantsev,
- I. Yu. Skobelev,
- M. I. Safronova,
- M. Starodubtsev,
- T. Vinci,
- O. Willi,
- S. Pikuz,
- S. Orlando,
- A. Ciardi,
- J. Fuchs
Affiliations
- G. Revet
- Institute of Applied Physics RAS
- B. Khiar
- Sorbonne Université, Observatoire de Paris, PSL Research University, LERMA
- E. Filippov
- Institute of Applied Physics RAS
- C. Argiroffi
- Dipartimento di Fisica e Chimica, Universitá di Palermo
- J. Béard
- LNCMI, UPR 3228, CNRS-UGA-UPS-INSA
- R. Bonito
- INAF-Osservatorio Astronomico di Palermo
- M. Cerchez
- Institut für Laser und Plasmaphysik, Heinrich Heine Universität Düsseldorf
- S. N. Chen
- Institute of Applied Physics RAS
- T. Gangolf
- LULI, CNRS, CEA, Sorbonne Université, École Polytechnique, Institut Polytechnique de Paris
- D. P. Higginson
- LULI, CNRS, CEA, Sorbonne Université, École Polytechnique, Institut Polytechnique de Paris
- A. Mignone
- Dip. di Fisica, Universiá di Torino
- B. Olmi
- INAF-Osservatorio Astronomico di Palermo
- M. Ouillé
- LULI, CNRS, CEA, Sorbonne Université, École Polytechnique, Institut Polytechnique de Paris
- S. N. Ryazantsev
- Joint Institute for High Temperatures RAS
- I. Yu. Skobelev
- Joint Institute for High Temperatures RAS
- M. I. Safronova
- Institute of Applied Physics RAS
- M. Starodubtsev
- Institute of Applied Physics RAS
- T. Vinci
- LULI, CNRS, CEA, Sorbonne Université, École Polytechnique, Institut Polytechnique de Paris
- O. Willi
- Institut für Laser und Plasmaphysik, Heinrich Heine Universität Düsseldorf
- S. Pikuz
- Joint Institute for High Temperatures RAS
- S. Orlando
- INAF-Osservatorio Astronomico di Palermo
- A. Ciardi
- Sorbonne Université, Observatoire de Paris, PSL Research University, LERMA
- J. Fuchs
- Institute of Applied Physics RAS
- DOI
- https://doi.org/10.1038/s41467-021-20917-x
- Journal volume & issue
-
Vol. 12,
no. 1
pp. 1 – 10
Abstract
Mass outflow is a common process in astrophysical objects. Here the authors investigate in which conditions an astrophysically-scaled laser-produced plasma flow can be collimated and evolves in the presence of a misaligned external magnetic field.
