Résumé
The experiments to simulate astrophysical jet generation are performed using Gekko XII (GXII) HIPER laser system at the Institute of Laser Engineering. In the experiments a fast plasma flow generated by shooting a CH plane (10 μm thickness) is observed at the rear side of the plane. By separating the focal spot of the main beams, a non-uniform plasma is generated. The non-uniform plasma flow in an external magnetic field (0.2∼0.3 T) perpendicular to the plasma is more collimated than that without the external magnetic field. The plasma β, the ratio between the plasma and magnetic pressure, is ≠1, and the magnetic Reynolds number is ∼150 in the collimated plasma. It is considered that the magnetic field is distorted by the plasma flow and enhances the jet collimation.
| langue originale | Anglais |
|---|---|
| titre | IFSA 2011 - 7th International Conference on Inertial Fusion Sciences and Applications |
| Les DOIs | |
| état | Publié - 1 déc. 2013 |
| Evénement | 7th International Conference on Inertial Fusion Sciences and Applications, IFSA 2011 - Bordeaux, France Durée: 12 sept. 2011 → 16 sept. 2011 |
Série de publications
| Nom | EPJ Web of Conferences |
|---|---|
| Volume | 59 |
| ISSN (imprimé) | 2101-6275 |
| ISSN (Electronique) | 2100-014X |
Une conférence
| Une conférence | 7th International Conference on Inertial Fusion Sciences and Applications, IFSA 2011 |
|---|---|
| Pays/Territoire | France |
| La ville | Bordeaux |
| période | 12/09/11 → 16/09/11 |
Empreinte digitale
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