𝔖 Bobbio Scriptorium
✦   LIBER   ✦

MHD interaction of pulsar wind nebulae with SNRs and with the ISM

✍ Scribed by E. van der Swaluw

Publisher
Elsevier Science
Year
2005
Tongue
English
Weight
327 KB
Volume
35
Category
Article
ISSN
0273-1177

No coin nor oath required. For personal study only.

πŸ“œ SIMILAR VOLUMES

Spectral analysis of the Crab Pulsar and
Spectral analysis of the Crab Pulsar and Nebula with the Fermi Large Area Telescope
✍ F. Loparco πŸ“‚ Article πŸ“… 2011 πŸ› Elsevier Science 🌐 English βš– 201 KB

The Crab Pulsar is a relatively young neutron star. The Pulsar is the central star in the Crab Nebula, a remnant of the supernova SN 1054, which was observed on Earth in the year 1054. The Crab Pulsar has been extensively observed in the gamma-ray energy band by the Large Area Telescope (LAT), the m

Multiscale MHD simulation of a coronal m
Multiscale MHD simulation of a coronal mass ejection and its interaction with the magnetosphere–ionosphere system
✍ T.I. Gombosi; D.L. DeZeeuw; C.P.T. Groth; K.G. Powell; Q.F. Stout πŸ“‚ Article πŸ“… 2000 πŸ› Elsevier Science 🌐 English βš– 758 KB

We report on the ΓΏrst comprehensive numerical simulation of a space weather event, starting with the generation of a CME and subsequently following this transient solar wind disturbance as it evolves into a magnetic cloud and travels through interplanetary space towards Earth where its interaction w