Formation of magnetic-tower jets in magnetohydrodynamic accretion flows

Details Formation of magnetic-tower jets in magnetohydrodynamic accretion flows Formation of magnetic-tower jets in magnetohydrodynamic accretion flows

Aug 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005asthe..98..525k&link_type=abstract

The Astronomical Herald (ISSN 0374-2466), Vol. 98, No. 8, p. 525 - 532 (2005)

Astronomy and Astrophysics

Astrophysics

Magnetohydrodynamics: Jets

Scientific paper

The previous study of astrophysical jets has been concentrated on the effects of large-scale magnetic fields permeating accretion disks. However, the existence of such global magnetic fields is not evident in many astrophysical objects. Instead, the magnetic fields, generated in the disks as a result of magneto-rotational instability, can create jets accelerated by the magnetic pressure of the magnetic-tower. We describe our attempt to explore the magnetic-tower jet solution as a unified model of astrophysical jets.

Affiliated with

Also associated with

No associations

Rating

Formation of magnetic-tower jets in magnetohydrodynamic accretion flows does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Formation of magnetic-tower jets in magnetohydrodynamic accretion flows, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Formation of magnetic-tower jets in magnetohydrodynamic accretion flows will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1347708