Dynamics of Magnetic Flux Tubes in Thick Accretion Disks in AGNs and Associated Observational Effects

Details Dynamics of Magnetic Flux Tubes in Thick Accretion Disks in AGNs and Associated Observational Effects Dynamics of Magnetic Flux Tubes in Thick Accretion Disks in AGNs and Associated Observational Effects

Dec 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992aas...181.2905c&link_type=abstract

American Astronomical Society, 181st AAS Meeting, #29.05; Bulletin of the American Astronomical Society, Vol. 24, p.1166

Astronomy and Astrophysics

Astronomy

Scientific paper

We study the dynamics of the magnetic flux tubes in the thick accretion disks around black holes. It is shown that due to strong pressure gradient force inside the disk, buoyant flux tubes predominantly gather in the openings near to the axis, known as funnels, from where the cosmic radio jets are believed to be originated. We discuss various observational signatures of such behaviour of the flux tubes, such as microvariabilities in Blazars, particle acceleration, and jet formation close to the funnel.

Affiliated with

Also associated with

No associations

Rating

Dynamics of Magnetic Flux Tubes in Thick Accretion Disks in AGNs and Associated Observational Effects 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 Dynamics of Magnetic Flux Tubes in Thick Accretion Disks in AGNs and Associated Observational Effects, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Dynamics of Magnetic Flux Tubes in Thick Accretion Disks in AGNs and Associated Observational Effects will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1110565