Astronomy and Astrophysics – Astrophysics
Scientific paper
Aug 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aipc..781..289w&link_type=abstract
THE PHYSICS OF COLLISIONLESS SHOCKS: 4th Annual IGPP International Astrophysics Conference. AIP Conference Proceedings, Volume
Astronomy and Astrophysics
Astrophysics
2
Shock Waves, Solar Wind, Interplanetary Magnetic Fields, Planetary Nebulae, Planetary Bow Shocks, Interplanetary Shocks, Interplanetary Magnetic Fields, Heliopause And Solar Wind Termination, Planetary Nebulae
Scientific paper
It is shown that the magnetic-pressure effect in the azimuthal direction in the heliosheath region results in the formation of a global V-shaped channel structure in both the heliopause and the termination shock surfaces. The physical processes involved in the formation of the V-shaped heliosphere is closely related with that of a bipolar-flow type Planetary Nebulae.
Tanaka Takashi
Washimi Haruichi
Zank Gary P.
No associations
LandOfFree
A Global V-Shaped Channel Structure of the Termination Shock Due to a Magnetic Pressure Effect, and Its Physical Connection to Bipolar Flow Type Planetary Nebulae 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 A Global V-Shaped Channel Structure of the Termination Shock Due to a Magnetic Pressure Effect, and Its Physical Connection to Bipolar Flow Type Planetary Nebulae, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A Global V-Shaped Channel Structure of the Termination Shock Due to a Magnetic Pressure Effect, and Its Physical Connection to Bipolar Flow Type Planetary Nebulae will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1344750