IS THE MAGNETIC FIELD IN THE HELIOSHEATH LAMINAR OR A TURBULENT SEA OF BUBBLES?

IS THE MAGNETIC FIELD IN THE HELIOSHEATH LAMINAR OR A TURBULENT SEA OF BUBBLES?

All current global models of the heliosphere are based on the assumption that the magnetic field in the heliosheath, in the region close to the heliopause (HP), is laminar. We argue that in that region the heliospheric magnetic field is not laminar but instead consists of magnetic bubbles. We refer...

Cur síos iomlán

Sonraí bibleagrafaíochta
Príomhchruthaitheoirí: Opher, M., Drake, J. F., Swisdak, M., Schoeffler, K. M., Richardson, John D, Decker, R. B., Toth, G., Richardson, John D.
Rannpháirtithe: MIT Kavli Institute for Astrophysics and Space Research
Formáid: Alt
Teanga:en_US
Foilsithe / Cruthaithe: Institute of Physics/American Astronomical Society 2015
Rochtain ar líne:http://hdl.handle.net/1721.1/95712

Ar líne

http://hdl.handle.net/1721.1/95712

Míreanna comhchosúla