Physics
Scientific paper
Jun 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002georl..29k..23t&link_type=abstract
Geophysical Research Letters, Volume 29, Issue 11, pp. 23-1, CiteID 1528, DOI 10.1029/2001GL013623
Physics
17
Interplanetary Physics: Discontinuities, Interplanetary Physics: Energetic Particles, Heliospheric (7514), Interplanetary Physics: Interplanetary Magnetic Fields, Interplanetary Physics: Mhd Waves And Turbulence
Scientific paper
Ulysses magnetic field data are used to study magnetic field microstructure over the solar poles. Magnetic holes (MHs) and magnetic decreases (MDs) are found to be located at the phase-steepened edges of nonlinear Alfvén waves. The phase-steepened edges (directional discontinuities) occur in time-coincidence with MHs, one edge of an MD, or throughout the whole MD. These MH- and MD-related discontinuities have both rotational and compressive properties, perhaps explaining why many directional discontinuities detected in interplanetary space have non-MHD properties. The dispersive, dissipative and compressive features of nonlinear Alfvén waves may be important for the heating of the solar corona.
Arballo John K.
Balogh André
Buti B.
Galvan Carlos
Lakhina Gurbax S.
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