The North-South Asymmetry of the Heliospheric Current Sheet: Results of an MHD Simulation
| dc.contributor.author | Usmanov, Arcadi V. | |
| dc.contributor.author | Goldstein, Melvyn | |
| dc.date.accessioned | 2024-01-17T11:28:14Z | |
| dc.date.available | 2024-01-17T11:28:14Z | |
| dc.date.issued | 2013-01-01 | |
| dc.description | Modeling of Space Plasma Flows (ASTRONUM-2012), 2013 | |
| dc.description.abstract | A displacement of the heliospheric current sheet (HCS) south of the helioequator by approx.10deg was proposed by Simpson et al. (1996) as a possible explanation of the north-south asymmetry in the galactic cosmic rays observed by Ulysses during its first fast transit in 1994-1995. The idea was not supported by magnetic field measurements on Ulysses and, on this ground, was dismissed by Simpson et al. (1996). In addition, Erdos & Balogh (1998) argued that any north-south symmetry was unlikely as there should be flux balance between the magnetic sectors of opposite polarity. Nonetheless, many in the scientific community have accepted the original suggestion of Simpson et al. (1996) that a displacement of the HCS was responsible for the cosmic ray asymmetry. In this paper, using a magnetohydrodynamic model of the solar corona and solar wind that includes both dipole and quadrupole magnetic source terms, we show that a north-south asymmetry of the magnetic field on the Sun does not give rise to a displacement of the HCS. The lack of displacement of the HCS results from a latitudinal redistribution of magnetic flux near the Sun where the plasma beta much < 1. The latitudinal redistribution is a direct consequence of the magnetic field gradient between pole and equator. Near the Sun, the latitudinal gradient in magnetic field generates meridional flows directed equatorward that tend to relax the gradient in the magnetic field (to make it more latitude-independent) as heliocentric distance increases. If there is an asymmetry between north and south magnetic field strength then the meridional flows are also asymmetric (i.e., stronger in the hemisphere of stronger magnetic field). Because the magnetic fluxes (positive and negative) in the hemispheres must be equal, the redistribution shifts the HCS into balance by approx. 16 R(solar mass). At larger distances, where the magnetic field is relatively weak (beta much > 1), the HCS can be displaced if there is a difference in total pressure between the hemispheres. | |
| dc.description.sponsorship | The work of AVU was supported by the NSF/DOE Partnership in Basic Plasma Science and Engineering Program grant AST-1004035, and by NASA grant NNX09AH79G to the University of Delaware. Resources supporting this work were provided by the NASA High-End Computing (HEC) Program through the NASA Advanced Supercomputing (NAS) Division at the Ames Research Center and the NASA Center for Climate Simulation (NCCS) at the Goddard Space Flight Center | |
| dc.description.uri | https://ntrs.nasa.gov/citations/20140010318 | |
| dc.format.extent | 6 pages | |
| dc.genre | conference papers and proceedings | |
| dc.identifier.citation | Usmanov, Arcadi V., and Melvyn L. Goldstein. “The North-South Asymmetry of the Heliospheric Current Sheet: Results of an MHD Simulation.” Astronomical Society of the Pacific Conference Series: Numerical Modeling of Space Plasma Flows (ASTRONUM-2012) 474 (January 1, 2013). https://ntrs.nasa.gov/citations/20140010318. | |
| dc.identifier.uri | http://hdl.handle.net/11603/31299 | |
| dc.language.iso | en_US | |
| dc.publisher | Astronomical Society of the Pacific | |
| dc.relation.isAvailableAt | The University of Maryland, Baltimore County (UMBC) | |
| dc.relation.ispartof | UMBC Goddard Planetary Heliophysics Institute (GPHI) | |
| dc.rights | This work was written as part of one of the author's official duties as an Employee of the United States Government and is therefore a work of the United States Government. In accordance with 17 U.S.C. 105, no copyright protection is available for such works under U.S. Law. | |
| dc.rights | Public Domain Mark 1.0 | en |
| dc.rights.uri | https://creativecommons.org/publicdomain/mark/1.0/ | |
| dc.title | The North-South Asymmetry of the Heliospheric Current Sheet: Results of an MHD Simulation | |
| dc.type | Text | |
| dcterms.creator | https://orcid.org/0000-0002-5317-988X |
