Three-dimensional multi-fluid model of a coronal streamer belt with a tilted magnetic dipole

Ofman, L.; Provornikova, E.; Abbo, L.; Giordano, S.

doi:https://doi.org/10.5194/angeo-33-47-2015

Articles | Volume 33, issue 1

https://doi.org/10.5194/angeo-33-47-2015

© Author(s) 2015. This work is distributed under
the Creative Commons Attribution 3.0 License.

Special issue:

Observation, analysis and modelling of solar and heliospheric...

https://doi.org/10.5194/angeo-33-47-2015

© Author(s) 2015. This work is distributed under
the Creative Commons Attribution 3.0 License.

Articles | Volume 33, issue 1

Regular paper

|

12 Jan 2015

Regular paper |

| 12 Jan 2015

Three-dimensional multi-fluid model of a coronal streamer belt with a tilted magnetic dipole

L. Ofman, E. Provornikova, L. Abbo, and S. Giordano

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Cited

Latest update: 16 Jul 2024

Short summary

First results from the three-fluid 3D model of the solar corona are reported. The model extends previous 2.5D three-fluid studies, and includes electron, protons, and oxygen ions (O5+) as coupled fluids in a tilted dipole solar magnetic field configuration. The model demonstrates the variation in abundances of the oxygen ions relative to protons in a coronal streamer belt, thus identifying the sources of the slow solar wind and helping in the interpretation of past spectroscopic observations.

Three-dimensional multi-fluid model of a coronal streamer belt with a tilted magnetic dipole

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Cited

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