Modeling Penumbral Microjets by Two-Fluid Simulations

We investigate how penumbral microjets, recently observed by the Hinode satellite, can be produced within sunspot penumbra. We consider two penumbral filaments with axial currents and axial flows. We assume that a vertical magnetic flux tube exists between two horizontal penumbral filaments. We also...

Full description

Saved in:
Bibliographic Details
Published inThe Astrophysical journal Vol. 687; no. 2; pp. L127 - L130
Main Authors Sakai, J. I, Smith, P. D
Format Journal Article
LanguageEnglish
Published Chicago, IL IOP Publishing 10.11.2008
University of Chicago Press
Subjects
Astronomy
Earth, ocean, space
Exact sciences and technology
Plasma
Sun : photosphere
plasmas
Sun : magnetic fields
MHD
Modelling
Magnetic fields
Sun
Online AccessGet full text

Cover

More Information
Summary:We investigate how penumbral microjets, recently observed by the Hinode satellite, can be produced within sunspot penumbra. We consider two penumbral filaments with axial currents and axial flows. We assume that a vertical magnetic flux tube exists between two horizontal penumbral filaments. We also assume that the axial flows are not steady; a high- velocity axial flow is imposed on the background slow axial flow. We find that this high-velocity axial flow can trigger magnetic reconnection between one penumbral filament and the vertical flux tube. As a result, inclined bidirectional jetlike flows, driven by the magnetic reconnection, propagate along the vertical magnetic flux tube. Strong proton heating, up to 25 times their original temperature, is observed in these generated jets. Conversely, the neutral-hydrogen particles are only very weakly heated. We propose that these plasma jets explain the phenomenon of penumbral microjets, recently observed by the Hinode satellite.
Bibliography:ObjectType-Article-2
SourceType-Scholarly Journals-1
ObjectType-Feature-1
content type line 23
ISSN:1538-4357
0004-637X
1538-4357
DOI:10.1086/593204