FARLEY-BUNEMAN INSTABILITY IN THE SOLAR CHROMOSPHERE

Journal Article · Fri Nov 20 04:00:00 EST 2009 · Astrophysical Journal (Online)

DOI:https://doi.org/10.1088/0004-637X/706/1/L12· OSTI ID:21378239

Gogoberidze, G; Voitenko, Y; Poedts, S; Goossens, M ^[1]

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1. CPA/K.U.Leuven, Celestijnenlaan 200B, 3001 Leuven (Belgium)

The Farley-Buneman instability (FBI) is studied in the partially ionized plasma of the solar chromosphere taking into account the finite magnetization of the ions and Coulomb collisions. We obtain the threshold value for the relative velocity between ions and electrons necessary for the instability to develop. It is shown that Coulomb collisions play a destabilizing role in the sense that they enable the instability even in the regions where the ion magnetization is larger than unity. By applying these results to chromospheric conditions, we show that the FBI cannot be responsible for the quasi-steady heating of the solar chromosphere. However, we do not exclude the instability development locally in the presence of strong cross-field currents and/or strong small-scale magnetic fields. In such cases, FBI should produce locally small-scale, approx0.1-3 m, density irregularities in the solar chromosphere. These irregularities can cause scintillations of radio waves with similar wave lengths and provide a tool for remote chromospheric sensing.

• OSTI ID: 21378239
• Journal Information: Astrophysical Journal (Online), Journal Name: Astrophysical Journal (Online) Journal Issue: 1 Vol. 706; ISSN 1538-4357
• Country of Publication: United States
• Language: English

Related Subjects

71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
79 ASTRONOMY AND ASTROPHYSICS
ATMOSPHERES
CHROMOSPHERE
ELECTROMAGNETIC RADIATION
ELECTRONS
ELEMENTARY PARTICLES
FERMIONS
INSTABILITY
LEPTONS
MAGNETIC FIELDS
MAGNETIZATION
MAIN SEQUENCE STARS
RADIATIONS
RADIOWAVE RADIATION
SCINTILLATIONS
SOLAR ATMOSPHERE
STARS
STELLAR ATMOSPHERES
SUN