Magnetic field structures for inverse polarity prominences.

A. O. Schönfelder; A. W. Hood; R. A. S. Fiedler

Magnetic field structures for inverse polarity prominences.

A. O. Schönfelder, A. W. Hood, R. A. S. Fiedler

Applied Mathematics

Research output: Contribution to journal › Article › peer-review

Abstract

Results of numerical solutions to the equilibrium equation indicate that a fully developed prominence will possess an O-type, but not in general an X-type neutral point.

Original language	English
Pages (from-to)	335-338
Journal	Solar Coronal Structures. Proceedings of the 144th IAU Colloquium held in Tatranska Lomnica; Slovakia; September 20-14; 1993; on the occasion of the 50th anniversary of the Skalnate Pleso Observatory; Tatranska Lomnica: VEDA Publishing House of the Slovak Academy of Sciences; edited by Vojtech Rusin, Petr Heinzel and Jean-Claude Vial, 1994
Publication status	Published - 1994

Keywords

Solar Prominences: Structure
Solar Prominences: Numerical Simulations
Solar Prominences: Solar Magnetic Fields

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http://adsabs.harvard.edu/abs/1994scs..conf..335S

Cite this

Schönfelder, A. O., Hood, A. W., & Fiedler, R. A. S. (1994). Magnetic field structures for inverse polarity prominences. Solar Coronal Structures. Proceedings of the 144th IAU Colloquium held in Tatranska Lomnica; Slovakia; September 20-14; 1993; on the occasion of the 50th anniversary of the Skalnate Pleso Observatory; Tatranska Lomnica: VEDA Publishing House of the Slovak Academy of Sciences; edited by Vojtech Rusin, Petr Heinzel and Jean-Claude Vial, 1994, 335-338. http://adsabs.harvard.edu/abs/1994scs..conf..335S

Schönfelder, A. O. ; Hood, A. W. ; Fiedler, R. A. S. / Magnetic field structures for inverse polarity prominences. In: Solar Coronal Structures. Proceedings of the 144th IAU Colloquium held in Tatranska Lomnica; Slovakia; September 20-14; 1993; on the occasion of the 50th anniversary of the Skalnate Pleso Observatory; Tatranska Lomnica: VEDA Publishing House of the Slovak Academy of Sciences; edited by Vojtech Rusin, Petr Heinzel and Jean-Claude Vial, 1994. 1994 ; pp. 335-338.

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title = "Magnetic field structures for inverse polarity prominences.",

abstract = "Results of numerical solutions to the equilibrium equation indicate that a fully developed prominence will possess an O-type, but not in general an X-type neutral point.",

keywords = "Solar Prominences: Structure, Solar Prominences: Numerical Simulations, Solar Prominences: Solar Magnetic Fields",

author = "Sch{\"o}nfelder, {A. O.} and Hood, {A. W.} and Fiedler, {R. A. S.}",

year = "1994",

language = "English",

pages = "335--338",

journal = "Solar Coronal Structures. Proceedings of the 144th IAU Colloquium held in Tatranska Lomnica; Slovakia; September 20-14; 1993; on the occasion of the 50th anniversary of the Skalnate Pleso Observatory; Tatranska Lomnica: VEDA Publishing House of the Slovak Academy of Sciences; edited by Vojtech Rusin, Petr Heinzel and Jean-Claude Vial, 1994",

}

Schönfelder, AO, Hood, AW & Fiedler, RAS 1994, 'Magnetic field structures for inverse polarity prominences.', Solar Coronal Structures. Proceedings of the 144th IAU Colloquium held in Tatranska Lomnica; Slovakia; September 20-14; 1993; on the occasion of the 50th anniversary of the Skalnate Pleso Observatory; Tatranska Lomnica: VEDA Publishing House of the Slovak Academy of Sciences; edited by Vojtech Rusin, Petr Heinzel and Jean-Claude Vial, 1994, pp. 335-338. <http://adsabs.harvard.edu/abs/1994scs..conf..335S>

Magnetic field structures for inverse polarity prominences. / Schönfelder, A. O.; Hood, A. W.; Fiedler, R. A. S.
In: Solar Coronal Structures. Proceedings of the 144th IAU Colloquium held in Tatranska Lomnica; Slovakia; September 20-14; 1993; on the occasion of the 50th anniversary of the Skalnate Pleso Observatory; Tatranska Lomnica: VEDA Publishing House of the Slovak Academy of Sciences; edited by Vojtech Rusin, Petr Heinzel and Jean-Claude Vial, 1994, 1994, p. 335-338.

Research output: Contribution to journal › Article › peer-review

TY - JOUR

T1 - Magnetic field structures for inverse polarity prominences.

AU - Schönfelder, A. O.

AU - Hood, A. W.

AU - Fiedler, R. A. S.

PY - 1994

Y1 - 1994

N2 - Results of numerical solutions to the equilibrium equation indicate that a fully developed prominence will possess an O-type, but not in general an X-type neutral point.

AB - Results of numerical solutions to the equilibrium equation indicate that a fully developed prominence will possess an O-type, but not in general an X-type neutral point.

KW - Solar Prominences: Structure

KW - Solar Prominences: Numerical Simulations

KW - Solar Prominences: Solar Magnetic Fields

M3 - Article

SP - 335

EP - 338

JO - Solar Coronal Structures. Proceedings of the 144th IAU Colloquium held in Tatranska Lomnica; Slovakia; September 20-14; 1993; on the occasion of the 50th anniversary of the Skalnate Pleso Observatory; Tatranska Lomnica: VEDA Publishing House of the Slovak

JF - Solar Coronal Structures. Proceedings of the 144th IAU Colloquium held in Tatranska Lomnica; Slovakia; September 20-14; 1993; on the occasion of the 50th anniversary of the Skalnate Pleso Observatory; Tatranska Lomnica: VEDA Publishing House of the Slovak

ER -

Schönfelder AO, Hood AW, Fiedler RAS. Magnetic field structures for inverse polarity prominences. Solar Coronal Structures. Proceedings of the 144th IAU Colloquium held in Tatranska Lomnica; Slovakia; September 20-14; 1993; on the occasion of the 50th anniversary of the Skalnate Pleso Observatory; Tatranska Lomnica: VEDA Publishing House of the Slovak Academy of Sciences; edited by Vojtech Rusin, Petr Heinzel and Jean-Claude Vial, 1994. 1994;335-338.

Magnetic field structures for inverse polarity prominences.

Abstract

Keywords

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