Are Magnetic Dips Necessary for Prominence Formation?

By J. Karpen, S. Antiochos, M. Hohensee, J. Klimchuk, P. MacNeice. 2001

168 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/b5cee5aced16e28adf6ccd340d9954324dc76e8b

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. G. Aulanier
2. S. Gibson
3. Brigitte Schmieder
4. Yuhong Fan
5. Roberto Lionello
6. Jon A. Linker
7. Zoran Mikic
8. J. Klimchuk

In Molecular Biology

1. G. Aulanier
2. S. Gibson
3. Yuhong Fan
4. Brigitte Schmieder
5. J. Karpen
6. D. Mackay
7. J. Klimchuk
8. P. Démoulin

Citations in the corpus

• MULTISPECTRAL EMISSION OF THE SUN DURING THE FIRST WHOLE SUN MONTH: MAGNETOHYDRODYNAMIC SIMULATIONS (2008, methodology): “From the loop density and temperature distributions provided by the models, the emission (at least for optically thin lines) can be calculated (e.g., Karpen et al. 2001) using the CHIANTI database (Dere et al. 1997).”
• Coronal prominence structure and dynamics: A magnetic flux rope interpretation (2006, background): “The latter analyses were performed on sheared, dipped arcade fields rather than flux ropes (it has even been proposed that dips are not necessary for filament support: in sufficiently flat-topped arcade fields, a steadystate dynamic solution can be found to represent the filament [ Karpen et al., 20”
• Physics of Solar Prominences: II—Magnetic Structure and Dynamics (2010, background): “In long, low-lying flux tubes with shallow arches or dips, unequal quasi-steady heating yields a repetitive cycle of condensation formation, motion along the tube, and destruction by falling onto the nearest chromosphere (Antiochos et al., 2000; Karpen et al., 2001, 2006).”
• Dynamics of solar coronal loops I. Condensation in cool loops and its effect on transition region lines (2003, background): “Recently, it was demonstrated by Karpen et al. (2001) that the condition of a “dipped” geometry is indeed not a necessary condition for prominence formation in long loops (their work describes a loop of 340 Mm length).”
• On Solving the Coronal Heating Problem (2005, background): “To further emphasize this point, we note that moving transition regions can form at locations other than the base of the loop, such as at the sides of coronal condensations (e.g, Karpen et al., 2001; Karpen, Antiochos, and Klimchuk, 2005; Mueller, Hansteen, and Peter, 2003).”