coronal filament cavities: why there is a there there and what to do about it
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Coronal filament cavities: why there is a there there and what to do about it. NCAR/HAO Newkirk WLCC telescope, March 18 1988 eclipse, Philippines. Sarah Gibson Jim Fuller , Giuliana de Toma, and Yuhong Fan. - PowerPoint PPT PresentationTRANSCRIPT
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Coronal filament cavities: why there is a there there and what to do about it
Sarah Gibson
Jim Fuller, Giuliana de Toma, and Yuhong Fan
NCAR/HAO Newkirk WLCC telescope, March 18 1988 eclipse, Philippines
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Talk outline
• Background/Motivation
• Model geometry
• Calculating density, temperature
• Implications for emission cavities
• Implications for magnetic field
• Conclusions
NCAR/HAO Newkirk WLCC telescope, March 18 1988 eclipse, Philippines
Problem: quantitative interpretation of cavities is complicated by the potential for projection of non-cavity plasma along the line of sight
Our solution: use geometric arguments to establish cases where non-cavity contributions are minimal, and include them as model uncertainties
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Quiescent cavity: November 18, 1999
CME eruption of cavity: November 19, 1999
CME eruption of cavity: flux rope model (Gibson and Fan, 2006)
Background: cavity --> CME
• Cavites are known to be CME precursors
• Highly suggestive of flux rope topology
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As early as eclipse of Jan 22, 1898, white light observations have demonstrated the presence of non-eruptive 3-part structures: prominence/cavity/helmet
• Prominence cavity = filament channel viewed at limb:
ubiquitous…
QuickTime™ and aTIFF (Uncompressed) decompressor
are needed to see this picture.
Background: cavities as filament channels
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…But low-lying!
Innermost to outermost: EIT 284, Mark IV, Lasco C2, Lasco C3
Quiescent cavities occur in the low corona
Background: cavities as filament channels
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Model geometry: Cavity as axisymmetric “tunnel”
• Matches observations of polar crown filaments (PCFs)
• Cavity rim as denser surrounding tunnel
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Model geometry: Best cavities for avoiding cavity rim projection
• Better for lower plane-of-sky heights
• Better for big cavities, nearer equator (less curvature)
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Model geometry: Best cavities for avoiding cavity legs projection
• Only needs to be a torus for as long as line of sight passes through
• Better for higher plane-of-sky heights
• Better for small cavities (more curvature)
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White light cavity that meets criteria: (Jan 25-31, 2006)
• Big enough (radius) for minimal rim projection
• Long-lived enough (longitudinal extent) for minimal leg projection
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Rim vs. Cavity profiles
• Include departure from axisymmetry as error bars
• Fit linear power law for polarized brightness vs. height
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Density, temperature and pressure
• Fit van de Hulst inversion to pB profiles to obtain density profiles
• Assumed polytropic and solved for ``hydrostatic’’ temperature and pressure
Density (cgs) Cavity: black/blue; Rim: purple/blue
RESULTS
• Density smaller in cavity (as much as 40%), but flatter profile vs. height than rim
• Cavity 21% hotter than rim! (but be careful…)
• Pressure still smaller in cavity, and profile flatter than rim
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Implications for emission cavity• Independent temperature diagnostics needed
• Geometry of model can also be used for emission cavities
• Rim projection not a problem: rim at heights where no emission (note cavity has no top on August 9-10
• Cavity axisymmetric enough so legs not a problem either for August 9
• Temperature diagnostics have been taken for this cavity in IHY filament/cavity campaign! (SOHO/CDS, Hinode/EIS)
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Implications for emission cavity• When cavities well-resolved in emission, minimal overlap with white
light
• Could use emission observations at the base of large white light cavity, but then substructure an issue
• IHY cavity about as good-sized as could be hoped for overlap of analysis
• Eclipse would be ideal!
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Implications for magnetic field• Axisymmetric flux rope model (Fan and Gibson, 2006)
• Flat density profile in cavity vs. rim:
• Total pressure continuity: gas pressure decrease across boundary compensated for by magnetic pressure increase
• DeltaP/P maximum at flux surface nearest flux rope axis, then decrease with height
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There is a there there!
• Cavity density double or more than coronal hole density
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Conclusions
• Unobservable? No!
• Projection effects of unrelated material can be dealt with
• Cavity plasma significantly denser than corona hole
• Assuming a polytropic profile, found that cavity hotter than rim
• Needs independent confirmation from temperature line diagnostics
• Flat density profile consistent with magnetic flux rope model
• Observations of cavity rising, getting more sharply defined in the 24 hours before a CME: possible indicator of magnetic energy reaching a critical threshold for eruption?