Helioseismology of Pre-Emerging Active Regions II: Average Emergence Properties
arXiv:1303.1391 · doi:10.1088/0004-637X/762/2/131
Abstract
We report on average subsurface properties of pre-emerging active regions as compared to areas where no active region emergence was detected. Helioseismic holography is applied to samples of the two populations (pre-emergence and without emergence), each sample having over 100 members, which were selected to minimize systematic bias, as described in Leka et al. We find that there are statistically significant signatures (i.e., difference in the means of more than a few standard errors) in the average subsurface flows and the apparent wave speed that precede the formation of an active region. The measurements here rule out spatially extended flows of more than about 15 m/s in the top 20 Mm below the photosphere over the course of the day preceding the start of visible emergence. These measurements place strong constraints on models of active region formation.
arXiv comment15 pages, 10 figures, ApJ (published)
References in corpus (8)
- The case for a distributed solar dynamo shaped by near-surface shear
- Simulation of the Formation of a Solar Active Region
- Local Helioseismology: Three Dimensional Imaging of the Solar Interior
- Solar Flux Emergence Simulations
- Photospheric and Subphotospheric Dynamics of Emerging Magnetic Flux
- Signatures of Emerging Subsurface Structures in Acoustic Power Maps
- Helioseismology of Pre-Emerging Active Regions I: Overview, Data, and Target Selection Criteria
- Time-Distance analysis of the Emerging Active Region NOAA 10790
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- Structure and Evolution of Magnetic Fields Associated with Solar Eruptions (Invited Review)
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- Helioseismology of Pre-Emerging Active Regions III: Statistical Analysis
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- Photospheric Velocity Structures during the Emergence of Small Active Regions on the Sun
- Impact of subsurface convective flows on the formation of sunspot magnetic field and energy build-up
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- Average solar active region: I. Intensities, velocities, and the photospheric magnetic field
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