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Photospheric Flows and Magnetic Fields, and Their Role in CME/Flare Initiation

Photospheric Flows and Magnetic Fields, and Their Role in CME/Flare Initiation

Photospheric Flows and Magnetic Fields, and Their Role in CME/Flare Initiation. Brian T. Welsch Space Sciences Lab, UC-Berkeley Although CMEs and flares are coronal phenomena, magnetic evolution at the photosphere must play a key role in driving the corona into an unstable state.

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529 views • 39 slides
Solar Sherlock: Investigating a complex X-class flare using NLFFF modeling

Solar Sherlock: Investigating a complex X-class flare using NLFFF modeling

Solar Sherlock: Investigating a complex X-class flare using NLFFF modeling. Blake Forland. Mentor:. Yingna Su. Prominence Eruption. Introduction. Flares. CME. Eruptions on the Sun. Contribute to space weather.

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367 views • 24 slides
Flare: motion of H-alpha kernels and coronal sources

Flare: motion of H-alpha kernels and coronal sources

Flare: motion of H-alpha kernels and coronal sources. Haisheng Ji Purple Mountain Observatory Nanjing, China. Method to determine the positions of H-alpha kernel (centroid):. But, we need to subtract the background, in order to get the real motion !. T1. T2. Region 1. Region 2. T1.

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308 views • 16 slides
Measuring Proton Energies and Fluxes Using EIT (SOHO) CCDs Areas Outside the Solar Disk Images

Measuring Proton Energies and Fluxes Using EIT (SOHO) CCDs Areas Outside the Solar Disk Images

Measuring Proton Energies and Fluxes Using EIT (SOHO) CCDs Areas Outside the Solar Disk Images. L. Didkovsky 1 , D. Judge 1 , A. Jones 1 , and J. Gurman 2 1 USC Space Sciences Center 2 Goddard Space Flight Center. We Propose.

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229 views • 13 slides
Yang et al. 2004, ApJ, 617, L151

Yang et al. 2004, ApJ, 617, L151

Photospheric shear flows along the magnetic neutral line of Active Region 10486 prior to an X10 flare. Yang et al. 2004, ApJ, 617, L151. ?????? 2005.5.16. Active Region 10486. TRACE white light. X-class flares in Active Region 10486. Day Start Peak Class

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251 views • 10 slides

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