Multi-Wavelength Observations of Coronal Structure and DynamicsThese are the Proceedings of the Yohkoh 10th Anniversary Meeting, a COSPAR Colloquium held in Kona, Hawaii, USA, on January 20-24, 2002. The title of the meeting was Multi-Wavelength Observations of Coronal Structure and Dynamics. In these proceedings the many and varied advances of the dynamics solar atmosphere in the past ten years of observations by Yohkoh have been reviewed. |
Contents
| 27 | |
Section III Education and Public Outreach | 101 |
Section IV Sigmoidality and Helicity | 123 |
Section V Reconnection in Flares | 153 |
Section VI MHD Simulations of Emergence and Eruptions | 179 |
Section VII Fine Structure in Flares | 207 |
Section VIII Preflare Phenomena | 237 |
Section IX Flare Plasma Dynamics | 259 |
Section XI Solar Cycle Studies | 321 |
Section XII High Energy Emission in Flares | 349 |
Section XIII Analysis Tools | 413 |
Section XIV Future Observing | 425 |
List of Acronyms | 433 |
List of Participants | 435 |
| 439 | |
Section X Coronal Mass Ejections | 301 |
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Multi-Wavelength Observations of Coronal Structure and Dynamics P. Martens,D. Cauffman Limited preview - 2002 |
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ABSTRACT acceleration active regions analysis Ap.J appear associated bright brightenings Center CMEs compared Connection coronal density determine DISCUSSION distribution effect ejection electrons emerging emission energy eruption estimated et al evolution Figure filament flux footpoints formed frequency function hard X-ray heating helicity images impulsive increase indicate initial intensity Japan jets limb loops magnetic field magnetic flux magnetic reconnection measure motion Observatory observed obtained occur origin particle peak period phase photospheric Physics plasma polar position present radio range ratio reconnection REFERENCES release Research resolution rotation scale Science seen sheet shown sigmoid simulation soft X-ray solar flares Solar Phys Space spectra spectrum speed structure suggest supported Telescope temperature TRACE tube twisted University values variation velocity wave wind Yohkoh
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Page vii - Institute of Space and Astronautical Science, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 229-8510, Japan ABSTRACT We have developed a novel architecture to process 2-dimensional digital image data with very high speed.