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3 Hα 1 km 50arcsec ( ) ( 1) Hα Fe(XII) X Hα Fe(XII) X 1 (6563 ) 150 (195 ) 200 Hα Hα 1 2
4 1.2 Hα ( 2, 2004) km km Hα (Bommier et al.,1994) ( Martin,1998) (eruption) km/s 2 Hα SMART 3
5 N S N S N S (Babcock and Babcock,1955,Howard,1959) N S 4 3 Hα 4 Hα (Leroy,1989) 3 SOHO MDI 4
6 4 Hα ( SMART) (SOHO/MDI) Kippenhahn-Schluter (Kippenhahn and Schluter,1957) Kuperus- Raadu(Kuperus and Raadu,1973) Kippenhahn-Schluter ( 5 ) Kuperus-Raadu ( 5 ) Leroy(1989) Kuperus-Raadu Kippenhahn-Schluter 5 Kippenhahn-Schluter Kuperus-Raadu 5
7 ( Hirayama,1971) ( ) 1.5 Hα (Martin,1998) (Martin et al.,1985) Rust and Kumar Rust Kumar S N 6
8 6 Rust and Kumar van Ballegooijen and Martens van Ballegooijen and Martens (1989) 6(a) ( B C) 6(b) A-D (c) E-F G-H E-F G-H A-D E-H E-H 1.5 ( 6(c) E-F G-H) ( 6(a) A-B C-D) 7
9 7 van Ballegooijen and Martens Martens and Zwaan Martens Zwaan 2001 van Ballegooijen and Martens 8 (p2) (f1) 8 van Ballegooijen and Martens (Welsch et al.,2005) Head-to-tail linkage 8 Martens and Zwaan 8
10 1.7 Wood et al/(2003) Hα Schmieder et al/(2006) Head-to-tail linkage 1.8 Hα 3 9
11 H α Hα SMART SMART Hα SMART Hα SMART SOHO MDI(Michelson Doppler Imager) MDI MDI Zeeman 20 MDI arcsec( 7000km) SMART SMART Hα 50arcsec 3. SOHO MDI
12 Hα [-200,200] : (UT)
13 (Martin,1998) Zeeman 39 van Ballegooijen and Martens Rust and Kumar Head-to-tail linkage
14 van Ballegooijen and Martens Head-to-tail linkage Hα 1 Hα Hα Rust and Kumar van Ballegooijen and Martens Head-to-tail linkage Head-to-tail linkage Welsch et al.(2005) 4.3 MDI 11 van Ballegooijen and Martens Head-to-tail linkage Rust and Kumar 13
15 Hα 1 Hα
16 6 Horace W. Babcock amd Harold D. Babcock, 1954, The sun s magnetic field, The Astrophysical Journal, 121, 349 Veronique Bommier, Egidio Landi Degl innocenti, Jean-Louis Leroy, and Sylvie Sahal-Brechot, 1994, Complete determination of the magnetic field vecor and of the electron density in 14 prominences from linear polarization measurements in the HeI D 3 lines and H α line, Solar Physics, 154, 231 Tadashi Hirayama, 1971, The abundance of helium in prominences and in the chromosphere, Solar Physics, 19, 384 Robert Howard, 1959, Observations of solar magnetic field, The Astrophysical Journal, 130, 193 R. Kippenhahn and A. Schluter, 1957, Eine theorie der sdaren filamente, Zeitschrift für Astrophysik, 43, 36 M. Kuperus and M. A. Raadu, 1973, The support of prominence formed in neutral sheets, Astronomy and Astrophysics, 31, 189 J. L. Leroy,1989, Observation of prominence magnetic fields, proceedings of the workshop, Palma de Mqllorca, Spain, Nov Petrus C. Martens, and Cornelis Zwaan, 2001, Origin and evolution of filament-prominence systems, The Astrophysical Journal, 558, 872 S. F. Martin, S. H. B. Livi and J. Wang, 1985, The cancellation of magnetic flux. II in a decaying active region, Australian Journal of Physics, 38, 929 Sara F. Martin, 1998, Conditions for the formation and maintenance of filaments, Solar Physics, 182, 107 D. M. Rust, and A. Kumar, 1994, Helical magnetic fields in filaments, Solar Physics, 155, 69 B. Schmieder, G. Aulanler, and P. Mein, 2006, Evolving photoshperic flux concentrations and filament dymanic charges, Solar Physics, 238, 245 A. A. van Ballegooijen, and P. C. H. Martens, 1989, Formation and eruption of solar prominences, The Astrophysical Journal, 343, 971 B. T. Welsch, C. R. DeVore, and S. K. Antiochos, 2005, Magnetic reconnection models of prominence formation, The Astrophysical Journal, 634, 1395 Paul Wood, and Piet Martens, 2003, Measurements of flux cancellation during filament formation, Solar Physics, 218,
- 3 Solar-B -
- 3 Solar-B - continuum - - - ( 3 ) Solar-B - ( ) ( ) (SoHO/MDI) Pore Penumbra (umbra) (= ) ( ) - - - 0.5km/s 3 (Advanced Stokes Polarimeter:ASP) (Lites al. 1998 ) - (pore ) - penumbra - SOT/EIS/XRT -
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SOHO - 1 - 20 2 0.4% 2025 18 3.5% 2530 88 17.2% 3035 169 32.9% 3540 132 25.7% 4045 62 12.1% 4550 22 4.3% 5055 14 2.7% 5560 3 0.6% 60 3 0.6% 513 100.0% - 2 - - 3 - - 4 - - 5 - - 6 - - 7 - - 8 - - 9 - -
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