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1 - 3 Solar-B -
2 continuum ( 3 ) Solar-B - ( ) ( )
3
4 (SoHO/MDI) Pore Penumbra (umbra) (= )
5 ( ) km/s 3 (Advanced Stokes Polarimeter:ASP) (Lites al ) - (pore ) - penumbra - SOT/EIS/XRT -
6 - ( 90 ) - B 500[Gauss] ( :800Gauss) - filling factor >80% Magnetic flux ASP filling factor 100[%] 0 [degree] B [Gauss] [%] [%] (binsize=5) (binsize=40)
7 Magnetic flux 3 -:90 - -:70 -:50 ( 45 ) -:30 - B [Gauss] -:10 - filling factor 60% 19-Nov-00 17:26-17:56UT [degree] B [Gauss] filling factor [%] [%] [%] [%] (binsize=5) (binsize=40) (binsize=5)
8 Convective collapse? 500Gauss Filling factor >80% :1-1.6 KGauss 45 Filling factor 60% downward region (Bellot Rubio et al. 2001) - Fe I 1.5 m (Tenerife Infrared Polarimeter) - downward velocity < 6 km/s pixel magnetic element
9 Penumbra pore 5 penumbra penumbra <1 pore ASP (Leka & Skumanich 1998) intensity - penumbra (Ic ) Evershed flow (cadence 20 min) - penumbra pore penumbra
10 converging flow (Meyer et al. 1974, Parker 1992) - magnetogram (Strous et al. 1994) - intensity (Sobotka et al. 1999, Roudier 2002) - subsurface (Zhao et al. 2001) Filling factor 80% ( ) diverging flow White light image( : ) Sobotka et al Zhao et al. 2001
11
12 1 - (Meyer et al. 1974) - (Simon & Leighton 1964, Meyer et al. 1974) (Petorvay & Moreno Insertis 1997)
13 Moving Magnetic Features (MMF) (Harvey & Harvey 1973, Brickhouse & Labonte 1998, Zhang et al. 2003) (2-7 ) 2 moat flow( 0.5km/s) moat flow 4 (0.25h 11h) (SoHO/MDI) MMF MMF
14 A(t) da( t) - Linear decay low = const dt - :Parabolic decay low d( A) A( t) dt Bumba (1963) - Greenwich Photoheliographic Results (GPR) Linear decay low Martinez Pillet et al. (1993) - GBR ( ) non-linearity parabolic decay low non-linearity disk Pertrovay and van Driel-Gesztelyi(1997) -Debrecen Photoheliographic Results (DBR) 1977,1978 Parabolic decay low
15 MMF ASP 2 (Martinez Pillet 2002) Mx/day MMF : Mx/day -MMF flux tube 4. 2 ASP continuum 3 8 (Harvey & Harvey ) Filling factor
16 MMF Shine & Title (2001) MMF 3 Type I ( arcsec ) -type (Ryutova et al. 1997, Thomas et al. 2002) U -type (Zhang et al. 2003) Type II ( )? Type III: ( ) (2 3km/s) return back flux tube Evershed flow Thomas et al. (2002)
17 penumbra [arc sec] penumbra (ASP) (ASP)[km/s] º 20 Magnetic flux (ASP) º (North) 45 º [degree] º (East) -56 º 0 º (West) disk center
18 penumbra [arc sec] penumbra (ASP) (ASP)[km/s] penumbra Evershed flow [degree] [degree]
19 penumbra [arc sec] (ASP) (ASP)[km/s] 1.5 [degree] -1.5 (MDI)[km/s] Evershed channels -
20 MMF 20 (ASP) (MDI)[km/s] :v horizontal >0.35km/s :v horizontal <0.35km/s, 90 < <135 :v horizontal <0.35km/s, >135 - ( ) Type III - Type I? - moat Type II - moat
21 MMF Type II, Type III Thomas et al. (2002) - Type III Evershed flow - Type II moat MMF Thomas et al. (2002)
22 Satellite spot moat (Shimizu 1993) (Wang et al. 1991) X (Shimojo et al. 1996) TRACE (171 ) MMF or
23 Solar-B ( ) FG,SP SP 1scan(0.16arcsec/pix) / 4.8sec - 1.2: penumbra - penumbra - Evershed flow penumbra MMF (Wang et al.1992) -MMF 3. inward flow outward flow 4. moat MMF - satellite spot -MMF 5. MMF
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