February 2001 1 - Interesting chains; 2 - Interesting chains; 09 UT: NW eruption and CME 19-24 UT: NE eruptions and CMEs (HALO and partial HALO), II/IV CORONAL MASS EJECTION DYNAMICS REGARDING RADIAL AND EXPANSION SPEEDS Nivaor R. Rigozo1, Alisson Dal Lago2 and D. J. R. Nordeman 2011 ApJ 738 107, File 3- !!Interesting/outstanding chains; CH 4- !!Interesting/outstanding chains; CH. 5- !!Interesting/outstanding chains; CH. NOBE 15 UT: NE eruptions, type II, CME; Yohkoh flaring structure in the center of the disk!! 23 UT: one more NE eruption and CME. 6- Interesting chains 7 - Very low activity; backside HALO 8 - Very low activity 9 - Interesting chains ++10 - !!Interesting chains!! NOBE: a chain aroung the growing AR; bright SW CME !!NOBE, 05 UT; a spectacular NW eruption of a compact, but clear filament; NW CME, large-scale disturbance !!Yohkoh, <10 UT: sharp dimming associated with filament eruption mentioned above ILLUSTRATION !!Suitable for SSRT and NOBE analysis!! +11 - !!Interesting/outstanding chains!! !!01 UT: C6 W flare, type II !!04 UT: N/center eruption with outstanding chains!! !!07 UT: SE CME 12 - Interesting chains; 20 UT; type II +13 - Interesting/outstanding chains at 171 A NOBE: global filaments +14 - Interesting/outstanding chains at 171 A NOBE: global filaments +15 - Outstanding NE filament eruptoions at 13 UT, димминги, распространяющееся возмущение на диске и над лимбом; Events 19 UT - поглощение на 304 А после замедленной эрупции южного волокна; Events Outstanding chains; halo CME; See Moves in Events ILLUSTRATION 16 - Interesting chains 17, 18, 19, 20 - No EIT data 20 - NOBE: interesting chains 21 - Interesting/outstanding EIT chains NOBE: interesting chains 22 - Interesting EIT chains NOBE: interesting chains +23 - Interesting chains; CH !!!NOBE: interesting chains and two propgating fronts 23 UT: large E CME and C2 LDE !! 24 - Interesting chains +25 - Interesting chains at E1 crossing a filament and CH Clear over-the-limb element !! 26 - Interesting chains; W/NW concave CME at 05 UT; ~19 UT: SW filamend eruption (below a CH) and CME 27 - Interesting chains; CH NOBE: global filaments +28 - ~13 UT: a spectacular central filament eruption and halo CME !! ILLUSTRATION NEW EVIDENCE FOR THE ROLE OF EMERGING FLUX IN A SOLAR FILAMENT’S SLOW RISE PRECEDING ITS CME-PRODUCING FAST ERUPTION Alphonse C. Sterling, Louise K. Harra, and Ronald L. Moore The Astrophysical Journal, 669:1359Y1371, 2007, File Multi wavelength investigation of the eruption of a sigmoidal quiescent filament? Ch. Marque, P. Lantos1, and J. P. Delaboudini_ere A&A 387, 317{325 (2002), File