Catania Obs (Moeller) 229 Fritz Egger 188 Hubert Joppich 28 Kanzelhoehe (Moeller) 212 Georg Robeck 168 Frank Ruemmler 65 Bob van Slooten 187 Slovak Central Obs. 32 Friedrich Smit 85 SOHO (Joppich) 0 Hugo Stetter 67 Wolfgang Strickling 20 Andreas Tarnutzer 116 SYNODISCHE SONNENROTATION NR. 2004 ROTATIONSBEGINN: 2003-06-09.35 ROTATIONSENDE: 2003-07-06.55 ES HABEN 12 BEOBACHTER INSGESAMT 1397 MESSUNGEN AN 28 SONNENFLECKENGRUPPEN GEMACHT Def-Nr Lfd-Nr Laenge P Sigma-LP Breite P Sigma-BP Laenge F Sigma-LF Breite F Sigma-BF Beotg P Beotg F Typ 1 1 359.2 1.4 -16.6 0.5 355.2 1.3 -17.4 0.7 24 25 D 4.8 2 3 356.2 1.3 2.5 0.4 348.1 1.3 3.9 0.5 69 54 D 5.9 3 2 355.5 0.8 14.9 0.8 353.2 0.9 15.0 1.0 10 11 C 4.0 4 4 338.6 1.1 15.1 0.7 333.5 1.3 16.1 2.0 20 9 C 3.8 5 5 333.8 0.7 -18.0 0.6 330.4 0.9 -18.5 0.8 53 33 D 5.1 6 6 315.2 1.3 -14.3 0.8 308.5 0.9 -16.7 0.6 54 75 E 6.0 7 7 302.1 1.2 19.8 0.4 299.1 0.4 21.6 1.0 8 5 B 3.8 8 8 273.5 0.5 -22.4 1.0 0.0 0.0 0.0 0.0 5 0 A 3.0 9 9 258.6 0.1 -13.9 0.1 0.0 0.0 0.0 0.0 2 0 A 2.5 10 10 252.1 0.3 -17.6 1.3 249.1 0.4 -18.1 0.7 7 6 B 3.4 11 11 245.2 0.8 27.4 1.2 239.5 0.7 29.2 0.6 38 32 D 5.4 12 12 216.4 1.0 -1.0 0.9 208.9 0.8 -3.7 0.9 35 36 D 5.7 13 13 194.9 1.0 -12.4 0.6 190.9 0.6 -11.8 0.4 4 5 B 4.3 14 14 191.7 0.4 -4.2 1.3 187.8 0.8 -6.6 0.5 36 47 D 6.0 15 15 174.6 0.6 18.5 0.5 165.5 0.8 17.8 0.5 67 63 E 6.5 16 16 167.3 1.0 14.1 0.9 161.4 0.5 13.5 0.6 44 33 D 5.5 17 17 129.0 0.9 -3.8 0.6 123.3 1.1 -4.4 0.6 31 31 E 6.1 18 18 108.2 0.5 9.1 0.8 104.1 0.8 10.3 1.1 42 19 D 5.1 19 19 103.9 0.9 15.1 0.5 0.0 0.0 0.0 0.0 63 0 J 1.9 20 21 87.9 0.7 -15.8 0.5 81.5 0.7 -17.4 0.6 23 9 C 4.1 21 20 84.2 1.0 6.0 0.3 81.4 0.0 6.8 0.0 36 2 C 3.1 22 22 76.7 0.6 -12.3 0.6 74.7 0.5 -11.4 1.3 6 4 B 3.8 23 23 65.2 0.7 10.6 0.4 0.0 0.0 0.0 0.0 39 0 J 2.5 24 24 40.8 1.1 8.6 0.6 28.5 0.9 11.6 0.5 59 56 F 7.5 25 25 31.4 0.4 -7.1 0.2 0.0 0.0 0.0 0.0 2 0 A 3.0 26 26 28.4 1.0 -12.5 0.6 22.5 1.1 -11.4 0.4 5 14 D 5.7 27 27 22.2 1.0 13.5 0.9 20.9 1.0 15.1 0.2 11 11 B 3.3 28 28 9.3 0.8 4.5 0.5 6.2 0.3 3.9 0.2 12 12 C 4.3