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| 20260703 - Filament data for 13 UTC |
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Available data for 20260703: »06 UTC »07 UTC »09 UTC »10 UTC »11 UTC »12 UTC »13 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 656 1292 (N18E25 L= 11) 281 62 0 ( 640/1268- 680/1324) -53.1 E26-E23 N16-N20
2 1763 1239 (N17W54 L= 90) 1151 205 3 (1688/1203-1814/1303) 11.3 W46-W61 N14-N20
3 1012 1238 (N16E01 L= 35) 313 116 0 ( 969/1196-1056/1274) -45.0 E04-W01 N13-N18
4 838 1186 (N12E12 L= 24) 477 166 0 ( 823/1104- 860/1260) 84.3 E13-E11 N07-N17
5 1827 1187 (N14W60 L= 97) 391 84 1 (1798/1158-1847/1219) 31.0 W56-W63 N11-N15
6 1630 1174 (N13W41 L= 77) 306 62 0 (1603/1146-1654/1203) -36.9 W38-W42 N11-N14
7 1292 1117 (N09W16 L= 53) 540 191 0 (1206/1058-1360/1162) -31.0 W10-W20 N05-N11
8 1499 1124 (N10W30 L= 67) 215 63 0 (1487/1086-1512/1160) 78.7 W29-W31 N07-N12
9 252 833 (S12E56 L=340) 1292 224 2 ( 200/ 742- 288/ 947) -71.6 E61-E52 S17-S05
10 1563 883 (S05W35 L= 72) 472 69 1 (1531/ 851-1595/ 913) 45.0 W33-W37 S06-S02
11 1610 834 (S08W40 L= 76) 549 87 2 (1577/ 788-1640/ 879) 90.0 W36-W41 S10-S04
12 1735 795 (S10W51 L= 87) 555 106 1 (1703/ 771-1782/ 823) 8.1 W47-W55 S11-S08
13 1844 761 (S13W65 L=101) 818 114 1 (1820/ 709-1869/ 807) 90.0 W62-W67 S15-S09
14 198 710 (S21E67 L=329) 812 101 0 ( 169/ 679- 241/ 755) -18.4 E71-E61 S22-S17
15 797 670 (S20E14 L= 23) 604 189 0 ( 729/ 604- 846/ 743) 51.3 E18-E10 S24-S14
16 1753 693 (S17W55 L= 92) 468 58 1 (1726/ 666-1771/ 724) 90.0 W52-W58 S18-S14
17 613 519 (S31E29 L= 8) 607 101 1 ( 548/ 495- 666/ 547) 16.7 E34-E24 S32-S28
18 1598 422 (S36W52 L= 88) 1171 140 1 (1540/ 376-1654/ 465) 36.9 W47-W56 S39-S32
19 767 252 (S53E24 L= 13) 602 79 0 ( 727/ 231- 809/ 273) 15.3 E29-E17 S56-S50
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Download FITS filament maps as tar archive
» All Filament Data of 20260703 ...
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The tar archive contains filament maps for all processed Hα images
with at least quality=1.
The maps contain the values 0 and 1, where 1 is the position of a detected filament.
The header in the FITS files is mostly taken from the corresponding Hα file,
so it should be compatible with standard solar software routines.
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