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| 20240114 - Filament data for 10 UTC |
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Available data for 20240114: »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 465 1636 (N33E49 L= 1) 2566 306 9 ( 395/1485- 529/1724) -29.4 E70-E38 N22-N40
2 923 1682 (N38E12 L= 38) 413 98 1 ( 879/1662- 972/1711) -15.9 E15-E08 N36-N40
3 636 1393 (N16E27 L= 23) 694 180 0 ( 599/1315- 684/1465) 73.3 E29-E24 N11-N21
4 1658 1425 (N25W43 L= 94) 606 95 0 (1609/1387-1698/1456) -23.2 W39-W46 N22-N26
5 1366 1398 (N21W20 L= 70) 269 89 0 (1325/1369-1402/1430) -31.0 W17-W22 N18-N22
6 192 1364 (N15E68 L=343) 1102 145 3 ( 156/1308- 248/1406) -15.3 E80-E58 N10-N17
7 796 1356 (N15E16 L= 34) 410 151 0 ( 732/1315- 852/1380) -14.0 E20-E12 N12-N16
8 746 1265 (N09E18 L= 32) 234 98 0 ( 713/1215- 766/1292) -59.0 E20-E16 N05-N10
9 188 1145 (N01E62 L=349) 2432 323 5 ( 135/1016- 230/1268) 90.0 E71-E56 S06-N08
10 607 1172 (N03E27 L= 24) 283 79 0 ( 586/1137- 636/1209) -53.1 E28-E24 N00-N04
11 1654 1038 (N01W41 L= 91) 280 86 0 (1643/ 990-1665/1087) 90.0 W39-W41 S02-N03
12 313 849 (S17E49 L= 1) 611 146 2 ( 272/ 789- 348/ 907) 45.0 E54-E45 S20-S13
13 539 858 (S16E31 L= 20) 737 261 2 ( 418/ 821- 656/ 884) 6.3 E40-E22 S18-S14
14 1586 812 (S13W38 L= 89) 331 96 4 (1540/ 774-1629/ 839) 0.0 W34-W41 S15-S11
15 1508 744 (S18W34 L= 84) 303 67 0 (1474/ 728-1539/ 766) 26.6 W31-W35 S19-S16
16 1547 695 (S21W38 L= 88) 678 214 1 (1489/ 640-1624/ 755) 45.0 W34-W42 S24-S16
17 1287 705 (S22W19 L= 69) 377 152 0 (1227/ 681-1360/ 740) -11.3 W14-W24 S23-S20
18 1595 481 (S34W50 L=101) 755 105 0 (1557/ 455-1628/ 525) -5.7 W45-W55 S35-S30
19 1225 420 (S42W20 L= 71) 309 66 1 (1201/ 402-1263/ 447) 11.3 W18-W23 S43-S39
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Download FITS filament maps as tar archive
» All Filament Data of 20240114 ...
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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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