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| 20230913 - Filament data for 07 UTC |
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Available data for 20230913: »06 UTC »07 UTC »08 UTC »10 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 1350 1498 (N25W35 L=269) 1175 330 2 (1211/1449-1499/1541) -15.3 W23-W46 N21-N27
2 802 1484 (N40E02 L=232) 685 149 2 ( 734/1457- 876/1511) -11.3 E07-W03 N37-N42
3 595 1466 (N44E20 L=214) 243 50 3 ( 575/1439- 613/1490) -63.4 E21-E18 N42-N46
4 1749 1463 (N11W65 L=299) 422 79 2 (1704/1449-1781/1481) -11.3 W59-W69 N09-N12
5 1480 1414 (N17W39 L=273) 312 63 0 (1458/1389-1504/1442) -76.0 W38-W41 N14-N18
6 900 1220 (N21E03 L=231) 805 368 1 ( 751/1130-1036/1281) -45.0 E11-W03 N12-N27
7 378 1107 (N26E42 L=192) 1764 392 4 ( 226/1009- 510/1235) -35.1 E59-E32 N17-N36
8 383 863 (N11E45 L=189) 318 140 0 ( 337/ 833- 447/ 878) 0.0 E49-E39 N09-N12
9 720 752 (S02E24 L=210) 440 138 0 ( 679/ 703- 745/ 818) 29.7 E28-E21 S03-N01
10 1560 748 (S23W26 L=260) 519 199 1 (1484/ 682-1621/ 808) 14.0 W19-W31 S25-S21
11 1404 711 (S21W15 L=249) 757 190 1 (1369/ 619-1430/ 790) 52.1 W10-W18 S25-S15
12 1744 534 (S47W47 L=281) 936 81 1 (1700/ 507-1782/ 555) -23.6 W39-W55 S49-S42
13 1577 413 (S50W26 L=260) 699 70 2 (1546/ 378-1605/ 448) 71.6 W22-W30 S52-S46
14 447 374 (S20E63 L=171) 605 71 1 ( 423/ 350- 477/ 404) 14.0 E69-E57 S22-S18
15 1495 370 (S50W17 L=251) 552 60 2 (1473/ 341-1514/ 404) 59.0 W15-W19 S52-S46
16 1221 333 (S42E07 L=227) 537 65 1 (1190/ 302-1250/ 358) 38.7 E09-E04 S44-S39
17 739 314 (S30E42 L=192) 332 46 1 ( 714/ 296- 764/ 331) -56.3 E43-E39 S31-S28
18 803 255 (S36E42 L=192) 694 106 2 ( 768/ 215- 826/ 294) 20.0 E48-E37 S39-S33
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Download FITS filament maps as tar archive
» All Filament Data of 20230913 ...
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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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