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| 20260407 - Filament data for 12 UTC |
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Available data for 20260407: »06 UTC »07 UTC »08 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
1 867 1843 (N39E44 L= 64) 496 94 1 ( 820/1829- 914/1857) 6.3 E48-E39 N37-N40
2 588 1426 (N04E37 L= 71) 357 50 0 ( 557/1407- 621/1443) 33.7 E39-E34 N03-N06
3 1566 1339 (N28W23 L=131) 1434 251 5 (1518/1224-1607/1437) -45.0 W18-W28 N21-N33
4 216 1331 (S08E65 L= 42) 690 65 1 ( 193/1296- 251/1359) 63.4 E68-E61 S10-S06
5 370 1089 (S19E43 L= 65) 1672 401 0 ( 213/1053- 560/1138) 9.2 E59-E28 S22-S14
6 1743 1022 (N16W44 L=152) 536 190 0 (1697/ 944-1778/1103) -28.6 W38-W49 N12-N18
7 1432 961 (N02W24 L=132) 242 47 1 (1404/ 934-1448/ 990) -71.6 W22-W25 N00-N04
8 1833 905 (N13W56 L=164) 448 63 1 (1815/ 873-1851/ 940) 90.0 W54-W58 N10-N14
9 1418 872 (S03W26 L=134) 335 68 1 (1384/ 840-1445/ 904) 0.0 W23-W28 S04-N00
10 1758 848 (N07W51 L=158) 583 62 1 (1731/ 806-1785/ 883) -18.4 W47-W53 N05-N08
11 276 774 (S40E49 L= 58) 328 52 0 ( 250/ 758- 315/ 792) 7.1 E52-E44 S41-S39
12 191 752 (S44E63 L= 44) 454 52 0 ( 169/ 728- 214/ 775) -8.1 E67-E59 S45-S42
13 1628 651 (S08W48 L=156) 683 117 0 (1570/ 624-1677/ 685) 50.2 W45-W50 S10-S04
14 1393 597 (S18W35 L=143) 341 66 0 (1359/ 572-1430/ 615) 68.2 W33-W37 S20-S15
15 458 473 (S57E29 L= 79) 810 104 2 ( 395/ 455- 511/ 497) 10.0 E38-E21 S59-S54
16 612 467 (S52E11 L= 97) 333 57 0 ( 588/ 442- 640/ 497) -21.8 E13-E07 S53-S49
17 1300 437 (S29W38 L=146) 264 22 0 (1285/ 415-1315/ 461) -26.6 W36-W40 S30-S27
18 1403 380 (S29W49 L=157) 410 49 0 (1376/ 356-1427/ 405) -76.0 W46-W51 S30-S26
19 1409 292 (S33W58 L=166) 527 107 1 (1369/ 253-1460/ 327) -81.9 W54-W59 S36-S29
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Download FITS filament maps as tar archive
» All Filament Data of 20260407 ...
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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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