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| 20251028 - Filament data for 12 UTC |
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Available data for 20251028: »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC »13 UTC »14 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 1495 1715 (N30W58 L=127) 1566 242 2 (1417/1620-1555/1789) 61.7 W52-W63 N23-N36
2 673 1754 (N62E03 L= 66) 547 75 0 ( 645/1712- 694/1781) -90.0 E06-W00 N57-N65
3 379 1641 (N62E49 L= 20) 813 72 1 ( 339/1615- 418/1665) 3.6 E61-E41 N60-N64
4 1586 1618 (N22W57 L=126) 375 36 1 (1560/1599-1610/1634) -11.3 W55-W60 N20-N22
5 1303 1515 (N24W31 L=100) 321 79 0 (1259/1499-1345/1528) -21.8 W28-W33 N22-N25
6 1098 1425 (N25W15 L= 84) 1127 227 3 ( 986/1383-1212/1447) -24.8 W09-W22 N21-N28
7 1375 1193 (N05W24 L= 93) 269 89 0 (1334/1173-1420/1220) -45.0 W21-W26 N03-N07
8 1631 1127 (S05W38 L=107) 339 78 1 (1612/1088-1650/1170) 45.0 W36-W40 S07-S03
9 1866 1036 (S18W58 L=127) 712 114 2 (1844/ 986-1904/1099) 29.1 W54-W64 S20-S15
10 686 1046 (N14E19 L= 50) 293 86 0 ( 640/1025- 724/1073) 0.0 E21-E15 N12-N14
11 941 982 (N04E06 L= 63) 255 25 0 ( 917/ 961- 963/1005) 14.0 E07-E03 N03-N05
12 722 735 (S04E24 L= 45) 1165 339 1 ( 574/ 647- 825/ 847) 14.0 E35-E15 S06-N00
13 240 715 (N04E61 L= 8) 710 121 2 ( 194/ 681- 299/ 756) -33.7 E65-E56 N01-N07
14 372 497 (S11E59 L= 10) 629 126 1 ( 351/ 442- 395/ 548) 36.9 E63-E54 S13-S07
15 1509 481 (S42W18 L= 87) 1099 255 2 (1403/ 401-1605/ 548) 11.3 W07-W27 S44-S38
16 456 452 (S15E54 L= 15) 321 58 0 ( 439/ 426- 478/ 487) 63.4 E55-E52 S16-S12
17 422 400 (S18E61 L= 8) 555 46 1 ( 393/ 380- 448/ 425) -21.8 E64-E58 S18-S15
18 1256 339 (S44E06 L= 63) 363 90 0 (1211/ 322-1308/ 354) -15.9 E08-E01 S45-S41
19 1020 251 (S43E27 L= 42) 670 127 1 ( 956/ 234-1083/ 275) -11.3 E31-E21 S44-S40
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Download FITS filament maps as tar archive
» All Filament Data of 20251028 ...
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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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