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| 20251025 - Filament data for 13 UTC |
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Available data for 20251025: »06 UTC »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 1041 1712 (N45W26 L=134) 324 38 1 (1014/1690-1065/1736) -56.3 W23-W27 N42-N46
2 399 1614 (N60E42 L= 66) 754 102 0 ( 364/1565- 443/1646) 35.5 E48-E35 N56-N62
3 1081 1398 (N24W14 L=122) 366 57 0 (1049/1374-1128/1418) -11.3 W11-W16 N22-N25
4 1855 1344 (S01W68 L=176) 1067 69 1 (1810/1316-1898/1367) -7.6 W61-W76 S02-N00
5 1327 1173 (N05W21 L=129) 186 70 0 (1289/1154-1359/1197) 0.0 W17-W22 N04-N05
6 558 1136 (N22E25 L= 83) 1260 231 3 ( 440/1098- 676/1163) -23.6 E33-E17 N19-N26
7 1104 1144 (N09W07 L=115) 209 86 0 (1061/1132-1153/1158) -18.4 W04-W10 N08-N10
8 1489 858 (S16W23 L=131) 686 357 0 (1385/ 751-1592/ 993) 24.0 W13-W31 S19-S11
9 842 919 (N04E13 L= 95) 247 92 0 ( 794/ 898- 866/ 952) 11.3 E15-E10 N02-N05
10 1610 891 (S18W32 L=140) 435 123 1 (1568/ 847-1634/ 949) 29.7 W27-W34 S19-S15
11 179 864 (N14E64 L= 44) 1662 204 4 ( 101/ 837- 281/ 897) -4.6 E77-E52 N12-N17
12 402 806 (N07E43 L= 65) 719 196 0 ( 376/ 738- 432/ 897) 56.3 E46-E40 N03-N12
13 1741 704 (S34W41 L=149) 2156 340 2 (1650/ 599-1850/ 853) 22.2 W31-W53 S38-S27
14 281 736 (N05E56 L= 52) 826 110 0 ( 239/ 700- 325/ 770) -39.8 E59-E52 N02-N07
15 1482 629 (S30W18 L=126) 637 260 0 (1420/ 514-1541/ 732) 45.0 W11-W23 S36-S25
16 663 651 (S07E30 L= 78) 476 125 1 ( 616/ 604- 715/ 701) 18.4 E34-E25 S09-S05
17 303 596 (S03E60 L= 48) 1658 190 1 ( 234/ 521- 359/ 677) 14.0 E75-E51 S06-N01
18 1355 363 (S45W02 L=110) 312 48 0 (1336/ 336-1374/ 396) -81.9 W01-W03 S48-S41
19 957 218 (S43E34 L= 74) 1411 304 3 ( 817/ 175-1084/ 294) 2.0 E49-E20 S46-S40
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Download FITS filament maps as tar archive
» All Filament Data of 20251025 ...
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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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