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| 20251025 - Filament data for 11 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 1410 1782 (N36W59 L=168) 435 71 0 (1385/1755-1448/1800) -7.1 W54-W63 N34-N37
2 1035 1720 (N45W26 L=135) 261 11 0 (1020/1696-1051/1743) 53.1 W24-W27 N43-N47
3 394 1612 (N60E43 L= 66) 641 110 0 ( 358/1565- 439/1644) 24.0 E48-E35 N56-N61
4 1064 1390 (N24W12 L=121) 300 51 0 (1037/1367-1098/1409) -14.0 W10-W14 N23-N25
5 1849 1341 (S01W67 L=176) 1067 86 1 (1801/1312-1896/1361) -7.1 W59-W75 S03-N00
6 1310 1165 (N05W19 L=128) 185 89 0 (1264/1143-1344/1192) 0.0 W16-W22 N04-N06
7 546 1130 (N22E26 L= 83) 1275 238 3 ( 427/1097- 678/1158) -19.4 E34-E17 N19-N26
8 1085 1136 (N10W06 L=115) 185 102 0 (1040/1126-1141/1149) -18.4 W03-W09 N08-N10
9 821 912 (N04E14 L= 95) 251 106 0 ( 765/ 891- 853/ 946) 0.0 E17-E11 N02-N05
10 1461 835 (S17W20 L=129) 640 316 0 (1368/ 743-1576/ 943) 15.5 W12-W30 S19-S13
11 1595 880 (S18W30 L=139) 362 111 1 (1551/ 835-1629/ 927) 33.7 W26-W33 S19-S15
12 1167 884 (S06W04 L=113) 204 90 0 (1121/ 865-1212/ 897) -38.7 W01-W06 S08-S04
13 217 808 (N11E61 L= 48) 2342 372 5 ( 97/ 699- 348/ 895) -26.6 E78-E50 N02-N17
14 382 820 (N08E45 L= 64) 905 270 4 ( 335/ 736- 421/ 893) -90.0 E47-E42 N03-N12
15 1735 708 (S33W40 L=149) 1776 351 2 (1670/ 620-1827/ 848) 32.0 W33-W50 S38-S27
16 1505 687 (S27W20 L=129) 270 73 0 (1484/ 653-1528/ 723) 36.9 W18-W22 S28-S25
17 645 640 (S07E32 L= 77) 428 136 0 ( 605/ 590- 695/ 685) 26.6 E35-E27 S09-S05
18 293 588 (S03E62 L= 47) 1439 189 2 ( 231/ 522- 349/ 672) 14.6 E76-E53 S06-N00
19 949 217 (S43E35 L= 74) 1293 306 3 ( 813/ 172-1076/ 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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