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| 20231129 - Filament data for 10 UTC |
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Available data for 20231129: »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 1207 1899 (N57W52 L=349) 744 60 1 (1189/1860-1223/1930) 20.2 W44-W63 N52-N59
2 1213 1698 (N40W30 L=326) 1487 216 2 (1105/1665-1319/1732) -17.4 W20-W37 N36-N42
3 1553 1607 (N26W51 L=348) 951 187 1 (1473/1553-1620/1650) -56.3 W46-W56 N21-N30
4 1493 1535 (N23W42 L=339) 685 119 1 (1461/1502-1537/1565) -68.2 W38-W45 N20-N25
5 1022 1468 (N28W08 L=305) 917 265 1 ( 903/1451-1158/1487) -10.6 W00-W16 N24-N30
6 1447 1451 (N19W35 L=332) 272 60 1 (1427/1424-1465/1478) -90.0 W33-W36 N17-N20
7 747 1455 (N32E11 L=286) 445 129 1 ( 683/1435- 809/1472) -18.4 E15-E06 N30-N34
8 1371 1396 (N17W28 L=325) 595 205 0 (1276/1376-1462/1414) -14.0 W22-W34 N14-N18
9 349 1338 (N32E44 L=253) 1235 257 2 ( 240/1291- 446/1388) -14.6 E57-E34 N27-N35
10 587 1370 (N29E23 L=274) 292 99 0 ( 537/1342- 626/1387) -26.6 E26-E20 N26-N30
11 953 1355 (N22W01 L=298) 489 223 0 ( 838/1333-1045/1378) -28.6 E05-W06 N18-N25
12 926 1252 (N16E02 L=295) 861 340 1 ( 800/1174-1075/1328) -45.0 E08-W05 N09-N22
13 1717 1152 (S03W47 L=344) 406 67 0 (1685/1129-1746/1175) -21.8 W44-W49 S05-S02
14 1853 1045 (S12W59 L=356) 696 170 1 (1836/ 967-1864/1136) 73.3 W56-W61 S16-S06
15 749 966 (N02E17 L=280) 210 47 1 ( 720/ 950- 775/ 985) 0.0 E19-E15 N01-N03
16 1203 754 (S18W06 L=303) 232 59 0 (1179/ 726-1234/ 785) 45.0 W04-W08 S19-S16
17 968 724 (S15E09 L=288) 407 155 0 ( 914/ 684-1035/ 775) -54.5 E10-E05 S18-S11
18 1245 749 (S19W09 L=305) 212 45 0 (1222/ 725-1273/ 769) 18.4 W06-W10 S20-S17
19 1035 494 (S31E10 L=287) 1099 228 0 ( 999/ 392-1083/ 614) 57.3 E14-E03 S38-S24
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Download FITS filament maps as tar archive
» All Filament Data of 20231129 ...
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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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