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| 20250224 - Filament data for 13 UTC |
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Available data for 20250224: »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 1121 1831 (N48E17 L= 61) 340 41 1 (1093/1811-1149/1849) 53.1 E19-E15 N45-N50
2 498 1660 (N21E53 L= 26) 815 90 4 ( 457/1630- 535/1694) 68.2 E55-E48 N18-N23
3 382 1637 (N18E63 L= 15) 858 92 2 ( 353/1608- 418/1678) 90.0 E66-E56 N16-N21
4 640 1585 (N18E37 L= 41) 370 77 0 ( 615/1551- 676/1616) 78.7 E38-E36 N15-N20
5 1629 1378 (N28W31 L=109) 390 82 0 (1604/1343-1663/1406) 50.2 W29-W34 N25-N31
6 266 1387 (N01E60 L= 18) 974 137 1 ( 196/1366- 333/1405) 3.8 E68-E53 N00-N02
7 1778 1377 (N33W46 L=124) 403 96 0 (1728/1354-1820/1398) 30.3 W40-W52 N29-N36
8 271 1218 (S09E54 L= 24) 351 49 0 ( 249/1188- 297/1241) 45.0 E55-E51 S11-S07
9 1082 1148 (N01W01 L= 79) 212 97 0 (1036/1115-1119/1184) -11.3 E02-W03 N00-N02
10 499 1150 (S10E34 L= 44) 253 65 0 ( 478/1121- 524/1181) 63.4 E35-E33 S11-S07
11 284 1128 (S14E51 L= 27) 464 66 1 ( 267/1087- 303/1163) 90.0 E53-E49 S16-S12
12 239 1065 (S19E55 L= 23) 462 47 0 ( 219/1034- 256/1098) -76.0 E57-E52 S20-S16
13 1513 1072 (N07W27 L=106) 266 81 0 (1472/1056-1555/1092) 0.0 W24-W30 N05-N07
14 735 1014 (S14E17 L= 62) 184 41 0 ( 712/ 995- 757/1034) -18.4 E18-E15 S14-S12
15 271 946 (S25E51 L= 27) 1129 257 1 ( 198/ 839- 367/1032) 39.5 E59-E42 S32-S18
16 1789 999 (N10W50 L=128) 296 49 2 (1774/ 965-1811/1023) -56.3 W47-W51 N08-N11
17 1221 801 (S15W16 L= 95) 1298 638 0 ( 977/ 727-1490/ 885) 25.8 W01-W30 S21-S04
18 1560 666 (S14W42 L=120) 592 145 2 (1477/ 637-1618/ 696) 40.6 W37-W46 S17-S11
19 1292 516 (S29W31 L=109) 294 59 0 (1260/ 497-1327/ 531) 36.9 W28-W32 S30-S27
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Download FITS filament maps as tar archive
» All Filament Data of 20250224 ...
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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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