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| 20250121 - Filament data for 11 UTC |
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Available data for 20250121: »07 UTC »08 UTC »09 UTC »11 UTC »12 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 571 1598 (N27E38 L=129) 701 193 2 ( 509/1567- 652/1644) 4.8 E43-E31 N25-N30
2 304 1479 (N18E57 L=109) 1062 121 6 ( 253/1441- 355/1517) 24.0 E63-E52 N15-N21
3 1571 1429 (N25W34 L=200) 872 169 0 (1509/1367-1624/1485) -36.9 W28-W37 N21-N28
4 1123 1358 (N16W03 L=170) 667 158 4 (1073/1308-1161/1423) 74.1 W00-W05 N12-N19
5 1002 1376 (N16E04 L=163) 223 89 1 ( 958/1349-1044/1401) 31.0 E06-E01 N13-N17
6 1506 1353 (N19W28 L=195) 214 44 2 (1483/1335-1530/1374) 18.4 W26-W29 N18-N20
7 905 1250 (N07E09 L=158) 1082 378 3 ( 768/1100- 977/1369) -45.0 E18-E03 S01-N13
8 1594 1234 (N13W34 L=201) 233 140 0 (1549/1214-1630/1268) -21.8 W31-W37 N11-N15
9 1934 1159 (N14W70 L=236) 675 91 0 (1902/1133-1958/1184) -14.0 W64-W75 N12-N15
10 378 1135 (S03E42 L=124) 490 127 0 ( 329/1098- 438/1160) -12.5 E46-E37 S04-S01
11 671 1003 (S09E21 L=146) 431 147 0 ( 615/ 949- 723/1044) 45.0 E24-E18 S12-S06
12 214 962 (S13E57 L=110) 413 85 2 ( 179/ 923- 240/ 999) -45.0 E61-E54 S15-S10
13 1178 912 (S10W10 L=177) 385 105 2 (1131/ 874-1238/ 946) 33.7 W07-W13 S12-S07
14 168 871 (S18E64 L=103) 455 69 3 ( 144/ 834- 186/ 899) -36.9 E67-E61 S20-S16
15 850 817 (S19E09 L=158) 1133 491 1 ( 645/ 747-1044/ 887) 18.4 E22-W02 S23-S13
16 1101 799 (S18W07 L=173) 727 407 2 ( 944/ 747-1266/ 845) 26.6 E02-W16 S22-S13
17 631 659 (S30E24 L=143) 273 51 0 ( 618/ 626- 646/ 690) -90.0 E24-E22 S32-S28
18 497 623 (S33E35 L=132) 389 67 1 ( 471/ 585- 526/ 655) -53.1 E36-E33 S35-S31
19 1327 494 (S34W28 L=195) 321 72 0 (1284/ 480-1367/ 511) 18.4 W24-W30 S35-S33
20 1316 390 (S42W31 L=198) 837 233 1 (1246/ 356-1429/ 447) -6.3 W23-W41 S44-S38
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Download FITS filament maps as tar archive
» All Filament Data of 20250121 ...
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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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