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| 20250118 - Filament data for 11 UTC |
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Available data for 20250118: »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
1 938 1542 (N26E10 L=197) 765 252 0 ( 838/1469-1028/1594) -17.1 E16-E03 N22-N29
2 281 1373 (N13E55 L=151) 3358 368 6 ( 210/1235- 374/1541) -46.5 E67-E44 N04-N24
3 526 1437 (N17E36 L=171) 747 211 0 ( 454/1362- 581/1518) 63.4 E39-E33 N12-N22
4 450 1420 (N16E41 L=165) 453 51 2 ( 421/1388- 484/1448) -9.5 E44-E38 N14-N17
5 364 1409 (N15E48 L=158) 696 86 3 ( 329/1375- 396/1447) 63.4 E51-E45 N13-N17
6 1421 1283 (N14W23 L=229) 706 278 1 (1278/1257-1522/1309) 14.0 W13-W29 N10-N16
7 220 1092 (S04E56 L=150) 479 89 2 ( 191/1060- 262/1124) 38.7 E59-E52 S06-S02
8 613 1042 (S06E25 L=181) 296 99 1 ( 586/1004- 633/1083) -59.0 E27-E23 S08-S03
9 197 974 (S11E59 L=148) 857 199 1 ( 168/ 896- 260/1058) 45.0 E62-E52 S15-S06
10 529 975 (S10E31 L=176) 260 54 1 ( 509/ 948- 556/ 998) 71.6 E31-E28 S12-S09
11 383 893 (S16E42 L=165) 1574 307 2 ( 311/ 808- 455/ 948) -41.2 E47-E35 S20-S12
12 606 918 (S13E25 L=181) 217 38 0 ( 585/ 896- 624/ 947) 56.3 E26-E24 S14-S11
13 196 854 (S18E61 L=146) 2001 194 3 ( 144/ 787- 269/ 911) 29.7 E68-E52 S22-S14
14 529 837 (S19E31 L=176) 376 104 1 ( 495/ 804- 582/ 874) -33.7 E33-E26 S20-S16
15 293 804 (S21E51 L=156) 311 67 1 ( 262/ 774- 318/ 838) 26.6 E54-E47 S23-S19
16 209 677 (S29E65 L=141) 667 57 2 ( 189/ 639- 228/ 713) 51.3 E68-E62 S31-S26
17 1331 512 (S34W27 L=233) 465 122 1 (1267/ 488-1385/ 537) -5.7 W21-W31 S34-S32
18 953 449 (S42E00 L=206) 327 105 1 ( 900/ 433-1009/ 463) 23.2 E04-W03 S42-S39
19 1411 241 (S52W53 L=259) 1392 196 2 (1327/ 221-1505/ 265) 2.0 W41-W69 S54-S49
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Download FITS filament maps as tar archive
» All Filament Data of 20250118 ...
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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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