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| 20251109 - Filament data for 08 UTC |
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Available data for 20251109: »06 UTC »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 1245 1812 (N45W46 L=319) 2145 313 4 (1134/1744-1343/1889) 4.9 W31-W67 N41-N47
2 1513 1419 (N14W40 L=313) 1336 243 2 (1412/1357-1630/1492) -50.2 W35-W46 N07-N20
3 307 1465 (N47E50 L=223) 495 60 1 ( 276/1445- 346/1480) -5.7 E54-E43 N45-N48
4 527 1313 (N31E25 L=248) 1557 253 2 ( 413/1287- 656/1341) -20.2 E34-E15 N28-N35
5 1029 1254 (N16W06 L=279) 436 212 0 ( 944/1210-1120/1304) 5.2 W00-W11 N15-N17
6 781 1016 (N08E14 L=259) 1233 453 3 ( 632/ 975- 977/1066) -13.4 E23-E02 N03-N11
7 1462 972 (S09W24 L=297) 585 108 1 (1425/ 915-1498/1032) -76.0 W22-W25 S13-S05
8 438 998 (N14E36 L=237) 256 53 3 ( 409/ 976- 464/1017) 0.0 E38-E34 N12-N15
9 1668 957 (S15W38 L=311) 329 44 0 (1648/ 927-1685/ 982) -76.0 W36-W39 S17-S13
10 265 709 (N01E59 L=214) 742 83 3 ( 236/ 669- 300/ 748) 38.7 E62-E54 S01-N03
11 667 635 (S11E30 L=243) 433 90 2 ( 630/ 596- 693/ 673) 78.7 E32-E28 S13-S08
12 603 638 (S09E34 L=239) 251 62 0 ( 579/ 613- 624/ 664) -90.0 E35-E32 S10-S07
13 1808 554 (S47W58 L=331) 646 45 0 (1774/ 537-1836/ 571) -13.2 W50-W67 S49-S45
14 1352 530 (S33W09 L=282) 456 69 2 (1321/ 506-1389/ 554) 11.3 W06-W11 S35-S31
15 354 503 (S12E60 L=213) 600 95 1 ( 312/ 471- 383/ 540) 18.4 E65-E55 S14-S10
16 574 510 (S16E41 L=232) 253 48 0 ( 560/ 481- 590/ 540) 76.0 E42-E39 S18-S14
17 409 383 (S21E64 L=209) 1631 249 5 ( 337/ 283- 476/ 466) 74.1 E70-E60 S28-S14
18 778 355 (S30E35 L=238) 1268 222 3 ( 677/ 308- 845/ 426) 10.0 E44-E27 S33-S26
19 774 169 (S45E53 L=220) 1634 132 2 ( 719/ 133- 818/ 221) 11.3 E65-E44 S47-S40
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Download FITS filament maps as tar archive
» All Filament Data of 20251109 ...
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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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