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| 20250623 - Filament data for 11 UTC |
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Available data for 20250623: »06 UTC »07 UTC »08 UTC »09 UTC »10 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
1 837 1650 (N42E21 L=286) 3933 650 11 ( 558/1512-1115/1760) -11.7 E56-W02 N33-N47
2 1345 1530 (N37W21 L=328) 1388 253 3 (1226/1503-1466/1555) 3.0 W11-W30 N34-N38
3 1580 1434 (N31W39 L=347) 932 170 2 (1521/1364-1641/1485) -48.8 W34-W43 N26-N34
4 325 1376 (N18E55 L=253) 1140 117 4 ( 268/1339- 376/1420) 21.8 E60-E50 N15-N20
5 572 1369 (N20E33 L=274) 590 93 2 ( 547/1326- 609/1419) -63.4 E35-E30 N17-N23
6 1405 1316 (N22W23 L=331) 326 106 0 (1391/1268-1416/1376) 81.9 W22-W24 N19-N26
7 1318 1309 (N21W17 L=325) 223 76 0 (1295/1277-1345/1346) -45.0 W15-W19 N19-N23
8 1807 1244 (N20W58 L= 6) 715 147 0 (1734/1223-1847/1282) 8.1 W50-W64 N18-N22
9 176 1222 (N07E68 L=239) 655 67 0 ( 153/1204- 213/1250) -5.7 E72-E62 N06-N08
10 526 1108 (N03E32 L=275) 1233 250 1 ( 497/ 994- 568/1220) 90.0 E34-E29 S03-N10
11 1844 1060 (N09W61 L= 8) 456 51 0 (1821/1033-1867/1086) -26.6 W57-W63 N06-N10
12 390 997 (S04E42 L=266) 335 65 1 ( 357/ 977- 431/1013) 18.4 E44-E38 S05-S03
13 1832 926 (N00W60 L= 7) 565 96 0 (1797/ 904-1873/ 963) 14.0 W56-W64 S01-N02
14 220 799 (S18E60 L=247) 469 55 1 ( 206/ 769- 238/ 833) 53.1 E62-E57 S20-S16
15 759 737 (S18E15 L=292) 512 183 1 ( 673/ 706- 836/ 782) -15.3 E20-E09 S19-S15
16 1412 577 (S24W30 L=338) 3118 593 6 (1161/ 472-1656/ 688) 25.9 W14-W47 S32-S15
17 542 659 (S24E31 L=277) 356 86 2 ( 506/ 637- 584/ 687) 29.7 E34-E27 S26-S22
18 358 535 (S35E53 L=255) 387 53 0 ( 324/ 523- 387/ 546) 7.1 E57-E48 S36-S34
19 1040 436 (S36W06 L=313) 462 101 2 ( 993/ 407-1078/ 479) 56.3 W02-W08 S38-S32
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Download FITS filament maps as tar archive
» All Filament Data of 20250623 ...
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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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