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| 20250922 - Filament data for 06 UTC |
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Available data for 20250922: »06 UTC »07 UTC »08 UTC »09 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 1624 1619 (N21W63 L=250) 659 71 2 (1586/1594-1660/1639) -5.2 W57-W68 N19-N22
2 1580 1526 (N18W52 L=239) 483 126 0 (1519/1504-1634/1543) -32.0 W47-W55 N15-N20
3 1641 1451 (N13W53 L=240) 372 38 0 (1623/1427-1662/1474) -71.6 W50-W54 N11-N14
4 1697 1371 (N07W53 L=240) 332 53 1 (1666/1352-1721/1390) -45.0 W50-W55 N05-N08
5 936 1348 (N27W04 L=191) 685 224 1 ( 839/1319-1050/1371) -28.6 E02-W10 N23-N30
6 517 1188 (N28E28 L=159) 278 58 2 ( 485/1167- 552/1203) -11.3 E30-E25 N27-N29
7 1204 1169 (N10W14 L=201) 217 37 1 (1176/1151-1228/1192) 0.0 W12-W15 N09-N11
8 1530 1151 (N00W33 L=220) 310 83 0 (1507/1107-1545/1185) 71.6 W31-W33 S01-N02
9 944 1147 (N16E01 L=186) 188 87 1 ( 910/1123- 984/1173) -68.2 E02-W00 N13-N18
10 1847 1061 (S15W56 L=243) 1053 126 3 (1813/1010-1882/1115) 50.2 W52-W60 S17-S11
11 197 894 (N17E63 L=125) 1582 270 3 ( 142/ 791- 289/ 991) -42.9 E69-E54 N09-N22
12 1786 838 (S26W46 L=233) 654 153 0 (1758/ 775-1805/ 915) -74.7 W44-W48 S30-S19
13 1482 864 (S14W22 L=210) 274 81 2 (1434/ 837-1511/ 888) -31.0 W19-W24 S15-S12
14 1505 748 (S22W22 L=209) 436 142 0 (1457/ 703-1541/ 818) 26.6 W17-W25 S23-S18
15 402 505 (S09E56 L=131) 6636 693 16 ( 171/ 312- 586/ 752) -67.0 E74-E48 S25-N08
16 904 413 (S26E25 L=162) 2126 353 2 ( 859/ 264- 957/ 578) 43.5 E36-E16 S35-S16
17 1108 441 (S30E11 L=176) 841 279 0 (1054/ 315-1185/ 539) 35.2 E20-E03 S37-S24
18 1682 487 (S48W36 L=223) 1026 77 2 (1635/ 469-1726/ 513) -17.1 W30-W43 S50-S44
19 614 335 (S25E49 L=138) 477 63 1 ( 588/ 308- 633/ 362) 33.7 E52-E46 S26-S22
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Download FITS filament maps as tar archive
» All Filament Data of 20250922 ...
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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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