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| 20250129 - Latest Filament data |
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Available data for 20250129: »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
1 981 1633 (N32E11 L= 49) 328 64 0 ( 943/1609-1017/1653) -18.4 E14-E08 N30-N32
2 289 1474 (N15E60 L= 0) 5308 323 16 ( 210/1329- 406/1568) 53.7 E74-E51 N05-N21
3 399 1493 (N16E49 L= 11) 1035 98 5 ( 356/1436- 447/1554) 82.9 E52-E46 N12-N20
4 188 1406 (N10E70 L=350) 1087 110 3 ( 160/1358- 213/1450) 68.2 E74-E66 N07-N13
5 439 1229 (N00E39 L= 21) 267 95 1 ( 400/1197- 479/1243) -9.5 E42-E36 S01-N01
6 1862 1122 (N13W58 L=118) 1545 231 2 (1814/1008-1892/1207) -55.0 W52-W61 N06-N16
7 687 1109 (S05E21 L= 39) 405 151 0 ( 670/1041- 704/1186) 90.0 E22-E19 S08-N00
8 1715 1116 (N09W43 L=104) 526 123 2 (1687/1058-1739/1169) 74.1 W41-W45 N05-N12
9 162 1070 (S10E64 L=357) 2016 176 7 ( 110/1003- 218/1149) 60.9 E71-E56 S14-S05
10 423 990 (S14E38 L= 22) 243 58 2 ( 397/ 960- 444/1013) -56.3 E40-E36 S15-S12
11 258 962 (S16E53 L= 8) 338 44 2 ( 236/ 941- 279/ 984) 26.6 E54-E50 S17-S14
12 774 926 (S14E14 L= 46) 264 115 0 ( 735/ 877- 800/ 972) -45.0 E16-E11 S16-S11
13 1409 897 (S08W25 L= 85) 371 168 0 (1374/ 821-1433/ 971) 84.3 W23-W25 S13-S03
14 214 872 (S22E58 L= 2) 2141 366 5 ( 89/ 815- 393/ 907) 7.9 E83-E40 S24-S18
15 438 730 (S29E38 L= 23) 2004 413 5 ( 289/ 619- 554/ 879) 33.7 E55-E28 S37-S19
16 1895 802 (S05W68 L=129) 1103 148 3 (1870/ 746-1918/ 860) -60.3 W64-W73 S08-S01
17 1346 705 (S20W24 L= 85) 562 220 0 (1270/ 666-1428/ 767) -5.2 W18-W29 S22-S17
18 997 439 (S42W07 L= 67) 2498 482 7 ( 772/ 401-1201/ 484) 12.0 E11-W23 S45-S37
19 1441 422 (S36W42 L=102) 418 101 1 (1396/ 401-1490/ 445) -5.7 W37-W47 S37-S34
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Download FITS filament maps as tar archive
» All Filament Data of 20250129 ...
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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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