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| 20250202 - Filament data for 09 UTC |
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Available data for 20250202: »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
1 483 1521 (N18E44 L=327) 547 125 2 ( 425/1497- 547/1538) 11.3 E48-E38 N15-N18
2 829 1475 (N18E18 L=352) 510 131 1 ( 773/1441- 873/1501) 0.0 E21-E15 N16-N19
3 860 1385 (N13E15 L=356) 1225 285 7 ( 750/1313- 959/1451) 45.0 E20-E09 N07-N18
4 529 1420 (N12E37 L=333) 247 67 1 ( 509/1386- 550/1444) 71.6 E38-E35 N09-N13
5 626 1385 (N10E29 L=341) 380 112 1 ( 587/1335- 653/1417) -38.7 E32-E26 N07-N12
6 794 1036 (S08E14 L=357) 288 112 1 ( 755/ 999- 823/1082) -36.9 E16-E11 S10-S05
7 625 1037 (S10E24 L=346) 326 118 0 ( 593/ 984- 647/1081) 90.0 E25-E22 S13-S07
8 1499 997 (S01W29 L= 39) 199 77 0 (1488/ 955-1512/1040) -78.7 W27-W29 S03-N02
9 150 900 (S22E66 L=304) 1978 203 5 ( 87/ 840- 210/ 970) 16.9 E82-E57 S25-S17
10 559 788 (S26E27 L=343) 1229 330 3 ( 413/ 746- 711/ 841) 10.3 E38-E16 S28-S21
11 1304 691 (S21W23 L= 33) 1065 414 1 (1186/ 569-1469/ 814) 57.7 W18-W30 S30-S11
12 993 771 (S21W02 L= 12) 676 298 1 ( 859/ 747-1130/ 794) 21.8 E06-W09 S24-S17
13 1537 635 (S21W40 L= 50) 680 144 1 (1509/ 571-1558/ 715) -66.0 W37-W42 S24-S15
14 1734 591 (S19W59 L= 70) 379 68 2 (1704/ 568-1761/ 619) 53.1 W56-W61 S20-S16
15 974 559 (S35W04 L= 14) 848 228 0 ( 858/ 539-1087/ 581) 7.1 E04-W12 S36-S33
16 1657 528 (S24W55 L= 66) 308 42 1 (1631/ 509-1683/ 544) 0.0 W52-W58 S25-S23
17 1399 294 (S45W50 L= 60) 1915 227 5 (1298/ 249-1481/ 344) 12.5 W37-W61 S47-S40
18 956 283 (S56W11 L= 21) 305 73 1 ( 926/ 263- 995/ 307) -12.5 W06-W15 S56-S53
19 1545 261 (S43W72 L= 82) 915 70 1 (1532/ 222-1562/ 302) -14.7 W64-W85 S44-S39
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Download FITS filament maps as tar archive
» All Filament Data of 20250202 ...
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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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