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| 20250531 - Filament data for 06 UTC |
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Available data for 20250531: »05 UTC »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
1 737 1790 (N44E45 L=209) 619 79 1 ( 708/1755- 768/1824) -24.4 E50-E39 N41-N46
2 1663 1506 (N42W44 L=298) 639 131 2 (1602/1465-1719/1536) -4.4 W36-W50 N39-N43
3 418 1484 (N17E52 L=203) 590 133 1 ( 366/1450- 472/1506) 26.6 E55-E47 N13-N18
4 931 1352 (N17E11 L=243) 196 62 2 ( 905/1329- 960/1371) -14.0 E13-E09 N16-N18
5 879 1267 (N11E13 L=242) 1746 299 12 ( 782/1193- 994/1350) 4.1 E19-E05 N06-N16
6 603 1281 (N07E30 L=224) 529 143 0 ( 586/1208- 621/1345) -53.1 E33-E27 N03-N11
7 791 1244 (N08E18 L=237) 311 79 1 ( 762/1206- 815/1277) -36.9 E19-E15 N06-N09
8 1068 1129 (N06W01 L=255) 255 114 2 (1031/1093-1120/1146) 0.0 E01-W04 N03-N07
9 843 1108 (N01E12 L=243) 199 116 0 ( 809/1060- 881/1142) 59.0 E13-E10 S02-N03
10 371 1082 (S08E44 L=211) 406 93 1 ( 324/1063- 422/1103) 20.6 E47-E39 S09-S06
11 842 890 (S12E09 L=246) 1207 379 1 ( 764/ 746- 940/1050) 74.1 E11-E05 S21-N00
12 414 777 (S26E38 L=217) 703 183 1 ( 335/ 744- 471/ 835) 30.3 E45-E32 S28-S21
13 1305 714 (S14W23 L=277) 385 138 0 (1241/ 674-1358/ 748) -12.5 W18-W27 S15-S13
14 1061 662 (S22W09 L=263) 346 106 1 (1014/ 640-1117/ 685) 38.7 W05-W12 S23-S19
15 1307 581 (S22W27 L=281) 320 107 0 (1256/ 564-1358/ 604) 26.6 W23-W29 S24-S20
16 1138 502 (S31W18 L=273) 319 122 1 (1085/ 479-1190/ 546) 51.3 W14-W21 S33-S26
17 384 429 (S53E53 L=201) 1247 93 0 ( 352/ 398- 417/ 467) 28.3 E61-E45 S56-S49
18 469 379 (S56E42 L=212) 845 72 1 ( 439/ 342- 498/ 421) 81.9 E47-E38 S58-S51
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Download FITS filament maps as tar archive
» All Filament Data of 20250531 ...
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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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