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| 20260619 - Filament data for 09 UTC |
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Available data for 20260619: »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 1420 1633 (N46W27 L=251) 697 108 2 (1383/1572-1445/1671) 63.4 W23-W30 N41-N49
2 1046 1389 (N24E02 L=222) 638 215 0 (1008/1298-1100/1478) -57.5 E05-W02 N18-N29
3 1757 1444 (N35W59 L=283) 1501 162 1 (1679/1421-1831/1477) 0.0 W47-W70 N32-N37
4 412 1418 (N19E48 L=176) 718 202 0 ( 350/1374- 505/1469) -13.2 E56-E39 N17-N21
5 796 1391 (N22E19 L=205) 246 88 0 ( 773/1340- 812/1427) -59.0 E21-E17 N18-N23
6 340 1341 (N14E52 L=172) 516 113 0 ( 326/1292- 355/1402) -66.8 E54-E49 N10-N17
7 1751 1101 (N13W50 L=274) 640 113 0 (1730/1042-1771/1162) -76.0 W48-W52 N08-N16
8 1016 1060 (N04E01 L=223) 568 193 1 ( 924/1017-1085/1087) -6.3 E06-W03 N01-N05
9 1838 1009 (N07W60 L=284) 768 131 0 (1819/ 953-1862/1062) 80.5 W57-W62 N04-N10
10 712 973 (S05E19 L=205) 611 133 0 ( 664/ 925- 757/1020) -33.7 E22-E15 S07-S02
11 1091 952 (S02W05 L=229) 211 74 0 (1072/ 923-1116/ 996) -71.6 W03-W06 S03-N00
12 476 912 (S11E34 L=190) 551 132 0 ( 412/ 894- 551/ 931) 11.3 E39-E29 S12-S08
13 682 708 (S21E19 L=205) 244 67 0 ( 667/ 673- 707/ 739) 76.0 E20-E17 S23-S19
14 1612 639 (S17W45 L=269) 1007 187 0 (1561/ 567-1665/ 713) 68.2 W42-W48 S21-S11
15 1257 646 (S20W19 L=243) 245 71 0 (1242/ 608-1277/ 681) 90.0 W18-W19 S22-S17
16 1236 516 (S28W20 L=244) 461 79 2 (1193/ 495-1272/ 543) 0.0 W17-W23 S29-S26
17 1417 508 (S27W34 L=258) 490 75 1 (1390/ 483-1461/ 537) -9.5 W31-W37 S29-S25
18 790 487 (S35E11 L=213) 420 116 1 ( 746/ 456- 843/ 527) -20.6 E14-E06 S37-S32
19 587 493 (S38E28 L=196) 1393 272 0 ( 483/ 451- 715/ 526) 15.3 E38-E16 S42-S34
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Download FITS filament maps as tar archive
» All Filament Data of 20260619 ...
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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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