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| 20250403 - Filament data for 09 UTC |
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Available data for 20250403: »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
1 533 1763 (N25E62 L=237) 498 31 1 ( 515/1739- 553/1784) -45.0 E66-E59 N22-N26
2 1087 1738 (N38E20 L=279) 595 121 0 (1040/1705-1140/1768) -5.7 E25-E15 N36-N39
3 1318 1623 (N38E00 L=299) 326 86 0 (1283/1598-1361/1643) 0.0 E02-W03 N35-N39
4 576 1539 (N11E42 L=257) 925 204 1 ( 532/1468- 629/1641) -28.1 E50-E35 N07-N16
5 1455 1334 (N23W16 L=316) 278 91 1 (1416/1302-1486/1367) -11.3 W13-W18 N21-N24
6 1721 1220 (N25W38 L=338) 372 106 0 (1686/1176-1753/1242) -36.9 W35-W41 N23-N26
7 1876 1097 (N24W57 L=356) 491 101 0 (1839/1054-1907/1138) -11.3 W51-W62 N22-N25
8 668 1057 (S14E21 L=278) 371 71 1 ( 642/1024- 695/1093) 90.0 E22-E19 S15-S11
9 1747 945 (N11W47 L=346) 659 128 1 (1722/ 885-1772/1005) -81.9 W44-W48 N07-N14
10 1025 916 (S12W03 L=302) 476 185 1 ( 967/ 845-1083/ 987) -24.0 E01-W08 S14-S09
11 1810 873 (N09W55 L=354) 2114 298 3 (1751/ 766-1873/ 984) 78.7 W50-W60 N02-N17
12 934 829 (S19W00 L=300) 396 132 2 ( 871/ 802- 991/ 854) 0.0 E03-W04 S20-S17
13 809 732 (S28E04 L=295) 469 152 1 ( 757/ 686- 872/ 761) 54.5 E07-W00 S32-S25
14 210 690 (S47E63 L=236) 669 59 1 ( 176/ 670- 245/ 715) 7.1 E72-E56 S48-S45
15 1418 620 (S17W36 L=335) 380 90 0 (1372/ 603-1462/ 639) 31.0 W32-W38 S18-S15
16 529 547 (S49E21 L=278) 912 191 1 ( 449/ 506- 610/ 586) 0.0 E30-E13 S50-S46
17 851 462 (S44W08 L=307) 355 90 1 ( 812/ 436- 893/ 493) 8.1 W04-W11 S45-S41
18 1577 332 (S26W69 L= 8) 489 52 0 (1547/ 310-1601/ 351) 5.2 W63-W74 S26-S24
19 1025 166 (S58W49 L=348) 465 48 0 (1007/ 142-1046/ 199) -17.1 W42-W55 S59-S55
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Download FITS filament maps as tar archive
» All Filament Data of 20250403 ...
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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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