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| 20250830 - Filament data for 06 UTC |
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Available data for 20250830: »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 1284 1685 (N40W40 L=171) 284 66 0 (1248/1672-1317/1700) -8.1 W36-W43 N38-N41
2 1638 1652 (N27W69 L=200) 517 62 1 (1612/1631-1672/1669) -26.6 W65-W73 N24-N28
3 859 1557 (N43W02 L=133) 237 32 1 ( 836/1536- 882/1574) -33.7 W00-W03 N41-N44
4 812 1477 (N39E04 L=127) 710 162 1 ( 791/1416- 853/1554) 63.4 E05-W00 N34-N43
5 1046 1533 (N37W15 L=145) 267 76 1 (1014/1505-1086/1554) -11.3 W12-W17 N35-N37
6 827 1200 (N21E08 L=123) 1198 341 1 ( 755/1073- 931/1335) -72.5 E11-E04 N11-N30
7 667 927 (N08E23 L=108) 204 56 0 ( 632/ 912- 690/ 943) 0.0 E25-E21 N07-N09
8 143 901 (N13E71 L= 60) 861 110 2 ( 115/ 859- 171/ 930) -68.2 E77-E66 N10-N15
9 912 836 (S01E10 L=121) 279 93 1 ( 859/ 817- 954/ 854) 0.0 E13-E07 S02-N00
10 1629 737 (S24W33 L=164) 1525 298 2 (1546/ 603-1695/ 847) 42.7 W25-W39 S30-S18
11 490 706 (S02E40 L= 91) 381 65 1 ( 477/ 666- 510/ 748) 76.0 E41-E38 S04-N00
12 1151 669 (S16E00 L=131) 681 109 6 (1114/ 623-1192/ 728) 82.9 E01-W02 S19-S11
13 989 600 (S17E11 L=120) 231 72 0 ( 948/ 589-1021/ 612) -26.6 E13-E09 S18-S16
14 872 537 (S19E20 L=111) 652 241 2 ( 817/ 482- 919/ 607) -83.7 E22-E16 S22-S13
15 1662 549 (S39W37 L=167) 616 115 2 (1610/ 512-1703/ 589) 12.5 W31-W41 S40-S36
16 1041 505 (S24E11 L=120) 285 96 0 (1009/ 468-1065/ 548) 45.0 E13-E08 S26-S21
17 946 313 (S36E24 L=107) 5334 753 10 ( 668/ 167-1225/ 508) 13.0 E65-W00 S44-S28
18 388 432 (S18E63 L= 68) 473 55 0 ( 364/ 411- 415/ 452) 11.3 E67-E57 S19-S16
19 1579 357 (S54W32 L=163) 767 72 1 (1552/ 337-1612/ 385) -32.5 W27-W38 S57-S49
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Download FITS filament maps as tar archive
» All Filament Data of 20250830 ...
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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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