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| 20250403 - Filament data for 11 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 1139 1712 (N38E16 L=283) 939 214 0 (1053/1665-1234/1764) 3.8 E23-E08 N36-N39
2 1329 1618 (N38W01 L=299) 321 77 0 (1296/1595-1371/1634) 0.0 E01-W04 N35-N39
3 589 1531 (N11E41 L=258) 883 195 0 ( 540/1465- 640/1624) -26.6 E48-E34 N07-N15
4 1467 1328 (N23W17 L=316) 280 91 0 (1426/1301-1501/1359) -8.1 W13-W20 N22-N24
5 1718 1216 (N25W38 L=337) 315 97 0 (1673/1193-1760/1231) 14.0 W34-W42 N22-N26
6 1889 1083 (N24W59 L=358) 702 91 0 (1851/1046-1915/1129) -11.3 W53-W63 N22-N25
7 681 1048 (S14E20 L=279) 324 63 3 ( 652/1022- 705/1086) 90.0 E21-E18 S15-S11
8 1762 946 (N11W48 L=347) 547 113 1 (1737/ 900-1779/1002) 90.0 W45-W50 N08-N14
9 1822 870 (N10W56 L=355) 2262 280 5 (1757/ 759-1882/ 977) 82.4 W52-W62 N02-N17
10 1040 905 (S12W04 L=303) 379 133 0 ( 993/ 856-1081/ 966) -23.2 W00-W07 S14-S10
11 947 820 (S20W01 L=300) 432 144 1 ( 887/ 793-1014/ 843) 15.9 E02-W05 S21-S17
12 799 719 (S29E05 L=294) 359 123 0 ( 768/ 670- 854/ 745) 56.3 E06-E01 S32-S26
13 213 689 (S47E62 L=236) 621 66 1 ( 172/ 672- 248/ 710) 6.0 E74-E55 S48-S45
14 1444 614 (S16W37 L=336) 313 80 0 (1409/ 600-1489/ 636) 31.0 W35-W40 S17-S14
15 537 546 (S48E21 L=278) 762 186 1 ( 455/ 512- 618/ 583) 6.7 E29-E12 S50-S46
16 859 459 (S44W09 L=307) 290 58 0 ( 838/ 435- 892/ 487) -11.3 W06-W11 S44-S41
17 1444 346 (S30W55 L=353) 455 75 1 (1406/ 316-1475/ 380) -5.2 W49-W60 S30-S28
18 1581 327 (S26W70 L= 9) 614 49 2 (1555/ 305-1604/ 346) 0.0 W64-W75 S27-S24
19 1024 170 (S58W48 L=347) 500 56 0 (1007/ 137-1046/ 200) -10.6 W41-W57 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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