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| 20260404 - Filament data for 10 UTC |
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Available data for 20260404: »07 UTC »08 UTC »09 UTC »10 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 1369 1694 (N46W00 L=148) 311 53 0 (1341/1678-1401/1708) 53.1 E01-W02 N43-N47
2 1013 1624 (N27E20 L=129) 248 48 0 ( 995/1601-1037/1654) -14.0 E21-E17 N25-N29
3 954 1440 (N15E16 L=133) 396 89 0 ( 931/1398- 983/1483) -45.0 E17-E13 N12-N17
4 275 1430 (S02E63 L= 85) 396 35 0 ( 255/1408- 294/1450) -9.5 E66-E60 S02-N00
5 1681 1287 (N29W34 L=182) 460 90 0 (1641/1252-1713/1321) -15.9 W29-W36 N27-N29
6 1403 1239 (N16W15 L=163) 292 95 0 (1391/1189-1416/1290) -63.4 W13-W16 N13-N19
7 426 1216 (S11E41 L=107) 263 76 0 ( 409/1191- 459/1251) -26.6 E43-E38 S12-S09
8 838 1199 (S02E15 L=134) 352 79 1 ( 811/1159- 856/1233) -63.4 E16-E13 S04-N00
9 1681 1050 (N15W38 L=187) 263 20 0 (1665/1027-1698/1077) -56.3 W36-W39 N13-N16
10 1141 1018 (S03W06 L=155) 218 61 1 (1113/ 995-1168/1043) 71.6 W05-W07 S04-S01
11 648 953 (S20E20 L=129) 378 78 0 ( 628/ 900- 671/ 989) -68.2 E21-E17 S23-S18
12 156 869 (S37E66 L= 82) 623 77 0 ( 113/ 851- 191/ 885) 10.0 E77-E60 S38-S35
13 951 697 (S26W06 L=154) 489 164 0 ( 869/ 677-1031/ 713) 21.8 W00-W10 S28-S24
14 1255 594 (S23W27 L=175) 230 122 0 (1197/ 571-1295/ 610) 33.7 W24-W30 S25-S21
15 306 585 (S53E50 L= 98) 463 46 1 ( 277/ 559- 337/ 606) -6.3 E55-E44 S54-S51
16 1443 506 (S21W43 L=191) 318 77 0 (1410/ 475-1468/ 545) -78.7 W41-W44 S23-S18
17 1119 446 (S35W26 L=175) 639 158 2 (1056/ 396-1155/ 516) 82.9 W23-W29 S38-S30
18 1186 376 (S37W35 L=184) 492 82 0 (1153/ 345-1219/ 412) -80.5 W33-W37 S39-S33
19 1319 234 (S40W59 L=207) 704 117 0 (1274/ 194-1356/ 275) -3.6 W50-W67 S41-S38
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Data will be available after one hour of observations. |
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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