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| 20231228 - Filament data for 08 UTC |
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Available data for 20231228: »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 1053 1766 (N48W06 L=282) 987 115 2 (1007/1729-1110/1818) -48.8 W02-W10 N44-N53
2 1494 1656 (N37W42 L=317) 1828 394 3 (1297/1611-1655/1691) -6.7 W24-W59 N33-N40
3 1279 1520 (N28W19 L=295) 3603 754 0 ( 942/1359-1559/1603) -20.6 E03-W37 N16-N34
4 971 1386 (N20E02 L=273) 400 105 0 ( 931/1342-1019/1424) -56.3 E04-W00 N16-N22
5 1823 1320 (N14W61 L=337) 2156 264 6 (1756/1245-1880/1402) 78.7 W52-W69 N09-N19
6 570 1351 (N19E29 L=247) 433 90 1 ( 536/1325- 611/1384) -26.6 E31-E25 N17-N21
7 1691 1294 (N12W47 L=322) 691 116 1 (1637/1252-1734/1327) -35.5 W42-W50 N09-N14
8 623 1297 (N16E25 L=251) 210 37 0 ( 599/1281- 652/1315) -14.0 E26-E22 N14-N16
9 1545 1254 (N10W34 L=310) 230 84 1 (1533/1215-1561/1300) 78.7 W33-W35 N07-N12
10 1444 1257 (N10W27 L=303) 242 76 0 (1407/1238-1476/1278) 11.3 W24-W29 N09-N11
11 727 1162 (N07E18 L=258) 456 115 1 ( 673/1124- 769/1213) -50.2 E21-E15 N04-N10
12 1743 897 (S12W49 L=325) 2189 323 2 (1668/ 763-1818/1052) 64.8 W43-W56 S19-S02
13 644 965 (S05E24 L=252) 222 46 0 ( 631/ 935- 657/ 994) 76.0 E24-E22 S06-S02
14 1109 854 (S13W05 L=280) 230 48 0 (1089/ 824-1127/ 886) 56.3 W03-W05 S14-S11
15 1385 768 (S19W22 L=298) 746 246 1 (1349/ 658-1442/ 868) 71.6 W20-W25 S26-S13
16 1751 651 (S27W56 L=331) 4170 620 4 (1546/ 482-1908/ 839) 39.2 W40-W75 S38-S15
17 290 655 (S21E58 L=218) 1027 174 3 ( 263/ 569- 335/ 720) 36.9 E66-E51 S26-S17
18 1007 488 (S36E04 L=272) 1006 371 0 ( 900/ 405-1113/ 640) 43.2 E12-W04 S42-S26
19 1291 462 (S39W18 L=294) 428 101 1 (1260/ 436-1343/ 501) -29.7 W15-W23 S41-S36
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Download FITS filament maps as tar archive
» All Filament Data of 20231228 ...
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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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