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| 20231225 - Filament data for 09 UTC |
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Available data for 20231225: »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 641 1694 (N45E29 L=286) 455 68 1 ( 616/1667- 668/1721) -26.6 E31-E25 N42-N47
2 1063 1617 (N36W06 L=321) 453 175 0 ( 966/1601-1139/1628) 0.0 W00-W12 N34-N36
3 1713 1586 (N31W63 L= 17) 854 134 1 (1653/1541-1767/1621) -24.4 W56-W68 N27-N33
4 709 1471 (N27E19 L=296) 2215 613 2 ( 431/1358- 962/1541) -18.9 E43-E02 N18-N33
5 1539 1467 (N23W38 L=353) 900 208 3 (1451/1421-1623/1525) -32.5 W32-W44 N19-N27
6 1323 1410 (N20W21 L=336) 203 74 0 (1292/1387-1350/1435) -45.0 W19-W22 N18-N21
7 1046 1345 (N17W03 L=318) 454 158 0 (1010/1290-1084/1409) 82.9 W00-W05 N13-N21
8 396 1328 (N20E42 L=273) 389 92 0 ( 377/1289- 425/1373) -45.0 E44-E38 N17-N23
9 670 1302 (N17E21 L=294) 230 87 0 ( 655/1256- 689/1336) -68.2 E22-E19 N13-N18
10 1887 1243 (N08W68 L= 22) 1675 133 2 (1856/1187-1921/1301) 37.9 W62-W74 N04-N11
11 1526 1263 (N10W33 L=348) 324 126 0 (1472/1246-1590/1286) -20.6 W29-W37 N08-N11
12 164 1178 (N13E65 L=250) 2277 233 6 ( 134/1092- 208/1271) -45.0 E72-E58 N07-N18
13 1797 1039 (S04W54 L= 8) 686 85 1 (1774/ 992-1826/1072) 38.7 W51-W56 S06-S02
14 1182 899 (S10W09 L=324) 1086 328 3 (1101/ 770-1278/1038) 53.7 W03-W15 S17-S02
15 803 799 (S15E15 L=300) 317 165 0 ( 754/ 726- 835/ 863) 53.1 E18-E12 S18-S10
16 1257 579 (S31W14 L=328) 758 280 2 (1180/ 496-1325/ 690) 50.2 W08-W18 S36-S23
17 560 575 (S27E36 L=279) 419 138 0 ( 531/ 522- 581/ 643) 48.8 E39-E32 S30-S22
18 824 433 (S39E19 L=295) 727 196 3 ( 763/ 410- 916/ 487) -33.7 E24-E12 S40-S34
19 538 375 (S41E48 L=267) 647 73 0 ( 501/ 357- 577/ 395) -7.1 E52-E43 S41-S39
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Download FITS filament maps as tar archive
» All Filament Data of 20231225 ...
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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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