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| 20231226 - Filament data for 08 UTC |
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Available data for 20231226: »07 UTC »08 UTC »09 UTC »10 UTC »11 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 1037 1841 (N56W08 L=310) 377 57 0 (1012/1823-1072/1853) 15.9 W05-W12 N54-N57
2 775 1712 (N45E17 L=285) 495 47 1 ( 749/1687- 810/1734) -18.4 E19-E13 N43-N47
3 1208 1633 (N36W17 L=319) 986 276 1 (1063/1612-1322/1651) -11.9 W06-W25 N34-N38
4 1619 1604 (N33W52 L=354) 514 87 0 (1571/1581-1663/1623) -14.0 W47-W56 N30-N34
5 656 1540 (N32E24 L=278) 884 149 0 ( 575/1520- 731/1561) 0.0 E30-E18 N30-N34
6 1652 1482 (N24W49 L=351) 1003 190 2 (1597/1436-1724/1540) -41.2 W45-W55 N20-N27
7 1019 1458 (N25W02 L=304) 1572 428 5 ( 832/1336-1169/1520) -31.0 E10-W10 N16-N29
8 1588 1353 (N16W39 L=341) 1376 394 4 (1448/1244-1750/1453) -33.7 W30-W51 N08-N22
9 1283 1333 (N15W18 L=320) 917 306 3 (1216/1245-1368/1440) -72.9 W13-W22 N09-N22
10 1813 1324 (N13W60 L= 2) 1099 168 2 (1779/1287-1859/1390) -56.3 W56-W66 N11-N17
11 573 1339 (N19E28 L=274) 219 65 0 ( 547/1314- 600/1371) -45.0 E30-E26 N17-N21
12 250 1310 (N20E57 L=245) 536 62 2 ( 230/1273- 279/1343) -68.2 E59-E53 N17-N22
13 303 1182 (N11E49 L=253) 879 103 2 ( 259/1146- 349/1215) -18.4 E53-E44 N08-N13
14 1377 891 (S12W21 L=323) 1541 390 3 (1302/ 732-1476/1055) 64.7 W16-W28 S21-S02
15 700 830 (S12E21 L=281) 212 78 0 ( 674/ 796- 726/ 859) 45.0 E23-E19 S14-S10
16 973 754 (S18E05 L=297) 321 132 1 ( 952/ 695-1009/ 815) 66.8 E06-E01 S21-S14
17 717 595 (S27E23 L=278) 518 151 1 ( 674/ 540- 757/ 669) 45.0 E27-E19 S30-S22
18 1435 592 (S31W27 L=329) 418 100 1 (1403/ 555-1464/ 640) 80.5 W24-W29 S33-S27
19 1325 507 (S36W20 L=322) 669 148 1 (1254/ 474-1393/ 552) 11.3 W14-W25 S38-S33
20 985 443 (S39E06 L=295) 706 167 4 ( 920/ 412-1070/ 481) -10.3 E11-W00 S41-S36
21 648 396 (S40E35 L=266) 583 106 1 ( 590/ 376- 697/ 416) -5.7 E40-E30 S41-S39
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Download FITS filament maps as tar archive
» All Filament Data of 20231226 ...
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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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