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| 20260127 - Filament data for 10 UTC |
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Available data for 20260127: »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC »13 UTC »14 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 502 1614 (N26E46 L=265) 1767 347 1 ( 406/1482- 596/1750) -28.5 E69-E33 N17-N36
2 1519 1542 (N33W28 L=339) 373 79 0 (1483/1514-1561/1564) -21.8 W25-W31 N32-N34
3 186 1410 (N11E71 L=240) 972 102 1 ( 143/1389- 225/1447) 4.1 E81-E66 N09-N13
4 1168 1333 (N14W05 L=316) 264 76 0 (1124/1309-1204/1356) -21.8 W02-W07 N13-N15
5 612 1338 (N09E29 L=282) 356 114 0 ( 551/1324- 671/1350) 14.0 E33-E25 N07-N09
6 1005 1318 (N11E05 L=306) 181 44 2 ( 987/1289-1025/1346) -71.6 E05-E03 N09-N13
7 327 1267 (N02E49 L=262) 376 73 1 ( 299/1243- 365/1287) 21.8 E51-E45 N00-N03
8 1767 1189 (N15W48 L=359) 514 75 2 (1744/1163-1801/1230) -45.0 W45-W51 N12-N17
9 1887 1082 (N11W61 L= 12) 1394 254 3 (1861/ 988-1920/1202) 69.0 W58-W66 N05-N18
10 303 965 (S16E48 L=263) 1986 311 2 ( 277/ 817- 353/1106) 73.6 E51-E44 S24-S07
11 482 1040 (S10E34 L=277) 529 75 1 ( 451/ 999- 508/1074) -45.0 E36-E31 S12-S07
12 724 910 (S16E17 L=294) 200 43 0 ( 703/ 885- 741/ 933) -33.7 E18-E15 S16-S14
13 731 810 (S21E16 L=295) 798 297 0 ( 600/ 735- 814/ 908) 42.7 E24-E11 S27-S14
14 854 864 (S17E08 L=303) 337 74 0 ( 821/ 844- 893/ 884) -11.3 E10-E05 S18-S15
15 1318 823 (S14W20 L=331) 234 111 0 (1293/ 775-1346/ 876) -56.3 W18-W22 S16-S10
16 1709 836 (S07W47 L=358) 359 81 0 (1669/ 816-1752/ 859) 26.6 W44-W50 S08-S04
17 678 827 (S21E19 L=292) 196 38 0 ( 650/ 812- 705/ 841) 14.0 E21-E17 S21-S19
18 234 647 (S35E63 L=248) 471 47 1 ( 211/ 629- 264/ 667) -8.1 E66-E58 S36-S34
19 1500 559 (S26W40 L=351) 360 67 1 (1460/ 544-1545/ 579) 0.0 W36-W43 S27-S25
20 693 452 (S46E18 L=293) 371 79 1 ( 674/ 413- 713/ 499) -90.0 E20-E16 S48-S41
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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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