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| 20260127 - Filament data for 11 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
1 435 1716 (N33E61 L=249) 610 18 0 ( 415/1695- 455/1735) 33.7 E65-E57 N31-N34
2 533 1579 (N23E41 L=269) 1134 286 1 ( 434/1481- 605/1671) -26.6 E56-E32 N17-N29
3 1521 1543 (N34W28 L=339) 333 82 1 (1487/1513-1563/1565) -21.8 W25-W31 N32-N34
4 192 1411 (N11E70 L=241) 1090 105 1 ( 146/1390- 230/1450) 14.0 E80-E64 N09-N13
5 1183 1327 (N14W06 L=316) 233 83 0 (1138/1301-1214/1351) -26.6 W03-W07 N12-N15
6 621 1336 (N09E28 L=282) 347 115 0 ( 562/1323- 679/1348) 14.0 E32-E24 N07-N09
7 330 1263 (N02E49 L=262) 355 54 0 ( 303/1242- 350/1288) 45.0 E50-E46 N00-N03
8 1773 1185 (N14W48 L=359) 575 80 2 (1746/1147-1804/1228) -78.7 W45-W51 N12-N17
9 1886 1078 (N10W61 L= 12) 1467 234 4 (1858/ 987-1922/1197) 65.2 W57-W67 N05-N18
10 310 963 (S16E47 L=263) 2186 355 4 ( 283/ 802- 360/1107) 80.5 E50-E43 S25-S07
11 491 1040 (S10E33 L=277) 417 60 0 ( 471/1009- 512/1076) -76.0 E34-E31 S11-S07
12 727 916 (S15E17 L=294) 213 57 0 ( 710/ 888- 745/ 951) -71.6 E17-E15 S16-S13
13 778 825 (S20E13 L=298) 1132 412 1 ( 618/ 740- 904/ 906) 26.6 E23-E05 S26-S14
14 1326 822 (S14W21 L=331) 242 118 0 (1299/ 774-1355/ 875) -45.0 W18-W23 S16-S10
15 1715 835 (S07W48 L=358) 347 78 0 (1677/ 815-1758/ 856) 23.2 W44-W51 S08-S04
16 684 825 (S21E19 L=291) 196 36 1 ( 658/ 806- 710/ 839) 18.4 E20-E17 S22-S19
17 237 646 (S35E62 L=248) 501 55 0 ( 215/ 627- 269/ 665) -7.1 E66-E57 S36-S34
18 1496 556 (S27W40 L=350) 286 51 1 (1463/ 539-1529/ 575) 0.0 W36-W42 S27-S25
19 705 442 (S46E17 L=293) 501 99 1 ( 678/ 406- 739/ 499) -81.9 E19-E14 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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