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| 20240122 - Filament data for 08 UTC |
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Available data for 20240122: »07 UTC »08 UTC »09 UTC »10 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 668 1809 (N46E44 L=262) 1456 154 2 ( 613/1776- 744/1843) -12.8 E56-E34 N42-N49
2 1095 1703 (N40E02 L=304) 1237 418 0 ( 896/1677-1262/1738) 6.3 E17-W10 N36-N41
3 625 1628 (N30E36 L=271) 609 148 1 ( 584/1567- 649/1677) -45.0 E41-E31 N25-N33
4 1522 1648 (N42W34 L=340) 454 89 0 (1476/1628-1564/1668) -6.3 W29-W38 N40-N43
5 781 1598 (N29E23 L=283) 518 100 3 ( 762/1548- 807/1655) -63.4 E25-E20 N25-N33
6 1764 1546 (N39W61 L= 7) 1177 143 2 (1704/1489-1808/1586) -24.4 W53-W67 N34-N40
7 307 1469 (N18E58 L=248) 1562 159 3 ( 270/1406- 362/1538) -27.9 E67-E50 N13-N22
8 1099 1352 (N15W02 L=308) 531 228 0 (1055/1260-1148/1464) -63.4 E01-W05 N09-N22
9 1557 1310 (N18W32 L=338) 359 148 0 (1497/1285-1629/1345) -11.3 W27-W37 N17-N19
10 1179 1221 (N08W07 L=314) 188 62 0 (1146/1207-1211/1233) 14.0 W05-W09 N07-N08
11 1483 1181 (N09W27 L=333) 326 115 0 (1450/1127-1518/1227) -51.3 W24-W29 N06-N11
12 1829 1142 (N11W56 L= 2) 420 76 0 (1814/1111-1847/1182) 76.0 W54-W58 N09-N13
13 1486 1047 (N01W28 L=334) 537 115 0 (1442/1008-1542/1074) 26.6 W25-W31 S01-N03
14 1789 943 (S01W53 L=360) 1104 161 1 (1727/ 903-1864/ 985) 21.0 W48-W61 S04-N02
15 441 626 (S34E41 L=265) 682 174 0 ( 420/ 536- 468/ 703) 59.7 E45-E36 S40-S28
16 1038 506 (S37W07 L=313) 2855 481 5 ( 864/ 404-1208/ 664) 47.9 E05-W15 S46-S25
17 1652 641 (S21W49 L=355) 398 97 1 (1606/ 617-1703/ 662) 26.6 W45-W53 S22-S18
18 650 595 (S35E23 L=283) 568 142 0 ( 588/ 574- 722/ 613) 10.3 E28-E17 S36-S33
19 1056 373 (S47W11 L=317) 250 60 0 (1029/ 357-1091/ 388) 26.6 W08-W13 S48-S45
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Download FITS filament maps as tar archive
» All Filament Data of 20240122 ...
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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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