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| 20241207 - Filament data for 10 UTC |
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Available data for 20241207: »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 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 1554 1650 (N30W52 L= 92) 1259 151 2 (1524/1574-1587/1725) 54.0 W48-W58 N24-N35
2 1299 1594 (N30W28 L= 69) 653 144 1 (1223/1572-1369/1608) -16.7 W23-W33 N28-N32
3 1689 1528 (N20W57 L= 97) 427 55 0 (1657/1505-1716/1546) -36.9 W53-W59 N18-N21
4 1795 1477 (N16W66 L=106) 634 101 1 (1768/1417-1816/1511) 45.0 W63-W70 N12-N17
5 1353 1337 (N14W24 L= 65) 221 79 0 (1308/1320-1390/1354) -11.3 W21-W26 N12-N15
6 748 1209 (N15E14 L= 26) 397 127 0 ( 704/1158- 786/1259) -60.3 E16-E11 N11-N18
7 1707 1103 (S05W45 L= 85) 312 72 2 (1672/1080-1735/1132) 18.4 W41-W47 S05-S03
8 1447 988 (S08W25 L= 65) 944 344 1 (1368/ 848-1488/1120) -82.4 W21-W27 S15-N00
9 1289 1036 (S03W16 L= 56) 606 185 1 (1260/ 958-1345/1105) 49.4 W13-W19 S07-N00
10 846 928 (S03E12 L= 29) 1644 399 6 ( 709/ 740- 937/1041) -63.4 E18-E08 S15-N04
11 1638 995 (S10W38 L= 78) 702 155 4 (1574/ 953-1711/1034) -10.3 W33-W44 S12-S06
12 723 815 (S08E21 L= 20) 279 110 1 ( 676/ 781- 745/ 860) 31.0 E23-E18 S09-S05
13 495 827 (S04E35 L= 5) 212 84 0 ( 471/ 788- 524/ 857) 38.7 E37-E32 S06-S02
14 193 716 (S07E66 L=334) 881 94 4 ( 157/ 682- 228/ 751) 15.3 E72-E61 S08-S04
15 956 514 (S30E13 L= 28) 2481 487 8 ( 847/ 344-1016/ 735) 52.0 E25-E07 S40-S16
16 1370 663 (S26W17 L= 57) 1170 275 2 (1248/ 612-1482/ 729) 13.2 W08-W25 S28-S23
17 409 661 (S13E46 L=354) 1331 277 2 ( 308/ 588- 535/ 714) -19.4 E53-E36 S17-S08
18 408 486 (S23E54 L=346) 2920 369 6 ( 296/ 400- 564/ 606) 11.8 E79-E36 S27-S17
19 709 295 (S41E40 L=360) 705 90 2 ( 668/ 274- 760/ 319) 0.0 E44-E34 S43-S39
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Download FITS filament maps as tar archive
» All Filament Data of 20241207 ...
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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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