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| 20240629 - Filament data for 08 UTC |
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Available data for 20240629: »06 UTC »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
1 589 1540 (N34E37 L=331) 396 95 0 ( 572/1482- 605/1580) -54.5 E39-E33 N29-N36
2 1584 1480 (N33W43 L= 50) 763 146 2 (1511/1438-1634/1518) -29.1 W36-W46 N30-N36
3 866 1478 (N31E13 L=354) 621 244 0 ( 779/1404- 945/1514) -21.0 E19-E06 N26-N33
4 1348 1478 (N33W22 L= 29) 238 85 0 (1313/1446-1379/1506) -38.7 W19-W24 N30-N34
5 1309 1435 (N30W19 L= 26) 319 206 0 (1217/1389-1386/1464) -18.4 W11-W24 N26-N31
6 1103 1199 (N14W04 L= 12) 335 79 1 (1073/1177-1146/1225) -11.3 W02-W07 N12-N15
7 707 967 (S02E20 L=348) 281 131 1 ( 659/ 935- 752/ 987) -18.4 E22-E16 S03-N00
8 468 934 (S05E36 L=331) 488 70 1 ( 444/ 891- 493/ 971) -78.7 E37-E34 S08-S03
9 1681 905 (S03W45 L= 52) 803 120 3 (1631/ 867-1735/ 947) -16.7 W40-W50 S05-N00
10 1048 800 (S11W02 L= 10) 275 94 1 (1009/ 767-1087/ 829) -36.9 W00-W04 S12-S09
11 435 769 (S16E40 L=328) 289 98 1 ( 418/ 733- 455/ 812) 68.2 E40-E37 S18-S13
12 1808 769 (S12W61 L= 68) 481 51 2 (1790/ 742-1832/ 798) -53.1 W58-W64 S13-S09
13 1402 769 (S12W25 L= 33) 251 71 1 (1367/ 747-1439/ 782) 11.3 W22-W27 S13-S10
14 857 677 (S20E10 L=358) 1015 215 7 ( 798/ 597- 904/ 769) -70.0 E13-E06 S24-S13
15 965 694 (S18E03 L= 5) 620 110 4 ( 922/ 642-1009/ 739) -50.2 E05-W00 S21-S15
16 410 568 (S30E46 L=321) 1512 248 3 ( 358/ 508- 508/ 655) -32.5 E49-E37 S34-S24
17 1138 488 (S32W10 L= 18) 4101 618 13 ( 926/ 389-1374/ 648) 28.9 E04-W25 S40-S19
18 747 582 (S27E17 L=350) 821 185 3 ( 683/ 533- 823/ 629) 32.5 E22-E11 S30-S23
19 1497 496 (S30W38 L= 46) 1540 309 4 (1370/ 429-1627/ 553) 25.3 W29-W48 S35-S25
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Download FITS filament maps as tar archive
» All Filament Data of 20240629 ...
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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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