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| 20240529 - Filament data for 06 UTC |
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Available data for 20240529: »06 UTC »07 UTC »08 UTC »09 UTC »10 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
1 575 1684 (N32E52 L= 7) 843 154 1 ( 557/1600- 602/1746) -47.7 E57-E46 N25-N36
2 1510 1500 (N39W27 L= 85) 373 76 2 (1478/1464-1530/1528) 56.3 W23-W28 N35-N41
3 740 1463 (N20E27 L= 31) 872 193 2 ( 671/1429- 810/1524) 40.6 E32-E23 N17-N23
4 855 1495 (N25E21 L= 38) 224 41 1 ( 837/1476- 881/1513) -14.0 E22-E18 N23-N25
5 1297 1442 (N30W10 L= 69) 492 217 0 (1208/1409-1385/1509) -12.1 W02-W16 N28-N32
6 1643 1269 (N26W38 L= 97) 284 47 1 (1626/1245-1660/1297) -56.3 W36-W39 N24-N27
7 169 1243 (S03E72 L=347) 728 79 1 ( 144/1208- 189/1274) -13.0 E79-E66 S04-S01
8 1681 1163 (N20W42 L=101) 762 93 2 (1637/1130-1721/1207) -8.1 W38-W45 N17-N22
9 410 875 (S21E39 L= 20) 3524 673 5 ( 188/ 692- 629/1108) 36.5 E71-E25 S37-S03
10 1736 1068 (N15W48 L=107) 509 65 0 (1695/1049-1767/1086) 26.6 W44-W51 N13-N16
11 152 978 (S19E69 L=350) 4553 215 8 ( 105/ 894- 198/1066) 40.2 E81-E61 S24-S13
12 1683 941 (N06W45 L=104) 416 94 0 (1655/ 899-1717/ 977) -26.6 W41-W48 N04-N08
13 1493 893 (S00W31 L= 90) 677 131 1 (1438/ 866-1561/ 931) 12.5 W27-W36 S01-N01
14 1489 751 (S09W35 L= 93) 261 182 0 (1456/ 723-1547/ 806) 0.0 W32-W38 S10-S05
15 1132 699 (S18W13 L= 72) 912 367 3 ( 969/ 654-1302/ 728) 30.1 W03-W22 S24-S13
16 1694 591 (S14W58 L=117) 2119 299 2 (1607/ 496-1788/ 704) 59.0 W53-W64 S21-S06
17 655 539 (S39E17 L= 42) 353 50 2 ( 636/ 510- 675/ 568) 68.2 E18-E15 S41-S36
18 1450 395 (S31W48 L=107) 1076 130 1 (1380/ 370-1501/ 438) 32.0 W43-W52 S34-S28
19 1268 380 (S37W34 L= 93) 305 46 0 (1242/ 359-1290/ 401) -9.5 W31-W37 S37-S35
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Download FITS filament maps as tar archive
» All Filament Data of 20240529 ...
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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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