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| 20240529 - Latest Filament data |
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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
1 607 1655 (N31E47 L= 8) 921 204 1 ( 589/1547- 629/1736) -40.9 E53-E38 N23-N36
2 1545 1486 (N39W30 L= 85) 402 77 1 (1510/1454-1577/1513) 35.5 W26-W33 N35-N41
3 1350 1427 (N30W14 L= 69) 493 236 0 (1253/1391-1446/1492) -7.6 W06-W21 N28-N32
4 806 1439 (N20E22 L= 33) 693 155 2 ( 747/1410- 872/1482) 39.8 E25-E18 N17-N24
5 1692 1239 (N25W43 L= 98) 425 48 0 (1669/1210-1714/1266) -33.7 W40-W45 N23-N26
6 211 1218 (S04E64 L=351) 705 88 1 ( 184/1174- 238/1257) -26.6 E69-E59 S05-S01
7 1731 1144 (N19W47 L=102) 656 90 1 (1684/1114-1770/1176) 0.0 W42-W51 N18-N21
8 449 857 (S21E35 L= 20) 3610 708 5 ( 206/ 701- 692/1094) 36.3 E66-E21 S36-S02
9 177 963 (S20E65 L=350) 4990 261 11 ( 121/ 866- 233/1082) 81.9 E78-E57 S25-S11
10 1778 1062 (N15W52 L=107) 444 58 0 (1742/1048-1811/1077) 15.9 W48-W55 N14-N16
11 1209 1038 (N03W11 L= 66) 266 81 0 (1170/1008-1244/1065) 51.3 W08-W12 N00-N05
12 1545 881 (N00W35 L= 90) 686 150 2 (1490/ 852-1615/ 925) 0.0 W30-W40 S01-N01
13 1280 701 (S15W22 L= 77) 305 86 0 (1241/ 686-1336/ 716) 18.4 W19-W25 S16-S14
14 1069 667 (S22W10 L= 65) 255 68 0 (1041/ 647-1103/ 688) 0.0 W07-W12 S22-S20
15 1732 582 (S14W63 L=118) 1845 263 1 (1645/ 490-1812/ 676) 63.4 W57-W68 S20-S06
16 704 528 (S38E13 L= 42) 337 43 1 ( 685/ 496- 726/ 551) -76.0 E14-E11 S40-S36
17 645 493 (S42E18 L= 37) 293 69 1 ( 624/ 471- 676/ 515) 45.0 E19-E14 S44-S40
18 1505 383 (S31W54 L=109) 1280 130 3 (1443/ 352-1564/ 428) 20.0 W49-W61 S34-S28
19 1306 369 (S37W38 L= 93) 307 63 0 (1284/ 353-1335/ 389) 0.0 W35-W40 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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