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| 20240422 - Latest Filament data |
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Available data for 20240422: »06 UTC »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 1015 1723 (N37E25 L=161) 1073 319 3 ( 875/1652-1126/1796) -4.6 E39-E14 N34-N39
2 866 1577 (N23E26 L=159) 1132 333 2 ( 794/1430- 927/1686) -35.8 E36-E18 N14-N28
3 641 1619 (N19E43 L=143) 607 145 0 ( 584/1579- 693/1672) 77.5 E45-E41 N15-N24
4 488 1572 (N13E52 L=134) 393 113 0 ( 445/1555- 540/1593) 6.3 E57-E48 N11-N14
5 1683 1457 (N42W35 L=221) 511 95 0 (1641/1424-1729/1481) 5.7 W30-W40 N40-N43
6 756 1256 (N01E21 L=164) 1133 303 1 ( 709/1121- 801/1383) -82.9 E23-E18 S07-N09
7 402 1270 (S07E46 L=140) 799 175 2 ( 339/1208- 477/1318) 41.6 E49-E40 S11-S02
8 1776 1274 (N33W46 L=232) 573 61 0 (1754/1240-1795/1312) -53.1 W43-W48 N30-N35
9 198 1239 (S13E66 L=120) 1003 122 2 ( 179/1175- 224/1298) -82.9 E69-E63 S16-S08
10 554 1227 (S06E33 L=153) 573 132 1 ( 535/1156- 575/1291) -63.4 E35-E30 S09-S01
11 1653 1197 (N23W34 L=220) 608 169 1 (1626/1130-1671/1276) 90.0 W31-W37 N18-N28
12 1415 1124 (N11W19 L=205) 380 73 1 (1381/1098-1456/1151) 9.5 W16-W22 N10-N12
13 1629 1073 (N15W35 L=221) 276 95 0 (1595/1039-1670/1102) -8.1 W32-W39 N14-N16
14 764 845 (S22E10 L=176) 486 150 0 ( 717/ 780- 813/ 896) 71.6 E11-E08 S26-S17
15 1149 812 (S13W13 L=199) 255 109 0 (1124/ 778-1183/ 848) -36.9 W10-W15 S14-S11
16 1452 686 (S11W35 L=221) 1166 334 5 (1313/ 643-1540/ 740) 34.7 W27-W42 S17-S06
17 1297 717 (S14W25 L=211) 209 28 0 (1276/ 701-1319/ 732) 56.3 W23-W25 S15-S12
18 1459 636 (S14W38 L=224) 325 65 1 (1437/ 598-1481/ 667) -68.2 W35-W39 S16-S11
19 1091 570 (S28W18 L=204) 1237 424 0 ( 934/ 526-1277/ 653) 11.3 W05-W30 S31-S23
20 926 302 (S52W23 L=209) 591 124 0 ( 864/ 284- 988/ 326) 15.3 W17-W29 S53-S49
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Download FITS filament maps as tar archive
» All Filament Data of 20240422 ...
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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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