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| 20230928 - Filament data for 06 UTC |
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Available data for 20230928: »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 1168 1751 (N45W41 L= 77) 804 82 2 (1135/1716-1211/1774) -68.2 W35-W45 N42-N47
2 1686 1519 (N14W62 L= 99) 679 126 0 (1626/1502-1734/1538) -13.0 W55-W69 N11-N15
3 1088 1347 (N23W13 L= 49) 302 77 1 (1057/1322-1117/1378) 11.3 W10-W15 N21-N25
4 1758 1298 (N00W56 L= 92) 702 114 1 (1731/1231-1781/1349) 71.6 W54-W58 S03-N03
5 877 1313 (N27E01 L= 35) 197 43 0 ( 863/1280- 891/1339) 71.6 E01-W00 N25-N28
6 824 1144 (N19E08 L= 28) 716 193 1 ( 754/1075- 884/1213) 20.0 E14-E03 N16-N21
7 266 1037 (N25E53 L=343) 1862 247 7 ( 229/ 942- 328/1149) -77.0 E57-E47 N19-N32
8 1167 1117 (N08W10 L= 47) 222 56 0 (1148/1095-1188/1138) 18.4 W09-W12 N07-N09
9 457 1060 (N22E35 L= 1) 657 190 1 ( 368/1007- 516/1092) -32.5 E42-E31 N18-N25
10 1857 937 (S24W56 L= 93) 726 118 0 (1821/ 890-1878/ 989) 20.6 W51-W59 S25-S21
11 412 871 (N12E42 L=354) 281 42 0 ( 392/ 853- 432/ 893) -45.0 E43-E40 N11-N13
12 1530 840 (S18W25 L= 61) 1192 359 2 (1366/ 817-1697/ 872) -20.6 W14-W38 S22-S12
13 312 784 (N09E53 L=343) 540 128 0 ( 279/ 735- 349/ 844) -69.4 E55-E51 N05-N13
14 1826 761 (S34W52 L= 88) 614 83 1 (1788/ 743-1873/ 777) -23.2 W46-W60 S37-S31
15 1091 731 (S11E04 L= 32) 311 126 0 (1046/ 689-1126/ 776) 23.2 E07-W00 S12-S09
16 680 544 (S12E34 L= 2) 1031 386 0 ( 618/ 409- 748/ 712) 38.7 E44-E23 S19-S03
17 478 347 (S21E63 L=333) 1300 137 3 ( 439/ 300- 512/ 396) 45.0 E69-E56 S25-S17
18 561 332 (S24E56 L=340) 528 77 0 ( 523/ 313- 586/ 359) 0.0 E59-E51 S25-S22
19 757 306 (S30E42 L=354) 655 109 0 ( 726/ 254- 798/ 345) 22.6 E48-E36 S33-S27
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Download FITS filament maps as tar archive
» All Filament Data of 20230928 ...
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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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