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| 20240208 - Filament data for 12 UTC |
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Available data for 20240208: »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC »14 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 584 1711 (N30E48 L= 33) 351 39 0 ( 559/1690- 604/1730) -9.5 E50-E44 N28-N31
2 468 1561 (N18E49 L= 32) 1571 268 5 ( 422/1490- 546/1661) -30.1 E58-E39 N13-N25
3 1120 1551 (N27E03 L= 77) 866 277 1 (1014/1465-1224/1618) -25.0 E11-W04 N23-N30
4 1670 1345 (N25W38 L=119) 329 81 1 (1650/1299-1688/1384) -68.2 W36-W39 N22-N27
5 503 1291 (N02E37 L= 43) 253 57 0 ( 472/1267- 530/1315) -21.8 E39-E34 N00-N03
6 492 1123 (S08E35 L= 46) 804 287 1 ( 427/1048- 567/1233) 61.7 E38-E30 S13-N00
7 1812 1135 (N16W52 L=132) 364 65 0 (1794/1107-1830/1164) -56.3 W50-W54 N13-N17
8 698 1093 (S07E21 L= 60) 221 66 0 ( 680/1056- 716/1131) 90.0 E21-E19 S09-S04
9 1679 1049 (N07W41 L=121) 268 56 0 (1647/1030-1710/1064) 0.0 W38-W43 N06-N08
10 255 959 (S20E54 L= 27) 361 69 0 ( 240/ 923- 268/ 997) -53.1 E55-E52 S22-S18
11 671 933 (S17E20 L= 60) 205 23 0 ( 646/ 922- 697/ 947) 18.4 E21-E18 S17-S16
12 782 886 (S18E12 L= 68) 237 146 0 ( 737/ 835- 828/ 920) 50.2 E14-E09 S21-S15
13 542 780 (S28E28 L= 52) 578 162 0 ( 498/ 716- 563/ 847) 66.0 E31-E26 S32-S23
14 713 666 (S33E15 L= 66) 1222 224 0 ( 676/ 556- 759/ 779) 82.4 E17-E12 S40-S25
15 391 738 (S33E41 L= 39) 255 64 0 ( 368/ 713- 422/ 769) -38.7 E43-E38 S34-S30
16 1619 654 (S16W47 L=127) 260 45 0 (1595/ 637-1639/ 674) 33.7 W45-W48 S17-S15
17 882 621 (S33E02 L= 78) 501 147 1 ( 804/ 605- 954/ 635) 12.5 E07-W02 S34-S31
18 658 536 (S43E18 L= 62) 531 75 1 ( 612/ 507- 694/ 566) 23.2 E22-E15 S44-S40
19 959 508 (S39W06 L= 86) 215 45 0 ( 929/ 484- 986/ 528) 45.0 W03-W07 S40-S37
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Download FITS filament maps as tar archive
» All Filament Data of 20240208 ...
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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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