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| 20241126 - Filament data for 08 UTC |
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Available data for 20241126: »07 UTC »08 UTC »09 UTC »11 UTC »12 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 443 1591 (N49E37 L=149) 346 39 1 ( 425/1567- 466/1614) -35.5 E40-E33 N46-N51
2 1228 1550 (N28W24 L=211) 261 82 1 (1190/1528-1269/1572) -21.8 W21-W26 N26-N30
3 1702 1410 (N11W53 L=240) 811 112 1 (1643/1374-1752/1446) -32.0 W48-W56 N07-N12
4 750 1323 (N24E11 L=175) 211 69 0 ( 713/1309- 787/1338) -11.3 E13-E08 N22-N25
5 1031 1278 (N16W05 L=192) 841 338 0 ( 889/1230-1172/1328) -14.0 E03-W13 N13-N19
6 261 1125 (N21E50 L=136) 806 162 2 ( 190/1077- 321/1183) -34.7 E58-E44 N16-N25
7 349 1129 (N19E42 L=144) 531 85 0 ( 317/1094- 388/1168) 18.4 E45-E38 N17-N21
8 1948 1111 (S11W73 L=260) 939 81 3 (1928/1067-1970/1141) -63.4 W69-W79 S13-S09
9 107 1032 (N18E71 L=115) 4357 184 4 ( 75/ 938- 140/1116) -65.6 E79-E65 N11-N22
10 166 958 (N12E63 L=124) 701 78 0 ( 133/ 920- 195/ 987) -68.2 E67-E59 N09-N14
11 347 932 (N08E45 L=142) 447 65 1 ( 306/ 909- 383/ 948) -15.9 E48-E41 N06-N09
12 1455 908 (S13W24 L=210) 199 57 0 (1424/ 895-1488/ 924) -26.6 W21-W25 S14-S11
13 512 643 (S11E40 L=147) 1879 522 2 ( 424/ 482- 555/ 867) 45.0 E53-E32 S20-N01
14 775 698 (S13E21 L=166) 1148 401 2 ( 647/ 624- 910/ 792) 11.9 E30-E11 S15-S09
15 267 699 (S04E58 L=128) 346 45 1 ( 239/ 677- 287/ 715) -33.7 E61-E55 S05-S02
16 1737 592 (S39W47 L=234) 1944 363 2 (1590/ 485-1874/ 693) 14.0 W32-W65 S44-S35
17 283 603 (S10E61 L=125) 783 72 0 ( 254/ 569- 304/ 644) 21.8 E66-E56 S11-S07
18 612 609 (S15E34 L=153) 325 48 1 ( 594/ 577- 630/ 638) 56.3 E35-E31 S16-S13
19 655 450 (S26E37 L=149) 1017 276 2 ( 532/ 419- 789/ 489) -2.9 E47-E26 S27-S23
20 1378 363 (S48W12 L=199) 496 47 1 (1345/ 337-1405/ 390) 36.9 W09-W15 S50-S46
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Download FITS filament maps as tar archive
» All Filament Data of 20241126 ...
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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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