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| 20250807 - Filament data for 06 UTC |
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Available data for 20250807: »06 UTC »07 UTC »08 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 1202 1836 (N58W44 L=119) 421 49 0 (1189/1806-1216/1866) 22.6 W38-W50 N55-N60
2 865 1738 (N57E00 L= 75) 421 58 0 ( 841/1712- 898/1760) 9.5 E03-W03 N54-N58
3 771 1727 (N58E11 L= 64) 321 24 0 ( 748/1710- 794/1743) 21.8 E14-E08 N56-N59
4 600 1704 (N59E33 L= 42) 1059 192 2 ( 512/1674- 692/1733) 4.8 E46-E21 N55-N60
5 857 1369 (N29E06 L= 69) 435 186 2 ( 797/1298- 886/1414) -60.9 E10-E04 N24-N33
6 645 1328 (N29E22 L= 53) 325 124 0 ( 611/1286- 695/1375) -45.0 E24-E18 N26-N32
7 143 1199 (N24E74 L= 1) 759 104 0 ( 132/1159- 160/1254) -33.7 E79-E69 N21-N27
8 256 1153 (N21E56 L= 19) 790 124 1 ( 237/1090- 274/1208) 90.0 E57-E53 N17-N24
9 1402 1154 (N08W25 L=100) 227 59 0 (1375/1127-1420/1173) -90.0 W23-W26 N06-N09
10 1805 992 (S09W54 L=129) 386 84 3 (1780/ 958-1827/1013) -53.1 W51-W56 S10-S06
11 1798 908 (S14W53 L=128) 884 206 0 (1746/ 848-1845/ 973) 28.6 W47-W58 S16-S10
12 692 830 (S02E23 L= 52) 343 190 0 ( 607/ 817- 782/ 858) -16.7 E28-E17 S03-N01
13 1804 686 (S29W56 L=131) 1302 158 1 (1750/ 635-1846/ 748) 36.9 W50-W62 S31-S24
14 807 631 (S15E19 L= 56) 205 36 0 ( 784/ 617- 831/ 645) -18.4 E20-E17 S16-S13
15 1640 597 (S31W39 L=114) 414 60 1 (1604/ 579-1668/ 617) 9.5 W35-W42 S32-S29
16 256 559 (S16E70 L= 5) 903 104 1 ( 241/ 519- 271/ 609) 41.2 E78-E65 S19-S12
17 1258 376 (S40W07 L= 82) 436 105 2 (1206/ 355-1309/ 396) 0.0 W03-W11 S41-S39
18 1109 327 (S42E05 L= 70) 383 49 1 (1081/ 304-1137/ 346) -36.9 E07-E03 S43-S39
19 925 242 (S46E24 L= 51) 1023 135 1 ( 870/ 211-1006/ 269) 7.6 E31-E16 S48-S43
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Download FITS filament maps as tar archive
» All Filament Data of 20250807 ...
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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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