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| 20250824 - Filament data for 12 UTC |
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Available data for 20250824: »06 UTC »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC »13 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 1319 1724 (N42W45 L=252) 1233 262 4 (1194/1688-1432/1748) -9.1 W32-W57 N38-N46
2 1011 1676 (N48W17 L=224) 333 65 0 ( 988/1643-1042/1700) 15.9 W14-W21 N45-N49
3 698 1555 (N47E13 L=194) 1618 320 5 ( 592/1493- 851/1621) 2.4 E23-W01 N43-N48
4 1576 1355 (N14W43 L=250) 664 227 0 (1489/1268-1630/1423) -71.6 W39-W44 N07-N19
5 504 1345 (N36E31 L=176) 401 85 0 ( 460/1316- 540/1368) -29.7 E34-E27 N33-N37
6 888 1138 (N16E06 L=201) 1105 335 0 ( 811/1004- 974/1274) -77.5 E08-E03 N07-N25
7 605 1231 (N27E23 L=184) 383 112 0 ( 549/1217- 662/1245) -7.1 E27-E19 N25-N27
8 209 982 (N17E61 L=146) 514 81 1 ( 191/ 951- 238/1020) 76.0 E62-E56 N14-N18
9 1497 990 (S05W28 L=235) 270 54 0 (1475/ 965-1522/1019) -76.0 W26-W29 S06-S02
10 1571 872 (S13W31 L=238) 251 59 0 (1548/ 844-1591/ 904) 45.0 W29-W32 S14-S11
11 303 770 (N03E54 L=153) 522 69 1 ( 277/ 732- 328/ 803) -68.2 E56-E51 N00-N05
12 711 737 (S04E24 L=183) 308 87 1 ( 697/ 698- 723/ 791) 59.0 E25-E22 S06-S01
13 1629 722 (S24W34 L=241) 878 174 1 (1573/ 684-1691/ 782) -35.0 W29-W39 S27-S19
14 1763 534 (S43W53 L=260) 706 54 1 (1734/ 515-1792/ 561) -28.3 W47-W61 S46-S39
15 1594 437 (S45W33 L=240) 2409 396 3 (1426/ 344-1742/ 520) 3.3 W15-W51 S49-S41
16 355 439 (S19E66 L=141) 4437 224 9 ( 276/ 370- 448/ 517) -48.0 E77-E55 S24-S13
17 602 407 (S24E43 L=164) 1302 213 1 ( 572/ 307- 631/ 500) 51.8 E49-E37 S31-S17
18 1204 445 (S33E01 L=206) 236 74 0 (1172/ 417-1236/ 476) 31.0 E03-W02 S34-S31
19 1039 378 (S34E14 L=193) 447 120 1 (1021/ 312-1069/ 419) 58.0 E16-E10 S39-S30
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Download FITS filament maps as tar archive
» All Filament Data of 20250824 ...
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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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