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| 20241230 - Filament data for 08 UTC |
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Available data for 20241230: »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 1384 1555 (N30W27 L=125) 2262 551 5 (1154/1468-1624/1674) -23.0 W11-W44 N23-N38
2 450 1509 (N30E41 L= 57) 737 144 1 ( 396/1445- 488/1558) -38.7 E47-E36 N25-N33
3 1192 1435 (N22W12 L=110) 395 175 0 (1148/1378-1210/1519) 71.6 W08-W12 N18-N27
4 1075 1463 (N24W05 L=103) 399 112 2 (1024/1438-1121/1481) 9.5 W01-W07 N22-N25
5 1299 1301 (N13W18 L=116) 472 190 1 (1285/1203-1324/1391) 79.7 W16-W19 N07-N18
6 1665 1316 (N14W44 L=142) 312 72 3 (1638/1278-1685/1343) -76.0 W41-W45 N11-N15
7 1857 1292 (N13W63 L=161) 724 52 0 (1832/1263-1884/1325) -36.9 W60-W66 N10-N14
8 185 768 (S14E65 L= 33) 4849 583 10 ( 110/ 500- 252/1033) 81.1 E77-E59 S31-N01
9 1874 855 (S14W63 L=162) 6360 0 23 (1761/ 723-1956/ 990) 36.9 W52-W79 S21-S05
10 739 960 (S06E17 L= 81) 286 57 2 ( 711/ 927- 767/ 989) 56.3 E19-E15 S07-S04
11 794 916 (S09E14 L= 84) 434 79 3 ( 772/ 873- 816/ 957) -78.7 E15-E12 S11-S06
12 857 867 (S12E11 L= 88) 176 73 0 ( 819/ 855- 895/ 883) 0.0 E12-E08 S12-S10
13 295 817 (S12E51 L= 47) 1214 171 4 ( 243/ 740- 346/ 863) 49.4 E56-E45 S16-S09
14 586 778 (S16E29 L= 70) 315 84 0 ( 562/ 734- 616/ 820) -68.2 E30-E27 S18-S13
15 473 665 (S22E39 L= 59) 1479 414 1 ( 339/ 627- 623/ 737) 0.0 E49-E26 S24-S17
16 1547 611 (S29W36 L=135) 272 58 2 (1529/ 583-1573/ 646) -45.0 W34-W38 S30-S26
17 1161 549 (S32W08 L=106) 474 213 0 (1056/ 535-1253/ 567) 4.1 W00-W14 S33-S31
18 828 383 (S43E19 L= 80) 1702 426 3 ( 645/ 288- 985/ 488) 19.9 E40-E04 S50-S36
19 1217 207 (S61W20 L=118) 1456 127 3 (1150/ 183-1280/ 239) -3.2 W10-W29 S63-S57
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Download FITS filament maps as tar archive
» All Filament Data of 20241230 ...
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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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