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| 20250811 - Filament data for 07 UTC |
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Available data for 20250811: »06 UTC »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 1114 1828 (N59W35 L= 57) 1503 254 3 ( 996/1783-1224/1866) 0.0 W18-W52 N56-N60
2 1430 1596 (N34W43 L= 64) 519 185 0 (1341/1555-1505/1620) -38.7 W36-W47 N29-N37
3 1362 1492 (N29W32 L= 54) 464 151 1 (1302/1472-1437/1517) -29.1 W28-W37 N26-N31
4 463 1344 (N33E37 L=345) 1913 404 1 ( 405/1169- 527/1512) 72.3 E40-E32 N22-N44
5 1829 1292 (N07W65 L= 86) 974 130 1 (1805/1240-1854/1365) 45.0 W60-W69 N04-N11
6 259 1240 (N28E56 L=325) 2846 297 8 ( 167/1133- 351/1352) -25.8 E77-E45 N21-N35
7 722 1212 (N22E16 L= 5) 294 89 0 ( 682/1197- 758/1237) 0.0 E19-E13 N20-N23
8 1110 1146 (N12W07 L= 28) 243 96 0 (1068/1129-1159/1167) -31.0 W04-W09 N10-N14
9 1569 1051 (S01W34 L= 56) 538 87 0 (1512/1033-1620/1070) -7.1 W30-W38 S02-N00
10 1701 864 (S15W43 L= 64) 1329 198 2 (1616/ 814-1775/ 928) 11.3 W35-W50 S17-S12
11 868 622 (S16E16 L= 6) 1009 340 0 ( 747/ 555- 951/ 735) 32.7 E24-E09 S19-S09
12 551 639 (S11E37 L=345) 1128 189 2 ( 531/ 538- 588/ 718) 61.4 E40-E32 S17-S05
13 700 643 (S12E26 L=355) 326 60 2 ( 662/ 629- 741/ 660) -11.3 E28-E23 S13-S10
14 277 535 (S16E69 L=313) 739 122 2 ( 249/ 503- 292/ 589) 33.7 E75-E63 S18-S12
15 321 547 (S15E61 L=320) 517 51 1 ( 306/ 513- 336/ 581) 59.0 E64-E58 S17-S12
16 1548 398 (S46W33 L= 55) 1610 281 4 (1457/ 339-1682/ 495) 15.3 W24-W46 S49-S40
17 1347 315 (S48W13 L= 35) 424 62 1 (1324/ 290-1375/ 340) -59.0 W11-W16 S50-S45
18 1280 251 (S53W06 L= 28) 1068 114 3 (1230/ 220-1328/ 292) -11.3 W01-W11 S57-S48
19 1276 189 (S61W06 L= 27) 647 70 1 (1235/ 173-1311/ 206) -26.6 W00-W10 S63-S57
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Download FITS filament maps as tar archive
» All Filament Data of 20250811 ...
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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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