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| 20241111 - Filament data for 12 UTC |
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Available data for 20241111: »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 1522 1692 (N28W57 L= 79) 2688 318 7 (1398/1644-1682/1736) -19.8 W45-W72 N22-N31
2 1611 1533 (N17W53 L= 75) 774 171 1 (1534/1484-1688/1574) -48.4 W48-W57 N12-N21
3 245 1223 (N32E52 L=330) 1419 256 2 ( 156/1121- 325/1296) -31.3 E67-E43 N23-N37
4 1836 1173 (S08W58 L= 80) 2265 335 7 (1769/1100-1907/1243) -39.3 W52-W66 S12-S02
5 1694 1158 (S05W44 L= 66) 471 140 3 (1669/1081-1724/1201) 35.5 W40-W47 S08-S02
6 1407 1104 (S01W23 L= 45) 626 229 1 (1360/1038-1482/1157) 0.0 W19-W28 S04-N01
7 256 1057 (N21E51 L=331) 355 60 1 ( 223/1038- 280/1081) 9.5 E54-E48 N19-N22
8 1141 918 (S05W04 L= 26) 2006 496 1 ( 994/ 750-1277/1064) -66.8 E01-W08 S17-N04
9 1546 1002 (S10W30 L= 52) 284 64 1 (1513/ 972-1568/1034) 26.6 W27-W31 S12-S08
10 1444 1000 (S08W23 L= 45) 419 99 3 (1401/ 961-1483/1027) -9.5 W20-W26 S10-S05
11 565 968 (N10E28 L=354) 518 127 0 ( 491/ 949- 633/ 988) -24.0 E32-E23 N07-N12
12 1603 743 (S27W30 L= 52) 1406 246 2 (1520/ 692-1704/ 819) -26.6 W24-W38 S30-S20
13 1404 637 (S28W14 L= 36) 1453 289 3 (1335/ 513-1456/ 776) 86.8 W11-W16 S36-S18
14 765 748 (S06E21 L= 1) 198 36 2 ( 740/ 726- 784/ 766) -63.4 E22-E19 S07-S05
15 664 468 (S21E37 L=345) 3740 718 4 ( 441/ 281- 840/ 698) 18.4 E72-E18 S28-S10
16 692 635 (S11E29 L=353) 873 194 3 ( 611/ 579- 784/ 696) -4.8 E35-E23 S13-S07
17 1394 459 (S40W10 L= 32) 842 144 2 (1335/ 396-1439/ 508) 26.6 W04-W14 S43-S37
18 1252 317 (S47E05 L= 17) 1630 152 4 (1176/ 276-1335/ 358) -8.7 E11-W02 S49-S43
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Download FITS filament maps as tar archive
» All Filament Data of 20241111 ...
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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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