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| 20221220 - Filament data for 11 UTC |
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Available data for 20221220: »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
1 634 1452 (N28E23 L=134) 1034 284 2 ( 577/1359- 725/1565) -51.3 E28-E16 N21-N36
2 884 1525 (N31E06 L=151) 305 99 0 ( 842/1497- 928/1558) -33.7 E08-E02 N28-N33
3 367 1394 (N27E45 L=112) 675 142 1 ( 341/1338- 395/1467) -48.4 E49-E41 N22-N31
4 251 1278 (N20E55 L=102) 1039 148 3 ( 214/1219- 297/1316) 56.3 E60-E50 N16-N22
5 1408 1074 (S01W24 L=181) 506 95 2 (1368/1031-1442/1116) -63.4 W21-W25 S03-N01
6 1877 975 (S10W63 L=219) 890 106 2 (1828/ 926-1912/1021) -59.0 W56-W68 S12-S07
7 1796 978 (S09W53 L=210) 344 56 1 (1770/ 952-1825/ 999) 18.4 W50-W56 S10-S08
8 1801 864 (S16W55 L=211) 562 100 2 (1767/ 827-1829/ 906) 33.7 W51-W57 S18-S13
9 1860 865 (S16W62 L=218) 410 45 3 (1833/ 844-1878/ 895) 26.6 W58-W64 S17-S14
10 1349 800 (S17W19 L=175) 205 98 0 (1313/ 774-1394/ 833) 31.0 W16-W21 S18-S15
11 706 716 (S18E23 L=134) 277 82 1 ( 693/ 672- 735/ 750) 68.2 E23-E20 S20-S15
12 1206 535 (S33W09 L=165) 2002 701 2 ( 995/ 375-1488/ 725) 26.6 E08-W28 S43-S22
13 273 703 (S15E58 L= 99) 374 66 0 ( 254/ 677- 304/ 721) 9.5 E60-E54 S15-S13
14 1732 636 (S30W52 L=209) 873 167 2 (1694/ 604-1786/ 672) -14.0 W47-W59 S32-S27
15 464 621 (S21E43 L=114) 299 58 2 ( 441/ 596- 489/ 652) 45.0 E44-E40 S22-S19
16 359 557 (S24E55 L=102) 561 89 1 ( 334/ 515- 390/ 598) -80.5 E56-E53 S27-S21
17 751 551 (S28E23 L=134) 358 72 0 ( 716/ 530- 799/ 568) 0.0 E25-E19 S29-S27
18 922 426 (S39E13 L=143) 900 205 0 ( 855/ 365- 994/ 501) -59.7 E16-E08 S44-S32
19 1393 246 (S60W34 L=191) 1191 107 2 (1339/ 225-1456/ 280) -10.8 W25-W46 S62-S55
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Download FITS filament maps as tar archive
» All Filament Data of 20221220 ...
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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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