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| 20230311 - Filament data for 10 UTC |
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Available data for 20230311: »06 UTC »07 UTC »08 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
1 887 1726 (N32E31 L=140) 1571 354 1 ( 807/1616- 975/1783) 85.9 E36-E22 N22-N36
2 1290 1671 (N40E02 L=169) 707 191 1 (1209/1614-1336/1727) -20.0 E09-W02 N36-N42
3 373 1663 (N17E71 L=100) 792 108 3 ( 340/1614- 394/1701) -60.3 E76-E65 N13-N20
4 486 1479 (N07E46 L=125) 781 140 3 ( 415/1447- 533/1527) 45.0 E50-E42 N03-N10
5 1804 1407 (N41W50 L=220) 587 98 2 (1773/1359-1829/1444) -29.7 W45-W52 N37-N43
6 1510 1202 (N16W24 L=194) 214 94 0 (1496/1157-1528/1246) 90.0 W23-W24 N12-N18
7 878 1127 (S05E11 L=160) 229 89 0 ( 864/1082- 892/1170) -78.7 E12-E09 S07-S02
8 315 893 (S31E46 L=124) 1329 345 1 ( 230/ 780- 384/1045) 48.4 E57-E41 S39-S20
9 855 862 (S20E06 L=165) 423 151 0 ( 807/ 795- 889/ 907) -29.7 E09-E02 S23-S18
10 695 840 (S26E15 L=156) 234 63 1 ( 669/ 808- 717/ 869) -36.9 E17-E13 S27-S24
11 455 763 (S36E32 L=138) 676 220 0 ( 423/ 683- 512/ 851) -45.0 E35-E26 S40-S30
12 1599 726 (S07W43 L=214) 527 100 2 (1576/ 694-1645/ 770) -68.2 W40-W46 S09-S04
13 1454 450 (S26W47 L=218) 732 175 0 (1370/ 422-1532/ 486) 41.6 W42-W51 S30-S21
14 1107 338 (S45W32 L=203) 476 112 0 (1083/ 292-1139/ 388) -54.5 W30-W36 S47-S40
15 688 304 (S64E01 L=170) 1827 226 5 ( 607/ 269- 798/ 365) 0.0 E13-W13 S68-S60
16 1569 335 (S28W69 L=239) 1682 158 3 (1486/ 304-1631/ 363) 12.3 W58-W82 S31-S25
17 1173 280 (S46W42 L=213) 295 49 0 (1158/ 252-1187/ 303) -45.0 W38-W44 S48-S44
18 1262 230 (S46W55 L=226) 2283 164 6 (1184/ 191-1343/ 286) 20.6 W45-W66 S49-S42
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Download FITS filament maps as tar archive
» All Filament Data of 20230311 ...
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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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