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| 20230407 - Latest Filament data |
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Available data for 20230407: »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
1 958 1828 (N42E37 L=136) 1159 212 2 ( 868/1762-1045/1877) -7.4 E49-E26 N39-N43
2 466 1648 (N16E59 L=114) 2312 326 2 ( 338/1608- 595/1689) 7.6 E76-E46 N11-N18
3 1563 1571 (N45W20 L=193) 386 111 0 (1521/1524-1602/1608) -24.0 W15-W24 N42-N46
4 835 1244 (N01E16 L=157) 709 204 1 ( 782/1147- 907/1326) -22.6 E21-E09 S02-N04
5 230 1128 (S20E58 L=115) 436 53 3 ( 210/1099- 253/1164) -76.0 E60-E55 S21-S17
6 326 1118 (S19E48 L=125) 354 68 0 ( 307/1087- 346/1151) 53.1 E49-E46 S20-S16
7 162 1051 (S26E66 L=107) 2634 201 1 ( 126/ 966- 198/1139) 63.4 E73-E61 S31-S19
8 1738 1099 (N20W43 L=216) 965 128 0 (1678/1054-1782/1139) 0.0 W36-W47 N18-N21
9 911 1070 (S07E07 L=166) 307 68 0 ( 882/1036- 939/1103) 78.7 E08-E06 S09-S04
10 526 816 (S31E26 L=147) 331 111 0 ( 476/ 783- 573/ 846) 40.6 E29-E22 S34-S28
11 1763 783 (N04W55 L=228) 348 58 1 (1744/ 751-1777/ 818) -45.0 W52-W56 N02-N05
12 1097 684 (S23W15 L=188) 759 218 0 (1003/ 629-1196/ 727) 54.0 W10-W19 S28-S17
13 1368 633 (S17W32 L=205) 1294 281 3 (1227/ 599-1505/ 665) 34.5 W24-W40 S22-S11
14 853 582 (S36W04 L=177) 388 55 1 ( 829/ 559- 883/ 608) 76.0 W01-W05 S38-S34
15 809 533 (S41W02 L=176) 337 65 1 ( 789/ 503- 835/ 571) -31.0 W00-W05 S42-S38
16 1620 451 (S18W62 L=235) 492 52 1 (1597/ 428-1648/ 476) 76.0 W59-W63 S19-S15
17 1543 444 (S21W55 L=228) 347 62 0 (1519/ 411-1566/ 473) -68.2 W53-W57 S23-S18
18 530 396 (S62E20 L=153) 807 140 0 ( 474/ 349- 577/ 456) -23.2 E28-E13 S65-S58
19 841 429 (S47W09 L=182) 261 40 0 ( 818/ 409- 861/ 449) -14.0 W07-W11 S47-S45
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Download FITS filament maps as tar archive
» All Filament Data of 20230407 ...
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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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