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| 20251003 - Filament data for 07 UTC |
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Available data for 20251003: »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
1 873 1829 (N62W27 L= 69) 477 59 1 ( 849/1804- 895/1853) 6.3 W23-W32 N59-N64
2 1224 1718 (N40W40 L= 82) 305 43 0 (1201/1690-1248/1745) -90.0 W39-W42 N37-N41
3 677 1711 (N60E03 L= 39) 436 113 0 ( 641/1676- 726/1732) 0.0 E08-W02 N58-N62
4 1516 1707 (N29W61 L=103) 658 59 2 (1488/1684-1548/1729) -63.4 W57-W64 N26-N30
5 1424 1532 (N23W41 L= 82) 1374 348 2 (1252/1489-1564/1587) -39.5 W32-W49 N16-N31
6 1856 1250 (S06W63 L=105) 4778 501 13 (1722/1084-1953/1464) -78.7 W54-W79 S17-N08
7 1084 1194 (N14W08 L= 49) 1242 483 8 ( 955/1089-1222/1275) -58.0 W01-W14 N05-N21
8 470 1217 (N31E31 L= 11) 533 161 0 ( 382/1198- 534/1239) -17.1 E38-E25 N29-N34
9 1248 1149 (N07W16 L= 57) 283 80 1 (1205/1132-1276/1177) -33.7 W13-W17 N06-N08
10 897 1141 (N16E04 L= 37) 439 171 0 ( 812/1112- 972/1157) -41.2 E08-W00 N12-N19
11 390 1113 (N27E39 L= 3) 505 108 2 ( 341/1094- 458/1131) -21.8 E43-E33 N24-N28
12 212 880 (N16E60 L=341) 662 111 3 ( 193/ 821- 227/ 935) 66.8 E62-E58 N12-N19
13 1160 872 (S05W03 L= 45) 395 48 1 (1127/ 841-1188/ 897) 0.0 W01-W05 S06-S03
14 918 791 (S04E12 L= 30) 485 174 1 ( 853/ 747-1002/ 842) 5.7 E16-E06 S04-S02
15 906 662 (S11E16 L= 25) 385 159 0 ( 865/ 585- 938/ 723) -90.0 E17-E15 S15-S06
16 460 392 (S17E59 L=343) 2311 292 3 ( 433/ 273- 487/ 530) 33.7 E76-E48 S26-S08
17 736 458 (S19E34 L= 8) 1043 294 2 ( 634/ 416- 854/ 520) -48.0 E38-E27 S24-S13
18 1521 481 (S41W18 L= 59) 839 88 2 (1477/ 446-1565/ 515) 0.0 W13-W21 S43-S38
19 1133 250 (S45E20 L= 21) 1718 347 3 (1005/ 159-1285/ 332) 5.5 E36-E04 S50-S42
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Download FITS filament maps as tar archive
» All Filament Data of 20251003 ...
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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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