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| 20251001 - Filament data for 12 UTC |
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Available data for 20251001: »06 UTC »07 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
1 631 1689 (N60E09 L= 56) 1866 368 4 ( 474/1602- 766/1789) 5.4 E30-W12 N56-N64
2 1207 1353 (N20W20 L= 85) 569 163 2 (1119/1315-1287/1369) -29.1 W15-W24 N16-N22
3 1837 1080 (S14W55 L=120) 3451 455 7 (1791/ 885-1887/1292) 48.0 W46-W65 S23-S02
4 1902 1159 (S12W66 L=131) 1893 263 2 (1861/1027-1945/1259) -78.7 W62-W71 S21-S06
5 1499 1191 (N03W32 L= 97) 337 109 0 (1484/1141-1510/1249) 51.3 W29-W33 N00-N05
6 247 1126 (N30E53 L= 12) 480 92 0 ( 205/1106- 292/1148) -16.7 E58-E48 N28-N32
7 796 1045 (N13E12 L= 53) 975 396 3 ( 635/ 986- 923/1118) -12.5 E22-E04 N09-N16
8 1751 1018 (S14W45 L=110) 1190 191 5 (1704/ 963-1790/1091) 32.0 W40-W50 S17-S11
9 179 1048 (N27E62 L= 3) 456 90 0 ( 138/1030- 224/1072) -14.0 E68-E56 N25-N28
10 541 990 (N16E30 L= 36) 387 148 0 ( 467/ 957- 607/1015) -33.7 E34-E25 N13-N19
11 890 963 (N07E09 L= 56) 237 59 1 ( 858/ 944- 917/ 994) -33.7 E10-E07 N05-N08
12 254 833 (N13E57 L= 8) 892 117 2 ( 223/ 770- 276/ 887) 74.1 E60-E53 N09-N16
13 743 817 (N02E21 L= 44) 217 66 2 ( 704/ 801- 766/ 836) -63.4 E22-E19 N00-N04
14 816 683 (S07E21 L= 45) 260 51 0 ( 778/ 671- 846/ 699) -14.0 E22-E18 S08-S06
15 1728 590 (S41W39 L=104) 2288 222 4 (1648/ 534-1789/ 677) 14.0 W30-W46 S46-S35
16 574 649 (S04E36 L= 29) 336 69 1 ( 538/ 628- 599/ 675) -33.7 E38-E34 S05-S02
17 469 429 (S15E55 L= 10) 594 71 2 ( 432/ 398- 498/ 456) -53.1 E58-E51 S17-S13
18 497 362 (S20E58 L= 8) 1077 222 2 ( 409/ 316- 588/ 418) -36.0 E63-E49 S23-S14
19 1254 347 (S41E06 L= 59) 1287 189 3 (1180/ 305-1336/ 398) 4.4 E12-W01 S43-S38
20 962 181 (S45E38 L= 27) 827 86 1 ( 921/ 155-1005/ 213) 5.2 E44-E33 S47-S42
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Download FITS filament maps as tar archive
» All Filament Data of 20251001 ...
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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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