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| 20230927 - Filament data for 08 UTC |
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Available data for 20230927: »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 1042 1690 (N45W27 L= 75) 975 151 3 ( 973/1652-1118/1714) -26.6 W20-W32 N43-N48
2 1383 1556 (N26W40 L= 89) 484 131 1 (1325/1536-1434/1573) -20.6 W35-W44 N23-N27
3 1579 1452 (N14W48 L= 97) 661 121 0 (1521/1434-1636/1473) -16.7 W43-W53 N12-N16
4 933 1277 (N23W02 L= 50) 268 68 1 ( 904/1251- 962/1307) 18.4 W00-W03 N21-N25
5 1646 1239 (N01W44 L= 92) 278 52 1 (1623/1205-1661/1269) 71.6 W42-W45 S01-N02
6 1840 1147 (S11W59 L=107) 1215 187 1 (1789/1070-1900/1208) 10.0 W51-W69 S13-S07
7 643 1065 (N18E22 L= 27) 665 190 1 ( 576/1011- 715/1133) 20.0 E26-E15 N16-N20
8 176 985 (N23E65 L=343) 2169 200 3 ( 150/ 891- 226/1067) -90.0 E69-E58 N17-N28
9 343 993 (N21E46 L= 2) 1044 223 3 ( 246/ 921- 398/1051) -37.6 E55-E41 N15-N25
10 979 1017 (N08E03 L= 46) 289 43 2 ( 949/ 992-1006/1041) -18.4 E04-W00 N06-N08
11 265 876 (N15E56 L=353) 985 164 3 ( 237/ 809- 300/ 956) -84.3 E58-E53 N10-N20
12 1510 915 (S13W25 L= 74) 286 99 2 (1482/ 881-1544/ 947) -45.0 W23-W27 S14-S10
13 1758 873 (S23W44 L= 92) 764 150 1 (1719/ 813-1801/ 931) 21.8 W39-W49 S25-S20
14 1805 812 (S29W49 L= 97) 383 65 0 (1781/ 785-1828/ 847) 31.0 W45-W51 S30-S27
15 192 769 (N10E69 L=340) 575 85 1 ( 176/ 733- 215/ 811) -59.0 E70-E66 N07-N12
16 1386 755 (S18W14 L= 62) 1047 374 1 (1220/ 731-1552/ 792) -20.0 W03-W25 S22-S13
17 535 502 (S12E46 L= 2) 1096 314 2 ( 488/ 379- 564/ 634) 45.0 E54-E38 S19-S04
18 845 595 (S13E22 L= 26) 211 53 1 ( 815/ 580- 877/ 606) -26.6 E23-E19 S14-S11
19 861 464 (S22E26 L= 22) 468 114 3 ( 839/ 406- 883/ 512) 60.3 E28-E23 S25-S18
20 462 382 (S18E61 L=348) 612 61 2 ( 440/ 354- 494/ 409) 63.4 E64-E57 S20-S16
21 644 281 (S29E53 L=355) 436 76 1 ( 625/ 249- 664/ 311) 24.0 E58-E49 S31-S26
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Download FITS filament maps as tar archive
» All Filament Data of 20230927 ...
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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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