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| 20230928 - Filament data for 07 UTC |
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Available data for 20230928: »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 1021 1772 (N52W33 L= 68) 363 57 2 ( 999/1742-1041/1800) 23.2 W29-W36 N49-N54
2 1169 1753 (N45W41 L= 77) 782 83 1 (1132/1725-1213/1778) -38.7 W36-W45 N42-N46
3 1692 1524 (N14W63 L= 99) 687 111 1 (1631/1506-1739/1549) -13.0 W56-W69 N12-N15
4 1097 1351 (N23W14 L= 49) 295 76 1 (1066/1326-1127/1383) 11.3 W11-W16 N21-N25
5 1765 1300 (S00W57 L= 92) 589 110 1 (1738/1242-1786/1355) 63.4 W55-W58 S03-N03
6 885 1318 (N27E00 L= 36) 208 62 0 ( 870/1281- 899/1347) 63.4 E01-W01 N24-N28
7 830 1147 (N19E08 L= 28) 678 182 1 ( 770/1084- 890/1216) 24.4 E13-E02 N16-N21
8 1177 1124 (N08W11 L= 47) 254 81 0 (1153/1102-1199/1158) 45.0 W09-W12 N07-N10
9 280 978 (N21E52 L=344) 2634 521 9 ( 229/ 735- 356/1149) -77.0 E56-E47 N05-N31
10 462 1061 (N22E34 L= 1) 660 190 1 ( 373/1009- 523/1093) -32.5 E41-E30 N18-N25
11 1860 939 (S24W57 L= 92) 728 121 1 (1825/ 893-1881/ 993) 18.4 W51-W60 S25-S20
12 389 920 (N16E43 L=353) 265 58 2 ( 367/ 895- 408/ 943) 71.6 E45-E41 N14-N17
13 1539 844 (S18W26 L= 62) 1151 367 2 (1373/ 821-1706/ 875) -20.6 W14-W39 S22-S12
14 1113 747 (S11E02 L= 33) 238 82 0 (1091/ 712-1130/ 782) 36.9 E04-W00 S12-S09
15 1832 764 (S34W53 L= 88) 592 83 0 (1793/ 748-1876/ 779) -21.0 W47-W60 S36-S31
16 687 549 (S12E33 L= 2) 1088 398 2 ( 622/ 409- 753/ 714) 38.7 E44-E23 S19-S03
17 480 339 (S22E64 L=332) 1773 129 6 ( 441/ 292- 524/ 393) 41.6 E73-E56 S25-S17
18 562 330 (S24E56 L=340) 496 89 0 ( 523/ 313- 590/ 358) -21.8 E58-E50 S25-S22
19 761 307 (S30E41 L=354) 638 112 0 ( 733/ 255- 803/ 345) 22.6 E47-E35 S33-S27
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Download FITS filament maps as tar archive
» All Filament Data of 20230928 ...
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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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