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| 20220912 - Filament data for 06 UTC |
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Available data for 20220912: »05 UTC »06 UTC »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 857 1738 (N57W14 L= 39) 463 82 1 ( 831/1715- 900/1760) -51.3 W10-W17 N54-N59
2 1586 1677 (N27W67 L= 92) 467 48 2 (1557/1662-1616/1692) -26.6 W63-W71 N25-N28
3 1504 1592 (N26W52 L= 77) 766 182 1 (1431/1549-1573/1626) -45.0 W46-W55 N21-N29
4 521 1558 (N54E28 L=358) 386 55 1 ( 485/1538- 546/1582) -14.0 E32-E24 N51-N55
5 1415 1467 (N22W37 L= 63) 254 39 0 (1392/1444-1434/1482) -63.4 W35-W39 N20-N23
6 1325 1428 (N22W30 L= 55) 472 132 0 (1266/1402-1381/1446) -23.2 W25-W33 N19-N24
7 1115 1248 (N18W11 L= 36) 890 230 2 (1008/1180-1190/1313) -61.4 W06-W14 N12-N24
8 409 1137 (N27E39 L=346) 255 48 1 ( 387/1115- 437/1152) 0.0 E40-E36 N25-N28
9 1806 1113 (S09W55 L= 80) 346 47 0 (1787/1088-1824/1136) -76.0 W52-W56 S11-S07
10 839 1089 (N15E09 L= 16) 278 79 1 ( 817/1050- 859/1126) 45.0 E10-E07 N13-N17
11 1870 906 (S24W59 L= 84) 3139 493 3 (1823/ 797-1930/1047) 75.1 W52-W70 S31-S16
12 430 994 (N18E39 L=346) 313 72 1 ( 417/ 955- 443/1035) -90.0 E39-E37 N15-N20
13 1149 932 (S01W05 L= 30) 949 219 4 (1097/ 835-1205/1021) 37.9 W00-W10 S06-N02
14 1317 689 (S20W09 L= 34) 429 140 0 (1249/ 651-1364/ 711) -35.5 W04-W11 S23-S17
15 1221 514 (S28E01 L= 24) 634 189 0 (1141/ 482-1308/ 558) -5.2 E06-W05 S29-S26
16 1510 518 (S37W20 L= 45) 729 87 1 (1474/ 474-1544/ 553) 38.7 W16-W22 S40-S34
17 1374 399 (S42W07 L= 32) 402 62 1 (1351/ 376-1407/ 424) 21.8 W04-W09 S43-S39
18 1276 351 (S43E02 L= 23) 345 52 0 (1260/ 326-1298/ 386) 80.5 E03-W00 S45-S39
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Download FITS filament maps as tar archive
» All Filament Data of 20220912 ...
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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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