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| 20241112 - Filament data for 09 UTC |
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Available data for 20241112: »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC »13 UTC »14 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 1530 1725 (N30W61 L= 71) 974 119 1 (1493/1678-1577/1759) 3.8 W55-W70 N27-N31
2 1898 1219 (S07W67 L= 78) 1532 148 5 (1864/1155-1928/1282) 60.3 W63-W74 S10-S03
3 1804 1178 (S07W55 L= 65) 1208 254 3 (1774/1083-1836/1271) 84.8 W50-W59 S12-S01
4 418 1215 (N27E35 L=335) 296 88 0 ( 394/1184- 451/1254) -59.0 E36-E32 N24-N29
5 1565 1190 (S00W36 L= 46) 227 132 0 (1526/1142-1613/1216) 7.1 W31-W39 S01-N00
6 203 1145 (N27E57 L=314) 488 64 1 ( 169/1117- 240/1169) 6.3 E61-E52 N26-N28
7 1303 1012 (S04W15 L= 26) 1959 587 3 (1098/ 835-1442/1149) -49.9 W04-W20 S16-N05
8 1580 1081 (S07W34 L= 44) 587 144 2 (1537/1013-1615/1135) -76.0 W31-W36 S10-S02
9 407 1112 (N21E37 L=333) 300 85 1 ( 375/1080- 437/1134) -45.0 E39-E34 N18-N22
10 1689 1063 (S10W42 L= 52) 346 87 1 (1660/1026-1720/1093) 18.4 W38-W44 S11-S09
11 744 1035 (N10E16 L=355) 602 173 2 ( 652/1011- 823/1062) -29.1 E20-E10 N07-N13
12 1647 978 (S14W37 L= 47) 615 184 3 (1581/ 931-1706/1031) 10.3 W31-W42 S16-S12
13 1731 800 (S27W42 L= 52) 1501 275 1 (1655/ 765-1841/ 876) -21.3 W34-W53 S30-S20
14 1542 732 (S26W25 L= 36) 469 115 1 (1526/ 679-1559/ 803) -90.0 W23-W26 S29-S21
15 888 707 (S12E15 L=355) 808 157 3 ( 818/ 663- 958/ 751) 0.0 E20-E10 S13-S08
16 749 466 (S23E31 L=339) 3433 811 7 ( 506/ 244-1000/ 690) 15.7 E66-E09 S33-S14
17 1530 537 (S39W23 L= 33) 2834 432 8 (1380/ 443-1629/ 660) 18.4 W09-W31 S45-S31
18 470 579 (S10E46 L=325) 388 154 0 ( 403/ 560- 529/ 616) 0.0 E51-E40 S11-S08
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Download FITS filament maps as tar archive
» All Filament Data of 20241112 ...
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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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