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| 20240820 - Filament data for 12 UTC |
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Available data for 20240820: »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 1772 1516 (N17W73 L=111) 3498 188 4 (1721/1466-1836/1589) -73.3 W66-W86 N12-N22
2 1444 1503 (N26W40 L= 77) 444 127 0 (1412/1478-1498/1546) -51.3 W38-W44 N23-N29
3 1720 1444 (N15W60 L= 98) 1619 282 5 (1643/1350-1814/1542) -70.3 W57-W67 N07-N21
4 352 1376 (N40E48 L=350) 868 115 2 ( 309/1338- 412/1416) -21.0 E53-E40 N36-N42
5 795 1145 (N18E12 L= 25) 488 197 0 ( 734/1077- 840/1222) -68.2 E14-E09 N13-N23
6 1430 1089 (N02W26 L= 63) 386 128 0 (1403/1043-1472/1146) -71.6 W24-W27 N00-N06
7 1891 1060 (S11W65 L=102) 2937 222 3 (1834/ 961-1939/1136) -55.3 W58-W74 S18-S05
8 1828 1026 (S11W56 L= 93) 800 109 2 (1806/ 980-1855/1084) 71.6 W53-W59 S14-S07
9 149 916 (N12E71 L=326) 829 76 1 ( 116/ 889- 178/ 949) -16.7 E77-E66 N10-N14
10 267 844 (N07E56 L=341) 377 60 2 ( 253/ 813- 282/ 880) 63.4 E58-E54 N05-N09
11 330 714 (S01E53 L=344) 585 93 1 ( 308/ 668- 351/ 760) 78.7 E55-E50 S04-N01
12 1703 715 (S27W41 L= 78) 463 104 0 (1668/ 669-1740/ 752) 29.7 W37-W45 S29-S25
13 291 694 (S02E58 L=339) 634 145 1 ( 256/ 632- 329/ 749) -74.1 E60-E56 S06-N01
14 343 574 (S10E58 L=339) 2873 308 6 ( 254/ 518- 405/ 644) 14.6 E73-E50 S13-S05
15 567 529 (S15E40 L=357) 274 71 0 ( 529/ 509- 599/ 558) -36.9 E42-E38 S17-S13
16 444 520 (S15E51 L=346) 328 58 2 ( 426/ 487- 465/ 547) 45.0 E53-E48 S16-S12
17 909 386 (S31E22 L= 15) 1423 421 3 ( 774/ 288-1076/ 462) 15.4 E37-E08 S36-S27
18 1293 379 (S41W05 L= 42) 890 123 2 (1249/ 332-1324/ 433) 83.7 W00-W07 S45-S36
19 957 308 (S38E23 L= 15) 593 108 0 ( 922/ 261- 988/ 354) 33.7 E27-E18 S42-S35
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Download FITS filament maps as tar archive
» All Filament Data of 20240820 ...
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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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