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| 20240918 - Filament data for 12 UTC |
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Available data for 20240918: »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 1020 1594 (N40W18 L= 33) 257 65 1 ( 989/1567-1052/1614) -45.0 W16-W20 N38-N41
2 461 1305 (N37E31 L=343) 312 97 1 ( 425/1270- 507/1340) 23.2 E34-E27 N35-N38
3 938 1280 (N23W02 L= 16) 197 50 2 ( 914/1254- 960/1298) -45.0 W00-W03 N22-N25
4 699 1241 (N27E14 L= 0) 314 117 1 ( 639/1226- 755/1259) -20.6 E18-E10 N25-N28
5 1212 1126 (N08W13 L= 27) 268 68 1 (1189/1095-1240/1150) 33.7 W11-W14 N06-N09
6 205 1036 (N25E59 L=315) 2037 216 3 ( 123/ 967- 292/1112) -22.2 E73-E50 N19-N30
7 1833 959 (S20W53 L= 67) 349 27 1 (1818/ 934-1848/ 986) -90.0 W50-W54 S21-S18
8 1354 842 (S12W14 L= 28) 356 117 2 (1331/ 797-1373/ 903) 51.3 W11-W16 S13-S08
9 1167 793 (S09W02 L= 16) 217 89 0 (1130/ 762-1206/ 821) 14.0 W00-W04 S10-S08
10 1087 740 (S10E04 L= 11) 247 93 2 (1036/ 707-1118/ 781) -45.0 E06-E01 S12-S08
11 1121 646 (S17E04 L= 10) 695 193 3 (1053/ 609-1193/ 705) 20.6 E08-W00 S18-S14
12 796 616 (S10E24 L=351) 603 171 2 ( 748/ 549- 838/ 696) 37.9 E28-E19 S13-S06
13 1673 578 (S39W33 L= 48) 340 55 0 (1653/ 553-1692/ 608) 36.9 W31-W35 S40-S37
14 611 454 (S16E42 L=332) 555 140 0 ( 586/ 403- 642/ 532) 38.7 E46-E36 S19-S11
15 542 468 (S14E46 L=328) 542 0 0 ( 513/ 442- 575/ 493) -63.4 E48-E44 S16-S12
16 1464 466 (S40W13 L= 28) 310 52 1 (1438/ 446-1487/ 490) 0.0 W11-W15 S41-S37
17 739 349 (S26E39 L=335) 499 81 1 ( 699/ 319- 772/ 383) 23.2 E42-E35 S27-S24
18 731 234 (S34E49 L=325) 2278 280 5 ( 646/ 128- 799/ 316) 57.0 E62-E44 S46-S26
19 1087 134 (S56E36 L=338) 868 109 1 (1033/ 116-1136/ 154) -54.5 E38-E31 S60-S51
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Download FITS filament maps as tar archive
» All Filament Data of 20240918 ...
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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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