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| 20231123 - Filament data for 07 UTC |
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Available data for 20231123: »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 1395 1743 (N38W50 L= 67) 513 53 1 (1374/1702-1412/1772) 26.6 W45-W54 N35-N39
2 1555 1714 (N32W63 L= 80) 1301 131 0 (1497/1688-1599/1749) -8.7 W55-W70 N29-N34
3 600 1697 (N56E21 L=356) 1462 116 2 ( 558/1637- 653/1742) 71.6 E27-E14 N50-N60
4 909 1596 (N39W05 L= 23) 1604 273 2 ( 795/1530-1043/1647) -42.9 E02-W12 N31-N45
5 1308 1596 (N30W33 L= 50) 308 62 0 (1271/1574-1338/1614) -45.0 W30-W34 N28-N31
6 1034 1390 (N23W08 L= 25) 451 70 2 ( 998/1361-1072/1412) 0.0 W05-W10 N21-N24
7 363 1270 (N29E41 L=336) 1528 341 2 ( 264/1180- 453/1380) -38.7 E54-E33 N21-N37
8 1170 1290 (N14W14 L= 31) 660 139 0 (1096/1255-1232/1332) -49.4 W10-W17 N11-N18
9 1898 1121 (S10W67 L= 84) 1465 160 0 (1876/1040-1925/1196) 41.6 W62-W72 S14-S06
10 532 1170 (N19E28 L=349) 245 47 0 ( 516/1135- 551/1192) -90.0 E29-E26 N17-N20
11 198 1071 (N19E59 L=318) 2589 297 5 ( 119/ 991- 314/1179) -26.6 E73-E47 N13-N27
12 420 1096 (N17E37 L=340) 783 126 1 ( 373/1058- 472/1134) 0.0 E41-E32 N15-N19
13 451 805 (S00E40 L=337) 488 70 1 ( 411/ 781- 494/ 832) -9.5 E42-E36 S02-N01
14 529 761 (S04E36 L=342) 237 57 1 ( 512/ 729- 544/ 790) 36.9 E37-E33 S06-S02
15 1055 675 (S19E05 L= 12) 330 149 1 (1037/ 612-1071/ 755) 58.0 E07-E02 S22-S14
16 1303 634 (S27W10 L= 27) 295 45 1 (1281/ 601-1322/ 664) -90.0 W08-W11 S28-S24
17 467 587 (S13E46 L=331) 436 148 0 ( 436/ 520- 497/ 649) 37.9 E50-E41 S17-S10
18 514 528 (S18E45 L=332) 290 24 0 ( 494/ 512- 539/ 546) -45.0 E46-E43 S18-S16
19 327 450 (S19E70 L=307) 1918 75 1 ( 286/ 412- 368/ 486) -16.7 E76-E64 S22-S16
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Download FITS filament maps as tar archive
» All Filament Data of 20231123 ...
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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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