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| 20231002 - Latest Filament data |
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Available data for 20231002: »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 1537 1648 (N25W59 L= 38) 708 42 0 (1506/1620-1562/1673) 76.0 W55-W62 N23-N27
2 1543 1534 (N19W50 L= 30) 330 59 1 (1525/1501-1559/1567) 26.6 W47-W53 N17-N20
3 1311 1512 (N25W33 L= 13) 341 107 0 (1259/1493-1357/1536) -56.3 W30-W35 N22-N28
4 1203 1411 (N23W22 L= 2) 523 187 0 (1115/1365-1275/1441) -45.0 W17-W25 N18-N26
5 247 1407 (N49E62 L=278) 485 63 0 ( 223/1381- 276/1425) 7.1 E66-E56 N47-N50
6 985 1330 (N25W06 L=346) 197 106 0 ( 965/1293-1006/1374) 38.7 W04-W09 N22-N26
7 990 1212 (N18W03 L=343) 923 396 2 ( 890/1084-1118/1341) -76.0 W00-W06 N07-N27
8 418 1261 (N35E36 L=304) 1141 190 2 ( 346/1211- 506/1313) -31.0 E43-E28 N31-N40
9 586 1140 (N24E24 L=316) 327 72 2 ( 554/1109- 624/1171) -51.3 E25-E21 N21-N26
10 177 1021 (N25E64 L=275) 690 84 1 ( 157/ 985- 195/1062) 53.1 E67-E61 N23-N27
11 209 898 (N18E62 L=278) 3368 334 8 ( 142/ 749- 250/1053) 60.9 E70-E54 N08-N26
12 1473 890 (S13W22 L= 2) 914 340 1 (1407/ 764-1538/1052) 38.7 W15-W30 S18-S06
13 1751 939 (S20W44 L= 24) 877 189 3 (1732/ 849-1768/1031) 59.0 W41-W47 S24-S14
14 716 918 (N08E20 L=319) 502 173 0 ( 654/ 863- 780/ 981) -60.9 E22-E17 N04-N13
15 421 892 (N13E41 L=299) 313 62 2 ( 386/ 865- 448/ 912) -36.9 E43-E39 N11-N14
16 1211 642 (S20W00 L=340) 275 100 1 (1192/ 616-1250/ 684) -80.5 W00-W02 S22-S16
17 1475 618 (S30W17 L=356) 544 105 1 (1447/ 572-1511/ 652) 33.7 W13-W19 S32-S27
18 968 434 (S26E21 L=319) 246 77 0 ( 951/ 397- 984/ 474) 38.7 E23-E18 S28-S23
19 963 267 (S39E31 L=309) 627 134 0 ( 936/ 212- 986/ 331) 55.0 E35-E27 S43-S33
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Download FITS filament maps as tar archive
» All Filament Data of 20231002 ...
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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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