|
|
|
|
| 20231228 - Filament data for 10 UTC |
|
Available data for 20231228: »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 1066 1767 (N48W07 L=282) 1012 140 3 (1020/1729-1129/1825) -41.2 W03-W12 N44-N53
2 1500 1659 (N37W42 L=317) 1827 436 3 (1279/1610-1670/1692) -7.7 W23-W61 N33-N40
3 1358 1487 (N25W24 L=299) 4321 984 3 ( 961/1254-1746/1606) -22.5 E02-W51 N09-N34
4 853 1488 (N27E10 L=265) 222 87 1 ( 823/1470- 898/1515) -31.0 E11-E06 N25-N29
5 983 1395 (N20E01 L=273) 280 74 0 ( 955/1361-1017/1425) -63.4 E03-W00 N18-N22
6 1321 1359 (N17W20 L=294) 259 86 0 (1309/1317-1336/1404) -90.0 W19-W21 N14-N19
7 586 1353 (N19E28 L=247) 373 91 0 ( 555/1335- 630/1389) -26.6 E30-E24 N18-N21
8 1792 1314 (N13W57 L=331) 1406 210 9 (1729/1241-1853/1384) -38.7 W52-W62 N08-N17
9 1559 1250 (N10W35 L=310) 325 75 1 (1546/1212-1578/1295) 78.7 W34-W36 N07-N12
10 740 1160 (N07E17 L=258) 392 121 0 ( 689/1119- 784/1208) -39.8 E20-E14 N04-N09
11 1754 895 (S12W50 L=324) 2167 305 5 (1679/ 761-1828/1041) 64.8 W44-W57 S20-S03
12 1414 739 (S21W24 L=299) 984 371 3 (1365/ 619-1475/ 877) 86.4 W21-W28 S28-S12
13 1877 785 (S18W67 L=342) 846 55 3 (1847/ 749-1900/ 818) -33.7 W62-W72 S20-S16
14 298 688 (S19E55 L=219) 532 111 3 ( 267/ 630- 340/ 727) 71.6 E58-E50 S22-S16
15 1089 591 (S29W03 L=277) 238 100 0 (1063/ 552-1121/ 632) 63.4 W00-W04 S32-S26
16 1665 541 (S34W51 L=325) 1701 248 2 (1556/ 480-1750/ 626) 31.0 W41-W57 S38-S28
17 1303 460 (S39W19 L=294) 449 96 1 (1270/ 433-1352/ 500) -33.7 W16-W23 S41-S36
18 960 425 (S41E08 L=267) 476 94 1 ( 910/ 405- 995/ 457) 15.9 E11-E04 S42-S38
|
Download FITS filament maps as tar archive
» All Filament Data of 20231228 ...
|
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.
|
|
|
|