|
|
|
|
| 20251113 - Filament data for 07 UTC |
|
Available data for 20251113: »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC »13 UTC »14 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 782 1660 (N48E00 L=220) 285 31 1 ( 757/1636- 799/1679) 0.0 E02-W01 N45-N49
2 1586 1613 (N23W56 L=276) 1020 158 4 (1532/1559-1644/1666) -54.5 W52-W59 N19-N26
3 588 1624 (N51E19 L=202) 404 71 0 ( 553/1599- 612/1655) 31.0 E22-E16 N49-N53
4 1229 1597 (N31W29 L=249) 1971 412 7 (1051/1542-1420/1633) -27.6 W16-W39 N23-N35
5 1680 1529 (N16W59 L=279) 954 177 4 (1617/1464-1728/1588) 15.5 W49-W67 N13-N18
6 1554 1518 (N19W47 L=268) 286 85 1 (1511/1499-1588/1538) -45.0 W44-W49 N16-N20
7 1662 1328 (N06W47 L=268) 930 191 2 (1580/1299-1717/1361) -33.7 W41-W52 N02-N08
8 593 1162 (N20E23 L=198) 1276 398 7 ( 405/1102- 751/1229) -27.6 E36-E13 N13-N27
9 127 1103 (N25E68 L=152) 729 69 1 ( 97/1074- 159/1128) -21.8 E75-E63 N23-N27
10 321 951 (N13E47 L=174) 499 110 4 ( 287/ 919- 361/ 994) -33.7 E49-E42 N11-N16
11 1428 931 (S11W21 L=242) 333 84 2 (1375/ 903-1458/ 957) -21.8 W18-W23 S12-S09
12 1399 824 (S16W17 L=238) 334 114 1 (1361/ 801-1441/ 845) -11.3 W15-W20 S18-S15
13 867 697 (S12E16 L=204) 530 160 0 ( 838/ 640- 907/ 763) 76.0 E17-E13 S16-S08
14 1875 739 (S35W61 L=282) 1053 120 0 (1816/ 718-1934/ 756) -7.1 W52-W76 S36-S33
15 1479 633 (S30W20 L=241) 707 190 0 (1390/ 578-1531/ 702) 15.3 W13-W24 S32-S26
16 840 436 (S27E26 L=194) 1915 462 3 ( 667/ 356-1044/ 551) 5.5 E41-E10 S29-S24
17 1222 339 (S44E05 L=216) 1764 364 1 (1055/ 283-1361/ 436) 2.2 E19-W08 S47-S40
18 400 392 (S21E64 L=156) 610 33 0 ( 380/ 357- 419/ 418) 26.6 E69-E60 S23-S19
|
Download FITS filament maps as tar archive
» All Filament Data of 20251113 ...
|
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.
|
|
|
|