|
|
|
|
| 20250723 - Latest Filament data |
|
Available data for 20250723: »06 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 1343 1598 (N39W31 L=301) 873 188 0 (1275/1545-1421/1638) 17.4 W24-W40 N35-N41
2 945 1572 (N41E01 L=269) 549 157 1 ( 864/1549-1026/1588) -15.3 E07-W04 N38-N42
3 939 1368 (N27E03 L=267) 229 63 1 ( 903/1350- 970/1382) 0.0 E05-W00 N25-N27
4 1093 1275 (N20W06 L=276) 273 62 0 (1055/1257-1123/1295) -11.3 W03-W08 N18-N21
5 1607 1203 (N11W40 L=310) 879 231 1 (1521/1120-1669/1256) -41.6 W34-W44 N05-N14
6 546 1022 (N07E31 L=239) 1026 363 1 ( 435/ 873- 659/1134) -45.0 E38-E23 S01-N14
7 960 1087 (N09E03 L=267) 284 78 0 ( 948/1041- 981/1122) 68.2 E04-E02 N06-N11
8 316 674 (S14E54 L=216) 1769 339 4 ( 256/ 601- 375/ 766) 79.7 E60-E49 S18-S07
9 1768 640 (S27W56 L=326) 896 126 1 (1711/ 597-1823/ 681) 14.0 W50-W62 S29-S24
10 1454 656 (S22W26 L=296) 226 68 0 (1419/ 638-1489/ 674) -21.8 W23-W28 S23-S19
11 741 605 (S19E22 L=248) 314 64 1 ( 723/ 572- 770/ 640) 78.7 E22-E19 S21-S16
12 1109 566 (S24W02 L=272) 401 156 0 (1062/ 524-1179/ 596) 26.6 E01-W07 S27-S22
13 1626 514 (S34W44 L=314) 647 80 2 (1597/ 482-1662/ 543) 53.1 W40-W47 S36-S31
14 1609 428 (S41W46 L=316) 964 95 1 (1564/ 400-1655/ 453) -18.4 W39-W54 S43-S38
15 1495 372 (S44W36 L=306) 2780 312 5 (1350/ 344-1624/ 412) -5.2 W21-W55 S48-S39
16 1213 322 (S45W09 L=279) 427 52 1 (1184/ 302-1246/ 349) 18.4 W06-W12 S46-S42
17 1062 290 (S46E04 L=266) 686 74 1 (1020/ 267-1103/ 320) -15.9 E07-W00 S48-S43
18 962 274 (S47E13 L=257) 589 84 0 ( 928/ 253- 994/ 307) 33.7 E16-E09 S48-S43
19 787 218 (S51E34 L=236) 767 88 2 ( 752/ 196- 832/ 246) 14.0 E40-E27 S53-S48
|
Download FITS filament maps as tar archive
» All Filament Data of 20250723 ...
|
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.
|
|
|
|