|
|
|
|
| 20250407 - Filament data for 06 UTC |
|
Available data for 20250407: »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 1285 1795 (N52E11 L=238) 721 84 1 (1244/1764-1327/1826) 0.0 E15-E06 N49-N54
2 396 1628 (N13E64 L=185) 767 77 1 ( 362/1602- 428/1654) 45.0 E66-E61 N11-N15
3 1556 1620 (N48W19 L=268) 364 48 0 (1530/1598-1585/1640) -9.5 W16-W22 N47-N49
4 573 1489 (N08E40 L=208) 301 76 0 ( 548/1458- 606/1518) 76.0 E41-E39 N06-N10
5 1652 1447 (N38W30 L=278) 469 58 0 (1623/1424-1679/1471) 0.0 W27-W32 N36-N39
6 222 1360 (S06E66 L=182) 2139 232 4 ( 175/1285- 277/1463) 84.3 E73-E62 S10-N00
7 208 1203 (S15E62 L=187) 2280 316 6 ( 88/1130- 357/1261) 13.7 E84-E47 S20-S10
8 650 1192 (S07E26 L=223) 686 256 0 ( 595/1103- 749/1245) 56.3 E28-E19 S12-S02
9 1301 1203 (N11W10 L=259) 411 97 1 (1258/1167-1342/1243) -9.5 W07-W13 N09-N12
10 960 1100 (S04E05 L=243) 262 50 0 ( 936/1077- 979/1135) 90.0 E06-E04 S05-S01
11 440 966 (S24E35 L=214) 765 230 1 ( 396/ 884- 537/1033) 54.0 E37-E28 S29-S18
12 1271 803 (S11W20 L=268) 275 152 0 (1199/ 773-1330/ 825) 35.5 W16-W23 S14-S08
13 1371 674 (S15W30 L=279) 291 82 0 (1336/ 648-1388/ 708) 90.0 W28-W31 S16-S12
14 1643 567 (S12W54 L=303) 756 124 1 (1607/ 514-1671/ 611) -26.6 W49-W57 S14-S09
15 521 546 (S49E22 L=226) 1257 250 2 ( 403/ 516- 632/ 600) 4.8 E35-E11 S51-S45
16 1180 531 (S29W25 L=274) 530 98 1 (1140/ 508-1237/ 564) 0.0 W21-W29 S29-S27
17 1585 427 (S21W59 L=308) 995 100 2 (1540/ 392-1633/ 459) 51.3 W56-W63 S23-S18
18 1454 418 (S26W50 L=298) 573 62 2 (1420/ 389-1490/ 443) 18.4 W46-W52 S27-S24
19 1119 257 (S47W41 L=290) 1596 301 2 (1001/ 189-1250/ 325) 7.9 W27-W57 S49-S44
|
Download FITS filament maps as tar archive
» All Filament Data of 20250407 ...
|
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.
|
|
|
|