|
|
|
|
| 20241109 - Filament data for 08 UTC |
|
Available data for 20241109: »07 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 1471 1709 (N31W54 L=105) 387 72 2 (1456/1669-1495/1742) 26.6 W50-W58 N28-N32
2 1624 1543 (N17W55 L=105) 1851 372 2 (1482/1484-1761/1628) -41.4 W47-W66 N10-N25
3 1299 1535 (N25W31 L= 81) 2281 611 4 (1037/1434-1557/1589) -28.7 W13-W44 N13-N32
4 1218 1401 (N20W21 L= 71) 313 136 0 (1157/1384-1287/1420) -29.7 W17-W24 N17-N21
5 1853 1249 (S05W62 L=113) 436 66 1 (1836/1211-1865/1281) 45.0 W60-W64 S06-S03
6 246 1093 (N24E52 L=358) 802 127 2 ( 179/1059- 301/1127) -12.1 E60-E46 N21-N26
7 1556 1073 (S07W32 L= 82) 242 29 1 (1531/1055-1579/1095) -18.4 W30-W33 S07-S05
8 1564 993 (S11W31 L= 81) 416 0 0 (1499/ 969-1613/1031) -7.1 W26-W34 S12-S09
9 1104 837 (S09W00 L= 50) 537 119 3 (1061/ 794-1147/ 895) -80.5 E02-W02 S11-S05
10 678 765 (S03E26 L= 25) 2040 560 5 ( 516/ 594- 866/ 894) -53.6 E34-E18 S16-N05
11 217 841 (N10E59 L=351) 741 125 2 ( 167/ 806- 278/ 878) -24.4 E64-E53 N07-N13
12 972 767 (S10E09 L= 42) 246 67 1 ( 935/ 749-1001/ 793) 11.3 E11-E06 S10-S08
13 1216 594 (S26W01 L= 51) 1387 376 4 (1113/ 539-1350/ 717) -49.8 E04-W10 S29-S15
14 412 615 (S06E49 L= 1) 470 59 3 ( 378/ 592- 447/ 637) -36.9 E51-E45 S07-S04
15 963 337 (S36E24 L= 26) 3862 608 5 ( 822/ 152-1080/ 600) 43.2 E48-E13 S48-S18
16 390 550 (S10E54 L=357) 654 101 3 ( 344/ 515- 423/ 586) -51.3 E57-E49 S12-S07
17 557 551 (S13E41 L= 10) 385 44 3 ( 525/ 526- 581/ 574) -56.3 E43-E38 S14-S11
18 459 463 (S16E53 L=358) 2034 251 2 ( 405/ 339- 505/ 566) 33.7 E69-E46 S23-S09
|
Download FITS filament maps as tar archive
» All Filament Data of 20241109 ...
|
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.
|
|
|
|