|
|
|
|
| 20260618 - Filament data for 12 UTC |
|
Available data for 20260618: »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 1308 1645 (N46W16 L=252) 422 93 2 (1285/1596-1324/1677) -74.1 W13-W17 N41-N48
2 1629 1467 (N36W43 L=279) 1713 243 2 (1539/1429-1704/1514) -14.9 W35-W50 N33-N38
3 875 1418 (N24E14 L=222) 610 216 0 ( 832/1328- 923/1512) -50.7 E19-E09 N18-N29
4 637 1431 (N22E31 L=205) 226 86 1 ( 617/1382- 650/1467) -59.0 E33-E29 N19-N24
5 242 1377 (N14E65 L=170) 691 122 0 ( 225/1318- 264/1441) -58.0 E68-E61 N10-N18
6 348 1416 (N18E55 L=181) 391 93 1 ( 309/1390- 394/1434) -11.3 E59-E49 N16-N18
7 1011 1134 (N08E02 L=234) 221 99 0 ( 962/1109-1050/1174) -21.8 E05-W00 N06-N09
8 1608 1127 (N13W37 L=273) 308 95 1 (1589/1071-1618/1170) -80.5 W36-W38 N09-N15
9 821 1092 (N03E13 L=223) 632 207 2 ( 729/1041- 901/1121) -5.2 E18-E07 N01-N05
10 528 1008 (S05E31 L=204) 690 129 2 ( 480/ 949- 565/1063) -50.2 E34-E28 S07-S01
11 320 942 (S11E47 L=188) 525 135 1 ( 267/ 923- 388/ 969) 15.3 E52-E41 S12-S08
12 810 820 (S13E11 L=224) 402 125 1 ( 758/ 790- 866/ 858) -15.9 E14-E07 S14-S11
13 535 689 (S25E30 L=206) 357 106 0 ( 500/ 661- 584/ 728) -26.6 E32-E26 S26-S22
14 1470 671 (S16W33 L=269) 493 131 0 (1415/ 629-1515/ 721) 50.2 W29-W35 S18-S12
15 1089 657 (S21W08 L=244) 329 134 0 (1072/ 616-1119/ 718) -74.1 W06-W10 S23-S16
16 1049 550 (S28W07 L=243) 357 105 1 ( 997/ 528-1107/ 570) 0.0 W03-W11 S29-S26
17 1258 532 (S27W22 L=257) 283 37 1 (1245/ 506-1278/ 563) 90.0 W20-W23 S28-S24
18 464 509 (S38E40 L=196) 2532 423 4 ( 303/ 465- 672/ 560) 7.8 E65-E20 S44-S33
19 1575 442 (S30W52 L=287) 706 83 1 (1526/ 427-1626/ 461) 5.2 W46-W57 S31-S28
|
Download FITS filament maps as tar archive
» All Filament Data of 20260618 ...
|
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.
|
|
|
|