|
|
|
|
| 20260616 - Filament data for 11 UTC |
|
Available data for 20260616: »06 UTC »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 1224 1557 (N38W08 L=271) 268 52 1 (1199/1539-1257/1579) 14.0 W06-W10 N35-N39
2 353 1460 (N20E56 L=206) 821 187 0 ( 334/1386- 373/1546) -51.3 E60-E51 N15-N25
3 1289 1486 (N33W13 L=276) 609 124 2 (1251/1424-1320/1531) -60.3 W10-W15 N29-N36
4 523 1450 (N21E40 L=222) 379 76 1 ( 505/1423- 545/1494) -51.3 E42-E38 N19-N24
5 1778 1376 (N31W58 L=320) 805 103 2 (1756/1321-1801/1420) 66.8 W55-W62 N27-N34
6 320 1276 (N08E52 L=210) 302 116 0 ( 303/1234- 348/1329) -35.5 E55-E48 N06-N11
7 425 1168 (N03E41 L=222) 693 150 2 ( 358/1137- 491/1193) 0.0 E46-E35 N01-N04
8 1563 1159 (N15W34 L=296) 264 67 0 (1544/1125-1588/1183) 53.1 W32-W35 N12-N16
9 192 1084 (S05E62 L=200) 832 100 2 ( 150/1037- 224/1118) -16.7 E68-E57 S07-S02
10 1405 1071 (N08W23 L=286) 411 107 1 (1389/1006-1436/1109) -80.5 W21-W25 N04-N10
11 925 1014 (S01E06 L=257) 263 59 0 ( 910/ 979- 939/1048) -71.6 E06-E04 S02-N01
12 406 925 (S12E40 L=223) 699 203 0 ( 340/ 887- 484/ 996) -20.0 E45-E33 S13-S08
13 680 740 (S20E19 L=244) 600 209 0 ( 655/ 677- 719/ 819) 84.3 E20-E16 S24-S14
14 1047 726 (S17W05 L=267) 421 106 1 (1006/ 687-1092/ 768) 50.2 W02-W07 S19-S13
15 891 619 (S26E04 L=259) 291 62 1 ( 863/ 591- 920/ 648) 63.4 E05-E02 S27-S23
16 706 611 (S28E17 L=246) 263 67 0 ( 672/ 596- 741/ 630) 0.0 E19-E14 S29-S27
17 316 585 (S36E54 L=208) 991 140 2 ( 247/ 547- 378/ 619) -6.7 E65-E47 S37-S32
18 1377 509 (S27W31 L=294) 276 36 1 (1355/ 489-1401/ 529) 33.7 W30-W33 S28-S25
19 1235 482 (S31W22 L=284) 585 164 0 (1159/ 464-1309/ 512) 0.0 W15-W27 S32-S29
|
Download FITS filament maps as tar archive
» All Filament Data of 20260616 ...
|
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.
|
|
|
|