|
|
|
|
| 20260116 - Filament data for 10 UTC |
|
Available data for 20260116: »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC »13 UTC »14 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 753 1733 (N40E28 L= 68) 286 28 0 ( 734/1714- 777/1751) 33.7 E29-E25 N38-N41
2 1195 1687 (N40W07 L=103) 327 47 0 (1173/1664-1223/1709) 45.0 W05-W09 N37-N41
3 372 1486 (N21E50 L= 46) 324 98 0 ( 356/1443- 392/1536) -80.5 E51-E48 N17-N23
4 300 1429 (N17E55 L= 41) 1855 235 5 ( 260/1311- 338/1511) -81.3 E61-E51 N09-N22
5 490 1262 (N07E35 L= 61) 536 170 0 ( 423/1215- 565/1317) 33.7 E39-E30 N03-N10
6 645 1181 (N02E24 L= 72) 614 105 0 ( 620/1127- 671/1237) -68.2 E25-E22 N00-N05
7 1779 1127 (N08W50 L=146) 1090 247 1 (1666/1100-1868/1179) 16.7 W40-W60 N05-N12
8 157 1071 (S05E64 L= 32) 530 91 1 ( 144/1026- 175/1119) 90.0 E65-E61 S07-S02
9 369 977 (S11E42 L= 53) 1329 219 5 ( 318/ 886- 406/1082) -74.7 E46-E39 S15-S04
10 461 1051 (S06E36 L= 60) 494 78 2 ( 429/1015- 504/1082) 21.8 E37-E32 S08-S04
11 258 981 (S10E52 L= 43) 305 37 0 ( 242/ 957- 271/1010) 56.3 E53-E51 S11-S08
12 268 938 (S13E52 L= 44) 949 183 1 ( 190/ 909- 315/1001) 17.1 E60-E47 S14-S09
13 504 928 (S13E32 L= 64) 306 115 0 ( 491/ 866- 516/ 986) -74.1 E33-E31 S16-S09
14 1919 957 (N00W67 L=163) 699 79 1 (1885/ 927-1951/ 979) 20.6 W62-W73 S02-N01
15 1046 807 (S17W03 L= 99) 251 94 0 ( 995/ 793-1092/ 825) 11.3 W00-W05 S18-S16
16 1883 743 (S13W69 L=165) 545 46 1 (1861/ 720-1901/ 770) 45.0 W66-W72 S14-S10
17 1432 675 (S22W30 L=125) 261 84 0 (1397/ 650-1469/ 703) 45.0 W27-W31 S24-S20
18 889 440 (S42E06 L= 90) 234 57 0 ( 865/ 420- 922/ 452) 26.6 E07-E02 S44-S41
|
|
Data will be available after one hour of observations. |
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.
|
|
|
|