|
|
|
|
| 20140113 - Filament data for 12 UTC |
|---|
|
Available data for 20140113: »07 UTC »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 1481 1435 (N24W29 L= 53) 891 229 2 (1392/1377-1585/1513) -26.6 W22-W36 N20-N28
2 1262 1454 (N23W13 L= 38) 277 107 0 (1203/1436-1318/1469) -7.1 W09-W17 N22-N24
3 351 1406 (N17E49 L=336) 313 80 0 ( 320/1362- 374/1434) 59.0 E50-E47 N14-N19
4 927 1347 (N15E08 L= 17) 231 75 0 ( 914/1312- 942/1389) -78.7 E08-E06 N12-N17
5 1329 1170 (N06W18 L= 42) 422 135 1 (1270/1132-1390/1231) -29.7 W13-W21 N03-N09
6 650 1184 (N04E24 L= 1) 228 74 0 ( 612/1168- 694/1202) 0.0 E26-E20 N02-N04
7 1041 1129 (N02W00 L= 25) 205 72 0 (1001/1112-1079/1149) 45.0 E01-W02 N00-N03
8 1939 1097 (N07W71 L= 95) 1269 166 2 (1908/1068-1968/1127) -10.3 W66-W77 N05-N08
9 486 1074 (S03E34 L=350) 333 55 1 ( 463/1045- 514/1101) 56.3 E35-E32 S04-S01
10 364 880 (S15E44 L=341) 1032 311 1 ( 269/ 815- 468/ 965) 25.2 E52-E35 S18-S09
11 788 925 (S11E14 L= 11) 189 88 0 ( 754/ 886- 831/ 944) 31.0 E16-E11 S13-S09
12 1796 681 (S19W59 L= 84) 3483 609 15 (1732/ 535-1861/ 890) 82.2 W52-W64 S28-S06
13 1917 827 (S09W71 L= 96) 1751 289 6 (1878/ 779-1955/ 884) 66.8 W65-W78 S12-S05
14 972 591 (S31E01 L= 23) 2645 612 4 ( 712/ 455-1243/ 747) 30.3 E21-W15 S41-S19
15 720 670 (S27E19 L= 6) 622 269 2 ( 596/ 595- 809/ 735) 29.4 E28-E12 S32-S22
16 1729 705 (S19W52 L= 76) 340 59 0 (1705/ 686-1751/ 726) 14.0 W49-W53 S19-S17
17 314 578 (S34E53 L=331) 1368 218 5 ( 280/ 515- 358/ 636) 69.4 E58-E48 S37-S29
18 427 605 (S32E42 L=342) 512 83 0 ( 391/ 590- 466/ 627) -18.4 E45-E38 S32-S30
19 1316 412 (S42W27 L= 52) 590 123 2 (1274/ 364-1363/ 460) 69.4 W23-W29 S45-S37
|
|
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.
|
|
|
|
