|
|
|
|
| 20140802 - Filament data for 07 UTC |
|---|
|
Available data for 20140802: »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 1311 1658 (N42W34 L=287) 276 81 0 (1275/1646-1355/1670) -26.6 W31-W37 N40-N43
2 1523 1539 (N30W45 L=298) 437 90 2 (1484/1503-1551/1559) -53.1 W42-W47 N27-N31
3 996 1335 (N25W02 L=255) 254 65 1 ( 969/1307-1030/1362) -53.1 W00-W04 N23-N27
4 1814 1308 (N11W64 L=317) 1344 225 4 (1766/1259-1859/1353) 14.0 W57-W70 N08-N13
5 539 1149 (N18E31 L=223) 1794 496 6 ( 375/1048- 706/1260) -33.7 E43-E19 N10-N26
6 1846 1225 (N05W65 L=318) 526 81 3 (1829/1177-1864/1257) 78.7 W63-W67 N02-N07
7 1310 1168 (N11W20 L=273) 396 140 2 (1253/1112-1351/1222) 32.0 W15-W23 N08-N13
8 1172 1130 (N10W10 L=263) 244 115 0 (1110/1110-1228/1155) -29.7 W06-W13 N08-N12
9 1844 1036 (S06W60 L=313) 1281 200 0 (1820/ 950-1865/1100) 71.6 W57-W63 S11-S02
10 374 1002 (N10E44 L=209) 635 181 0 ( 324/ 925- 425/1055) -48.8 E48-E40 N05-N13
11 1887 979 (S10W65 L=318) 556 111 2 (1868/ 945-1909/1010) -51.3 W62-W68 S13-S08
12 1600 738 (S20W35 L=288) 2366 449 9 (1455/ 596-1696/ 896) 41.6 W24-W43 S27-S11
13 901 774 (S08E11 L=243) 197 45 1 ( 881/ 752- 929/ 793) 18.4 E11-E08 S09-S06
14 972 695 (S14E07 L=246) 844 328 1 ( 843/ 621-1069/ 786) 23.6 E16-W00 S17-S08
15 791 708 (S11E18 L=235) 344 83 1 ( 755/ 677- 815/ 752) 63.4 E20-E16 S12-S08
16 661 696 (S11E27 L=226) 506 130 5 ( 616/ 653- 717/ 749) -56.3 E29-E23 S13-S06
17 1269 593 (S24W11 L=264) 226 52 1 (1253/ 570-1289/ 621) -90.0 W09-W12 S26-S22
18 538 583 (S17E39 L=215) 656 144 2 ( 488/ 546- 584/ 619) -51.3 E41-E35 S19-S14
|
|
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.
|
|
|
|
