|
|
|
|
| 20130508 - Filament data for 08 UTC |
|---|
|
Available data for 20130508: »08 UTC »09 UTC »10 UTC »11 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 1267 1765 (N52E07 L= 81) 383 78 0 (1233/1748-1305/1782) 0.0 E10-E02 N50-N54
2 1107 1608 (N34E11 L= 77) 1131 177 3 (1067/1524-1145/1686) -39.3 E16-E05 N28-N39
3 488 1483 (N11E47 L= 41) 450 121 0 ( 466/1425- 509/1540) -76.0 E48-E45 N06-N14
4 731 1427 (N13E28 L= 60) 286 92 1 ( 692/1397- 767/1455) -8.1 E31-E24 N11-N14
5 1737 1435 (N42W45 L=133) 491 58 1 (1706/1414-1765/1453) 20.6 W41-W49 N40-N44
6 1010 1325 (N13E08 L= 80) 410 125 5 ( 966/1275-1048/1371) -80.5 E10-E06 N10-N16
7 1404 1246 (N19W17 L=105) 932 256 2 (1354/1170-1480/1351) 70.3 W15-W20 N13-N27
8 1857 1288 (N36W61 L=149) 1031 127 0 (1819/1246-1884/1319) 36.9 W54-W66 N32-N38
9 1662 1106 (N18W38 L=126) 1041 149 2 (1628/1030-1703/1178) -36.9 W34-W42 N13-N21
10 1067 1130 (N04E00 L= 88) 263 85 2 (1024/1110-1106/1154) 45.0 E02-W01 N01-N05
11 1797 918 (N11W55 L=143) 1719 264 7 (1749/ 793-1839/1000) 90.0 W50-W59 N03-N16
12 448 812 (S29E33 L= 55) 428 111 0 ( 416/ 780- 479/ 868) 60.3 E35-E31 S32-S25
13 332 787 (S34E44 L= 44) 1017 181 5 ( 257/ 745- 405/ 838) -7.1 E53-E36 S36-S31
14 1437 622 (S16W36 L=124) 291 108 1 (1397/ 589-1493/ 645) 38.7 W34-W39 S17-S12
15 1004 598 (S29W10 L= 98) 391 114 1 ( 973/ 549-1048/ 643) -29.7 W07-W14 S30-S26
16 1273 540 (S25W29 L=117) 419 137 0 (1221/ 509-1330/ 563) 0.0 W25-W34 S25-S23
17 1616 446 (S20W61 L=149) 1266 245 4 (1535/ 354-1677/ 537) -82.4 W58-W65 S28-S13
18 1502 422 (S25W53 L=141) 626 165 0 (1470/ 376-1548/ 479) -81.9 W50-W57 S27-S20
19 932 253 (S56W24 L=112) 621 107 1 ( 878/ 233- 983/ 276) 11.3 W17-W28 S57-S53
|
|
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.
|
|
|
|
