|
|
|
|
| 20150704 - Filament data for 11 UTC |
|
Available data for 20150704: »04 UTC »05 UTC »06 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
1 882 1691 (N48E15 L=122) 2860 425 7 ( 776/1564-1023/1753) 10.3 E23-E01 N37-N54
2 1448 1662 (N47W37 L=174) 715 116 1 (1404/1637-1487/1683) 16.7 W32-W42 N44-N48
3 1305 1607 (N42W22 L=159) 760 140 2 (1254/1553-1343/1659) 53.1 W17-W27 N38-N46
4 1583 1605 (N42W48 L=185) 473 81 1 (1561/1577-1611/1626) -33.7 W45-W50 N39-N43
5 1664 1549 (N37W53 L=190) 466 69 1 (1636/1535-1693/1568) -11.3 W49-W55 N36-N38
6 459 1425 (N27E43 L= 94) 678 207 3 ( 441/1341- 482/1512) -65.6 E45-E39 N21-N32
7 1319 1433 (N29W20 L=157) 292 64 1 (1291/1401-1342/1466) -76.0 W18-W21 N27-N31
8 1002 1307 (N21E02 L=135) 423 83 0 ( 967/1281-1061/1336) -31.0 E04-W01 N19-N22
9 926 1225 (N15E07 L=130) 605 265 2 ( 797/1201-1063/1255) 3.4 E15-W02 N13-N17
10 880 1141 (N10E09 L=128) 382 169 0 ( 832/1088- 980/1195) -31.0 E12-E02 N06-N13
11 1597 1072 (N06W38 L=175) 379 86 1 (1566/1036-1635/1110) -45.0 W35-W40 N04-N08
12 1294 896 (S04W17 L=154) 300 95 0 (1282/ 843-1312/ 945) 90.0 W16-W18 S07-S01
13 317 803 (S13E50 L= 87) 1184 316 6 ( 237/ 726- 378/ 903) -42.3 E57-E44 S17-S07
14 274 782 (S15E54 L= 83) 371 62 0 ( 254/ 760- 298/ 812) -33.7 E56-E52 S15-S12
15 1010 685 (S18E00 L=137) 545 149 1 ( 975/ 621-1040/ 764) 84.3 E02-W01 S22-S12
16 493 395 (S42E45 L= 93) 1514 246 2 ( 429/ 355- 541/ 460) 33.7 E52-E37 S45-S35
17 1663 445 (S35W55 L=192) 542 145 1 (1630/ 436-1705/ 460) -6.3 W50-W59 S36-S33
18 1323 374 (S41W26 L=163) 1633 350 3 (1182/ 328-1498/ 429) 13.5 W15-W40 S44-S36
|
|
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.
|
|
|
|