|
|
|
|
| 20150510 - Filament data for 10 UTC |
|
Available data for 20150510: »06 UTC »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC »13 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 662 1785 (N35E51 L= 94) 1076 229 1 ( 619/1711- 707/1846) -59.7 E56-E48 N28-N40
2 1051 1733 (N42E21 L=125) 980 136 0 (1021/1678-1077/1786) -37.9 E25-E16 N37-N45
3 1533 1615 (N49W23 L=169) 508 49 2 (1506/1592-1559/1638) 11.3 W20-W25 N47-N51
4 701 1605 (N23E37 L=109) 331 50 0 ( 675/1579- 723/1634) 90.0 E37-E35 N21-N25
5 452 1546 (N14E53 L= 93) 2432 511 8 ( 367/1462- 530/1614) -20.2 E63-E44 N08-N18
6 619 1501 (N15E38 L=108) 448 79 1 ( 596/1456- 650/1536) -68.2 E39-E35 N12-N17
7 761 1435 (N14E26 L=120) 334 173 1 ( 678/1405- 817/1482) 58.0 E31-E23 N10-N18
8 894 1390 (N15E17 L=129) 480 118 2 ( 847/1365- 937/1430) 21.8 E19-E13 N12-N17
9 741 1313 (N07E23 L=122) 337 71 3 ( 722/1273- 755/1351) -78.7 E24-E21 N04-N09
10 998 1293 (N11E08 L=138) 214 23 0 ( 982/1273-1016/1316) -33.7 E09-E06 N10-N12
11 1127 1052 (N01W05 L=151) 340 64 2 (1096/1023-1152/1082) 71.6 W03-W06 S01-N02
12 1565 859 (N01W37 L=182) 375 113 1 (1523/ 806-1608/ 905) 66.8 W35-W38 S03-N04
13 932 830 (S16E01 L=145) 267 59 1 ( 899/ 795- 961/ 855) -56.3 E02-W01 S18-S15
14 1735 526 (S13W66 L=212) 1628 210 2 (1666/ 465-1805/ 593) 45.0 W61-W72 S17-S07
15 1515 515 (S20W46 L=192) 278 76 1 (1479/ 500-1547/ 540) 21.8 W43-W48 S21-S17
16 663 489 (S46E11 L=134) 322 94 1 ( 618/ 475- 716/ 508) 12.5 E15-E06 S46-S44
17 686 395 (S52E07 L=139) 294 82 1 ( 640/ 382- 725/ 409) 7.1 E11-E03 S53-S50
18 1144 366 (S39W30 L=175) 1213 287 0 (1024/ 337-1289/ 398) 13.4 W19-W40 S42-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.
|
|
|
|