|
|
|
|
| 20150704 - Filament data for 13 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
1 887 1697 (N49E15 L=121) 3298 533 5 ( 787/1564-1004/1783) 56.3 E22-E04 N38-N57
2 1456 1664 (N47W38 L=174) 690 131 1 (1412/1637-1498/1684) 16.7 W32-W42 N44-N48
3 1317 1604 (N42W23 L=159) 815 156 3 (1276/1546-1350/1660) 56.3 W19-W27 N37-N46
4 1593 1605 (N42W49 L=184) 495 54 1 (1568/1579-1619/1625) -33.7 W46-W50 N39-N43
5 301 1548 (N34E63 L= 73) 703 105 3 ( 278/1521- 329/1569) 26.6 E65-E59 N31-N35
6 1673 1549 (N37W54 L=190) 442 74 0 (1647/1535-1701/1562) 9.5 W50-W56 N36-N38
7 467 1454 (N29E43 L= 93) 439 149 0 ( 456/1385- 488/1509) -82.9 E44-E41 N24-N32
8 1334 1430 (N29W21 L=157) 293 50 1 (1313/1402-1355/1464) -76.0 W20-W22 N27-N31
9 1021 1306 (N21E01 L=135) 429 79 1 ( 984/1277-1077/1337) -45.0 E03-W02 N18-N22
10 1014 1228 (N16E01 L=135) 367 157 1 ( 924/1213-1077/1259) 6.3 E06-W03 N14-N17
11 1612 1071 (N06W39 L=175) 415 86 1 (1580/1038-1651/1109) -38.7 W36-W42 N04-N08
12 1312 893 (S04W18 L=154) 294 88 0 (1297/ 845-1330/ 943) 80.5 W17-W19 S07-S01
13 296 855 (S10E52 L= 84) 317 127 0 ( 259/ 831- 337/ 894) -20.6 E55-E47 S11-S07
14 357 765 (S15E47 L= 89) 510 83 1 ( 324/ 736- 391/ 789) 18.4 E49-E43 S17-S13
15 1040 730 (S15W02 L=137) 276 62 0 (1021/ 695-1057/ 765) -78.7 W00-W02 S17-S12
16 1017 645 (S21W00 L=136) 265 36 1 ( 992/ 620-1038/ 670) -26.6 E01-W01 S22-S19
17 507 395 (S41E43 L= 93) 1507 221 0 ( 450/ 354- 557/ 456) 31.0 E51-E35 S45-S35
18 1336 373 (S41W27 L=163) 1586 352 3 (1192/ 328-1508/ 428) 13.5 W15-W41 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.
|
|
|
|
