|
|
|
|
| 20150706 - Latest Filament data |
|---|
|
Available data for 20150706: »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 1251 1631 (N44W19 L=128) 991 232 1 (1226/1547-1274/1708) 61.7 W15-W23 N37-N50
2 1562 1614 (N42W47 L=156) 1369 168 4 (1509/1556-1605/1663) -69.4 W41-W50 N37-N45
3 484 1532 (N35E44 L= 66) 507 79 1 ( 464/1494- 512/1563) -51.3 E46-E41 N32-N37
4 771 1458 (N31E19 L= 91) 418 135 2 ( 755/1399- 786/1519) -82.9 E19-E16 N26-N34
5 1631 1443 (N30W46 L=156) 408 93 1 (1600/1413-1675/1475) -38.7 W43-W49 N27-N31
6 1397 1308 (N21W25 L=134) 459 108 0 (1348/1261-1453/1350) -39.8 W21-W28 N18-N23
7 1116 1270 (N19W06 L=115) 226 54 0 (1093/1253-1148/1290) -33.7 W04-W07 N17-N19
8 902 1196 (N14E08 L=102) 314 139 0 ( 878/1131- 929/1266) -71.6 E09-E06 N09-N18
9 1379 1217 (N15W23 L=132) 228 91 1 (1341/1206-1431/1232) 9.5 W20-W26 N14-N16
10 681 1178 (N12E22 L= 87) 334 111 0 ( 659/1123- 716/1231) 81.9 E23-E20 N08-N15
11 1339 1122 (N09W20 L=129) 514 230 1 (1269/1072-1459/1187) -30.3 W15-W27 N06-N13
12 351 1024 (N02E46 L= 63) 522 149 2 ( 299/ 978- 391/1086) 40.6 E50-E42 S01-N05
13 1695 863 (S07W46 L=156) 309 52 3 (1678/ 833-1713/ 894) -56.3 W44-W48 S08-S05
14 609 831 (S09E27 L= 83) 217 104 0 ( 562/ 812- 666/ 857) -15.9 E29-E22 S10-S07
15 542 643 (S22E33 L= 76) 478 98 0 ( 500/ 617- 591/ 681) -26.6 E35-E29 S23-S19
16 370 610 (S25E48 L= 61) 952 215 1 ( 300/ 583- 434/ 643) 13.0 E55-E42 S26-S22
17 827 359 (S42E16 L= 94) 804 152 1 ( 783/ 314- 867/ 424) 63.4 E20-E12 S46-S36
18 706 398 (S39E25 L= 84) 306 65 1 ( 678/ 370- 733/ 422) -45.0 E27-E23 S41-S37
19 1539 365 (S42W46 L=156) 1549 288 1 (1449/ 334-1637/ 413) 6.7 W37-W56 S44-S38
|
|
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.
|
|
|
|
