|
|
|
|
| 20140707 - Filament data for 05 UTC |
|---|
|
Available data for 20140707: »05 UTC »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
1 744 1277 (N19E19 L=220) 648 145 3 ( 706/1241- 791/1316) -18.4 E21-E15 N16-N21
2 1489 1250 (N17W31 L=269) 522 184 0 (1448/1168-1511/1312) 77.5 W28-W32 N12-N21
3 1314 1281 (N19W19 L=257) 350 115 2 (1276/1259-1346/1310) 36.9 W16-W21 N18-N21
4 1581 1180 (N13W37 L=276) 574 199 2 (1546/1101-1604/1264) -78.7 W35-W38 N07-N17
5 1831 1169 (N11W61 L=299) 1309 185 3 (1795/1092-1857/1243) -90.0 W57-W64 N06-N15
6 1357 1157 (N12W21 L=259) 463 162 3 (1295/1118-1432/1208) -18.4 W17-W26 N09-N14
7 462 1171 (N12E38 L=200) 257 95 1 ( 421/1147- 501/1187) -8.1 E41-E34 N10-N12
8 1882 1109 (N07W67 L=306) 724 84 1 (1865/1070-1895/1140) -63.4 W65-W69 N04-N08
9 318 964 (S02E49 L=189) 1501 283 4 ( 243/ 917- 391/1024) 0.0 E56-E42 S04-N01
10 723 976 (N00E19 L=219) 390 106 2 ( 688/ 931- 742/1021) -78.7 E21-E17 S02-N03
11 1376 849 (S08W22 L=261) 284 83 1 (1353/ 814-1407/ 877) 33.7 W20-W24 S09-S05
12 1716 784 (S12W49 L=287) 1125 175 1 (1677/ 705-1764/ 872) 63.4 W46-W53 S17-S06
13 1016 783 (S12E00 L=238) 206 80 0 ( 968/ 763-1050/ 803) 26.6 E03-W01 S12-S10
14 604 672 (S19E28 L=210) 447 90 0 ( 566/ 625- 634/ 715) -63.4 E30-E26 S22-S16
15 1039 472 (S33W01 L=240) 1157 388 1 ( 936/ 370-1120/ 615) 56.3 E06-W06 S41-S22
16 1348 565 (S26W23 L=261) 297 96 0 (1323/ 514-1369/ 609) 71.6 W21-W23 S29-S23
17 1593 578 (S26W42 L=280) 528 95 0 (1552/ 555-1632/ 602) 0.0 W38-W45 S27-S24
18 810 540 (S28E15 L=223) 309 63 1 ( 782/ 521- 844/ 558) 26.6 E16-E12 S29-S26
|
|
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.
|
|
|
|
