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| 20141213 - Filament data for 09 UTC |
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Available data for 20141213: »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 1682 1487 (N20W53 L=349) 522 115 1 (1642/1424-1713/1537) -76.0 W50-W54 N15-N23
2 269 1356 (N29E51 L=245) 884 166 3 ( 225/1290- 299/1426) 71.6 E55-E48 N24-N33
3 482 1310 (N23E32 L=264) 652 190 0 ( 400/1269- 545/1374) 21.8 E38-E27 N20-N26
4 1859 1122 (S04W61 L=358) 1091 253 4 (1823/1065-1899/1178) 45.0 W56-W66 S07-N00
5 1424 1134 (N01W25 L=322) 441 132 2 (1400/1089-1441/1176) 76.0 W23-W26 S01-N03
6 1413 1045 (S04W24 L=321) 329 74 1 (1379/1006-1444/1076) -45.0 W21-W25 S06-S01
7 1721 910 (S15W45 L=342) 716 172 0 (1677/ 823-1768/ 981) 45.0 W41-W49 S19-S11
8 1620 909 (S14W37 L=334) 274 72 0 (1603/ 880-1636/ 952) 76.0 W35-W38 S15-S11
9 1415 878 (S14W22 L=319) 265 56 1 (1387/ 847-1443/ 909) -63.4 W20-W24 S15-S11
10 319 867 (S02E49 L=248) 311 58 1 ( 302/ 833- 335/ 894) -76.0 E50-E47 S04-N00
11 1454 848 (S16W25 L=322) 260 88 0 (1426/ 789-1478/ 893) 56.3 W22-W26 S19-S13
12 1837 829 (S21W56 L=353) 513 107 0 (1807/ 790-1873/ 860) 29.7 W53-W60 S23-S19
13 1106 693 (S21W01 L=298) 1041 235 4 (1031/ 601-1165/ 790) 48.0 E04-W05 S26-S15
14 522 737 (S12E35 L=261) 283 48 1 ( 499/ 713- 551/ 761) -33.7 E36-E33 S13-S10
15 377 683 (S14E48 L=249) 1453 239 6 ( 320/ 631- 435/ 730) -40.6 E52-E43 S17-S10
16 471 575 (S21E44 L=253) 1143 342 5 ( 437/ 455- 504/ 718) 53.1 E49-E37 S28-S12
17 1619 665 (S29W37 L=334) 593 118 1 (1563/ 618-1668/ 710) 32.0 W33-W41 S31-S26
18 785 278 (S46E33 L=264) 564 114 1 ( 758/ 244- 811/ 316) 40.6 E36-E29 S49-S43
19 637 226 (S48E50 L=247) 589 186 0 ( 608/ 202- 680/ 253) 14.0 E55-E43 S50-S46
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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.
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