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| 20141210 - Filament data for 10 UTC |
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Available data for 20141210: »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
1 886 1744 (N49W02 L=338) 293 51 0 ( 856/1730- 923/1760) -9.5 E01-W05 N47-N51
2 554 1295 (N22E27 L=309) 2054 370 3 ( 416/1177- 630/1371) -37.4 E40-E22 N14-N29
3 131 1204 (N22E71 L=265) 1200 187 2 ( 92/1170- 174/1240) 7.6 E86-E63 N20-N25
4 295 1190 (N19E49 L=287) 370 145 3 ( 244/1174- 342/1210) -16.7 E55-E44 N17-N21
5 765 1123 (N09E14 L=322) 240 62 0 ( 740/1098- 803/1154) -53.1 E15-E12 N07-N11
6 1233 1058 (S01W13 L=349) 364 129 1 (1175/1019-1306/1086) 14.0 W10-W17 S04-N01
7 411 1019 (N07E39 L=297) 323 110 3 ( 367/ 996- 440/1051) 18.4 E42-E37 N06-N10
8 1365 1005 (S06W20 L=356) 213 60 0 (1338/ 991-1406/1023) -26.6 W19-W23 S07-S04
9 1324 955 (S08W17 L=353) 398 127 1 (1263/ 939-1389/ 975) -14.0 W13-W21 S10-S06
10 1851 926 (S17W59 L= 35) 891 114 2 (1822/ 878-1882/ 975) 56.3 W56-W64 S20-S13
11 1191 857 (S12W08 L=344) 552 177 2 (1138/ 773-1236/ 951) 52.1 W06-W10 S18-S06
12 1043 804 (S13E02 L=334) 660 158 0 (1026/ 728-1058/ 886) 71.6 E02-E02 S18-S08
13 1879 833 (S23W65 L= 40) 600 100 1 (1856/ 808-1909/ 864) -24.0 W61-W71 S25-S20
14 172 715 (S07E71 L=265) 3262 317 5 ( 136/ 636- 219/ 786) 73.3 E73-E68 S13-S03
15 1608 669 (S30W38 L= 14) 1743 256 4 (1531/ 587-1652/ 776) 70.0 W30-W44 S36-S22
16 345 687 (S11E52 L=284) 318 94 1 ( 329/ 647- 367/ 717) 38.7 E52-E51 S14-S09
17 546 583 (S20E39 L=297) 1284 268 1 ( 496/ 487- 578/ 697) 42.7 E39-E41 S27-S13
18 238 593 (S15E69 L=267) 537 110 3 ( 216/ 566- 267/ 619) -15.9 E70-E67 S17-S14
19 1370 538 (S35W18 L=354) 478 106 2 (1344/ 489-1388/ 589) 90.0 W16-W20 S39-S31
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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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