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| 20141218 - Filament data for 11 UTC |
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Available data for 20141218: »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 453 1447 (N30E37 L=193) 1198 234 3 ( 363/1405- 543/1497) -17.4 E45-E29 N26-N34
2 1388 1461 (N22W28 L=258) 262 124 0 (1328/1448-1447/1474) 0.0 W23-W32 N21-N22
3 1049 1347 (N18W04 L=235) 313 78 2 ( 999/1327-1095/1366) -9.5 W01-W07 N16-N19
4 302 1303 (N22E48 L=182) 519 144 0 ( 259/1266- 345/1340) -29.1 E52-E43 N19-N25
5 281 1192 (N16E49 L=181) 286 52 1 ( 265/1156- 295/1222) 76.0 E50-E48 N13-N17
6 1267 1143 (N04W15 L=246) 361 104 0 (1251/1093-1283/1201) -90.0 W14-W16 N00-N07
7 1584 1086 (S02W36 L=266) 747 153 2 (1531/1033-1653/1137) -32.0 W32-W40 S05-N00
8 320 1081 (N08E46 L=184) 763 138 3 ( 278/1022- 348/1117) -50.2 E49-E43 N04-N11
9 996 940 (S06E02 L=228) 232 85 0 ( 954/ 913-1046/ 962) -45.0 E04-W00 S08-S04
10 199 922 (N00E60 L=170) 418 112 2 ( 170/ 895- 225/ 952) 8.1 E63-E56 N00-N01
11 1408 890 (S12W22 L=253) 434 83 1 (1372/ 847-1429/ 925) -59.0 W20-W23 S15-S10
12 206 737 (S11E63 L=167) 4884 592 5 ( 114/ 592- 302/ 873) -71.6 E76-E55 S19-S01
13 492 816 (S09E36 L=194) 232 54 1 ( 475/ 788- 510/ 848) 53.1 E37-E34 S10-S06
14 1389 727 (S22W21 L=251) 716 214 0 (1311/ 635-1467/ 830) 47.7 W15-W26 S27-S16
15 1195 801 (S16W08 L=239) 217 35 0 (1173/ 784-1221/ 820) -18.4 W07-W10 S17-S14
16 1281 731 (S21W14 L=244) 493 153 0 (1210/ 685-1333/ 796) 32.0 W08-W17 S23-S17
17 497 538 (S26E42 L=188) 938 148 4 ( 441/ 491- 559/ 578) -12.5 E46-E36 S28-S22
18 1466 414 (S45W30 L=260) 658 86 2 (1437/ 385-1498/ 450) -59.0 W27-W33 S47-S42
19 1361 372 (S47W21 L=251) 1068 169 3 (1274/ 345-1431/ 399) 4.1 W13-W28 S49-S45
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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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