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| 20141214 - Filament data for 09 UTC |
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Available data for 20141214: »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
1 369 1431 (N32E43 L=240) 318 75 1 ( 341/1402- 403/1463) 31.0 E45-E40 N29-N33
2 394 1390 (N29E40 L=243) 312 69 1 ( 364/1356- 428/1421) 31.0 E42-E37 N26-N30
3 1420 1365 (N15W29 L=312) 256 91 0 (1404/1321-1432/1410) 68.2 W27-W30 N12-N18
4 640 1333 (N22E21 L=262) 389 156 0 ( 570/1295- 719/1352) 10.3 E26-E15 N20-N22
5 268 1196 (N18E50 L=233) 364 96 0 ( 233/1182- 302/1214) -26.6 E53-E47 N16-N19
6 1159 1174 (N07W10 L=293) 222 132 0 (1102/1158-1219/1203) -15.9 W06-W13 N05-N08
7 133 1055 (N11E66 L=217) 762 156 5 ( 98/1033- 159/1085) 15.9 E71-E62 N09-N12
8 1789 986 (S11W52 L=335) 776 190 0 (1759/ 888-1816/1082) 61.4 W48-W55 S16-S05
9 379 1003 (N05E42 L=242) 260 50 1 ( 362/ 970- 401/1028) 71.6 E43-E39 N03-N06
10 1857 936 (S14W59 L=342) 495 110 0 (1831/ 894-1881/ 988) 45.0 W55-W61 S16-S11
11 1557 938 (S11W33 L=316) 239 67 1 (1528/ 918-1595/ 957) 21.8 W30-W35 S12-S10
12 1327 750 (S20W16 L=300) 998 191 3 (1260/ 674-1377/ 827) 45.0 W11-W19 S24-S16
13 521 738 (S12E35 L=248) 860 141 3 ( 467/ 702- 573/ 771) -14.0 E39-E31 S14-S10
14 627 601 (S22E31 L=252) 580 236 0 ( 591/ 510- 658/ 710) 50.2 E36-E26 S27-S15
15 1733 668 (S30W48 L=331) 448 93 0 (1695/ 636-1768/ 697) 26.6 W44-W50 S31-S28
16 472 569 (S22E44 L=240) 295 57 0 ( 446/ 539- 491/ 589) -90.0 E45-E42 S23-S20
17 905 315 (S46E21 L=263) 482 95 1 ( 877/ 284- 926/ 355) 39.8 E24-E17 S47-S42
18 603 333 (S40E44 L=239) 329 40 0 ( 577/ 315- 631/ 354) -63.4 E45-E42 S41-S37
19 729 254 (S48E39 L=244) 573 124 1 ( 695/ 231- 775/ 276) 6.3 E43-E34 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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