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| 20131118 - Filament data for 11 UTC |
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Available data for 20131118: »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC »13 UTC »14 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 1137 1409 (N22W15 L= 59) 207 70 1 (1123/1373-1156/1446) 78.7 W14-W16 N19-N24
2 568 1421 (N36E22 L= 21) 402 92 0 ( 517/1402- 617/1442) 0.0 E26-E18 N34-N36
3 946 1380 (N25W03 L= 46) 1292 408 5 ( 806/1253-1113/1428) -47.0 E05-W10 N14-N29
4 1238 1323 (N15W19 L= 62) 237 91 2 (1212/1283-1263/1353) 76.0 W17-W20 N12-N16
5 322 1188 (N26E45 L=358) 1582 333 3 ( 205/1086- 452/1283) -34.2 E59-E34 N17-N34
6 755 1202 (N18E12 L= 31) 614 242 1 ( 659/1151- 844/1275) -47.7 E17-E07 N13-N24
7 1833 1008 (S16W55 L= 99) 2451 309 10 (1776/ 895-1875/1136) 63.4 W48-W61 S23-S08
8 1044 1110 (N07W03 L= 46) 212 108 1 ( 999/1066-1069/1129) -63.4 W00-W04 N04-N08
9 1756 1017 (S14W48 L= 91) 612 146 2 (1694/ 979-1805/1051) -21.8 W42-W52 S16-S11
10 1386 1013 (S06W21 L= 64) 206 64 0 (1353/ 996-1416/1032) 0.0 W18-W22 S06-S04
11 164 987 (N17E64 L=339) 480 66 1 ( 147/ 950- 188/1020) 45.0 E66-E60 N14-N18
12 205 949 (N14E59 L=344) 456 59 2 ( 186/ 917- 222/ 985) 63.4 E61-E57 N12-N16
13 1265 863 (S12W11 L= 54) 577 206 4 (1210/ 801-1317/ 947) 41.2 W06-W14 S15-S07
14 1448 815 (S19W21 L= 64) 235 105 0 (1428/ 774-1475/ 875) 63.4 W19-W23 S21-S15
15 1477 719 (S25W22 L= 65) 817 340 3 (1349/ 641-1597/ 806) -45.0 W14-W30 S33-S17
16 571 749 (S04E33 L= 10) 391 116 2 ( 535/ 717- 594/ 781) 36.9 E35-E31 S06-S02
17 462 631 (S09E45 L=358) 413 80 1 ( 444/ 593- 483/ 670) 78.7 E45-E42 S11-S06
18 270 550 (S10E68 L=335) 993 157 6 ( 223/ 511- 314/ 586) -39.8 E73-E62 S13-S07
19 660 409 (S26E40 L= 3) 1836 341 4 ( 620/ 262- 685/ 572) 49.4 E52-E33 S36-S15
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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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