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| 20140316 - Filament data for 11 UTC |
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Available data for 20140316: »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 1249 1813 (N51E13 L=276) 534 74 3 (1222/1789-1277/1840) 45.0 E15-E10 N48-N54
2 465 1711 (N21E61 L=228) 558 89 0 ( 441/1690- 497/1726) 21.8 E64-E57 N19-N22
3 659 1535 (N13E36 L=253) 855 337 1 ( 612/1417- 725/1656) -39.1 E43-E27 N07-N20
4 971 1411 (N13E13 L=275) 280 91 1 ( 947/1355- 989/1451) -71.6 E14-E11 N09-N15
5 251 1259 (S11E58 L=230) 341 25 1 ( 234/1236- 268/1283) -71.6 E60-E56 S12-S09
6 289 1205 (S13E53 L=236) 480 83 1 ( 271/1160- 308/1246) -68.2 E55-E50 S15-S10
7 175 1199 (S15E65 L=224) 1113 202 4 ( 141/1161- 214/1236) -24.0 E70-E59 S17-S12
8 209 1113 (S20E58 L=231) 481 71 1 ( 185/1086- 229/1143) 76.0 E60-E56 S21-S17
9 736 1088 (S11E18 L=271) 356 80 2 ( 700/1061- 768/1118) 63.4 E20-E16 S12-S08
10 485 1074 (S17E34 L=255) 611 184 2 ( 420/1050- 585/1099) 9.5 E38-E26 S19-S14
11 1160 976 (S06W09 L=297) 316 103 1 (1129/ 931-1203/1024) -23.2 W05-W12 S08-S04
12 117 972 (S29E66 L=223) 752 223 0 ( 83/ 941- 152/1004) 26.6 E69-E61 S30-S27
13 236 985 (S27E53 L=236) 458 125 1 ( 197/ 969- 274/1002) 8.1 E56-E49 S28-S25
14 775 898 (S20E11 L=277) 1320 424 1 ( 595/ 806- 970/ 979) 9.5 E22-W02 S24-S16
15 409 879 (S30E36 L=252) 864 181 0 ( 340/ 848- 482/ 929) -4.8 E42-E30 S31-S28
16 1182 694 (S21W18 L=307) 339 92 0 (1141/ 663-1226/ 725) 0.0 W15-W21 S21-S19
17 868 586 (S36W03 L=292) 739 193 2 ( 770/ 545- 967/ 615) 7.6 E04-W11 S38-S34
18 1747 549 (S10W65 L=354) 858 163 4 (1707/ 462-1780/ 591) 90.0 W62-W68 S15-S07
19 1684 526 (S14W60 L=348) 993 169 4 (1648/ 474-1716/ 577) -80.5 W57-W64 S16-S10
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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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