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| 20140414 - Filament data for 08 UTC |
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Available data for 20140414: »05 UTC »06 UTC »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
1 891 1682 (N29E30 L=238) 398 71 1 ( 862/1659- 926/1706) -9.5 E32-E26 N27-N30
2 626 1537 (N13E39 L=228) 482 127 1 ( 564/1489- 678/1587) 77.5 E42-E37 N08-N17
3 962 1534 (N22E19 L=249) 546 98 0 ( 930/1489- 997/1581) -29.7 E22-E15 N19-N23
4 517 1412 (N03E42 L=226) 247 34 0 ( 499/1390- 535/1434) -14.0 E43-E39 N01-N04
5 447 1357 (S02E45 L=223) 371 118 1 ( 414/1333- 502/1380) 8.1 E47-E40 S03-N00
6 852 1325 (N06E18 L=250) 439 151 0 ( 784/1267- 889/1359) -14.0 E22-E14 N03-N07
7 267 1263 (S11E57 L=211) 820 255 2 ( 194/1192- 344/1304) 30.3 E62-E50 S15-S07
8 747 1237 (S01E21 L=246) 542 172 1 ( 673/1211- 827/1287) 0.0 E26-E16 S02-N00
9 1169 1243 (N10W02 L=270) 207 51 2 (1136/1225-1194/1259) -18.4 W00-W03 N09-N11
10 265 1195 (S15E55 L=213) 1190 233 3 ( 196/1128- 332/1249) 26.6 E60-E48 S19-S11
11 340 1109 (S18E46 L=222) 505 80 2 ( 313/1072- 363/1148) 59.0 E47-E44 S20-S15
12 344 967 (S26E42 L=225) 1758 334 5 ( 314/ 810- 394/1085) -86.8 E45-E39 S36-S18
13 994 868 (S15W03 L=270) 200 66 0 ( 957/ 852-1030/ 890) 53.1 W00-W04 S16-S12
14 640 872 (S24E19 L=249) 204 40 0 ( 614/ 858- 668/ 889) 0.0 E20-E16 S25-S23
15 896 769 (S23E00 L=268) 705 262 0 ( 763/ 736-1009/ 807) 34.7 E08-W05 S27-S18
16 470 620 (S45E28 L=240) 261 64 0 ( 451/ 582- 494/ 653) -45.0 E29-E25 S47-S43
17 1581 537 (S15W51 L=319) 316 54 1 (1551/ 520-1609/ 552) 11.3 W48-W53 S16-S13
18 722 450 (S49E01 L=266) 500 100 0 ( 692/ 421- 778/ 493) -8.1 E04-W03 S50-S46
19 834 431 (S46W08 L=276) 367 85 4 ( 810/ 397- 854/ 464) -80.5 W05-W10 S49-S43
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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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