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| 20140930 - Filament data for 06 UTC |
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Available data for 20140930: »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 1439 1705 (N31W53 L=247) 979 215 1 (1374/1683-1517/1723) -17.1 W46-W59 N28-N34
2 1014 1426 (N29W11 L=206) 320 82 0 ( 966/1399-1056/1454) 0.0 W07-W14 N28-N30
3 1484 1406 (N14W39 L=233) 2692 630 4 (1213/1364-1708/1433) -21.8 W21-W56 N06-N21
4 714 1234 (N27E13 L=181) 694 157 1 ( 674/1160- 743/1310) 84.3 E14-E10 N21-N31
5 1857 1194 (S10W62 L=256) 2510 365 9 (1801/1094-1915/1260) 38.7 W55-W72 S15-S05
6 1121 1135 (N10W08 L=203) 374 133 1 (1108/1063-1142/1207) 54.5 W06-W11 N06-N13
7 1810 1107 (S12W53 L=248) 671 104 3 (1786/1071-1837/1152) -78.7 W50-W56 S14-S09
8 1753 1071 (S12W47 L=241) 1522 339 4 (1711/ 964-1818/1146) -77.0 W42-W50 S20-S07
9 1672 1043 (S11W40 L=234) 620 102 3 (1649/ 990-1695/1096) 81.9 W36-W41 S14-S07
10 1164 1007 (N02W07 L=202) 471 93 0 (1111/ 984-1215/1034) -38.7 W04-W09 N00-N04
11 316 942 (N19E48 L=146) 420 84 0 ( 301/ 892- 330/ 989) 71.6 E50-E46 N15-N21
12 1518 791 (S20W23 L=217) 2055 424 4 (1404/ 625-1568/ 940) -87.5 W18-W25 S31-S08
13 688 488 (S16E36 L=159) 721 258 1 ( 645/ 392- 731/ 580) 45.0 E42-E30 S20-S09
14 460 544 (S07E50 L=145) 581 124 0 ( 417/ 512- 523/ 577) -39.8 E52-E45 S10-S04
15 278 526 (S06E71 L=124) 807 181 2 ( 244/ 501- 324/ 566) -26.6 E75-E64 S07-S02
16 921 341 (S31E28 L=166) 1547 322 3 ( 794/ 286-1007/ 453) 15.9 E39-E18 S34-S25
17 552 419 (S17E49 L=146) 369 90 2 ( 507/ 401- 586/ 434) -36.9 E51-E46 S18-S15
18 701 223 (S35E51 L=143) 802 184 2 ( 680/ 186- 730/ 265) 33.7 E56-E47 S37-S31
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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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