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| 20140113 - Filament data for 11 UTC |
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Available data for 20140113: »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 1475 1437 (N24W28 L= 53) 916 258 2 (1382/1378-1576/1515) -28.3 W21-W35 N20-N28
2 1275 1449 (N23W14 L= 39) 285 121 0 (1208/1424-1332/1465) -6.3 W09-W18 N21-N23
3 342 1398 (N17E49 L=336) 380 82 2 ( 312/1354- 369/1438) 59.0 E51-E47 N13-N19
4 919 1340 (N14E08 L= 17) 253 96 0 ( 903/1302- 944/1385) -68.2 E08-E06 N11-N17
5 1300 1182 (N06W16 L= 41) 326 138 1 (1257/1134-1351/1259) -49.4 W13-W19 N03-N10
6 640 1185 (N04E24 L= 1) 231 84 0 ( 602/1170- 685/1202) 0.0 E26-E21 N03-N04
7 1015 1118 (N01E01 L= 24) 244 117 0 ( 958/1082-1070/1144) 26.6 E04-W02 S01-N02
8 1934 1099 (N07W70 L= 95) 1279 217 3 (1903/1059-1965/1135) -45.0 W65-W76 N04-N09
9 477 1064 (S04E35 L=350) 411 70 2 ( 456/1022- 495/1102) 90.0 E36-E33 S06-S01
10 907 957 (S09E07 L= 18) 174 84 0 ( 864/ 937- 946/ 981) 21.8 E09-E04 S10-S07
11 321 858 (S16E47 L=338) 723 186 2 ( 263/ 813- 390/ 903) 18.4 E53-E41 S18-S13
12 1911 830 (S09W70 L= 95) 1591 281 8 (1876/ 779-1949/ 890) -81.9 W65-W77 S12-S05
13 1791 696 (S19W58 L= 83) 3378 615 15 (1729/ 539-1862/ 878) 81.9 W51-W64 S28-S07
14 962 590 (S31E02 L= 23) 2554 631 3 ( 712/ 451-1239/ 750) 32.6 E21-W15 S42-S19
15 713 670 (S27E19 L= 6) 702 283 4 ( 590/ 591- 800/ 747) 31.0 E28-E13 S32-S22
16 1723 707 (S19W51 L= 76) 328 36 1 (1699/ 690-1742/ 729) 33.7 W49-W53 S19-S17
17 413 609 (S32E43 L=342) 613 115 0 ( 363/ 588- 458/ 641) -26.6 E47-E39 S33-S29
18 313 577 (S34E54 L=332) 1377 273 5 ( 276/ 515- 360/ 634) 76.0 E58-E48 S37-S29
19 1304 414 (S41W26 L= 51) 671 118 3 (1263/ 376-1349/ 467) 81.9 W22-W28 S44-S37
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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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