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| 20140415 - Filament data for 08 UTC |
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Available data for 20140415: »06 UTC »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC »14 UTC »15 UTC »16 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 409 1623 (N14E64 L=190) 677 236 2 ( 386/1577- 429/1674) -23.2 E74-E58 N11-N17
2 316 1535 (N07E67 L=187) 565 123 0 ( 282/1522- 351/1547) 6.3 E74-E62 N07-N07
3 806 1481 (N14E26 L=228) 554 123 0 ( 746/1433- 862/1538) 77.5 E32-E21 N13-N16
4 1135 1463 (N22E06 L=248) 649 134 1 (1102/1407-1168/1535) -36.9 E11-E03 N20-N26
5 193 1240 (S13E66 L=189) 4767 619 16 ( 127/1111- 244/1422) -62.2 147-E56 S19-S-2
6 690 1323 (N02E27 L=227) 497 119 2 ( 659/1258- 717/1376) -33.7 E31-E24 S01-N05
7 589 1304 (S01E33 L=221) 508 127 0 ( 526/1282- 647/1323) 12.5 E38-E29 S01-S01
8 1041 1250 (N07E05 L=249) 321 92 0 ( 998/1214-1088/1275) -8.1 E08-E02 N07-N08
9 389 1215 (S11E45 L=210) 520 192 0 ( 324/1174- 464/1241) 35.0 E51-E38 S11-S10
10 360 1147 (S15E46 L=209) 792 206 2 ( 301/1091- 446/1202) 32.5 E52-E37 S16-S13
11 919 1146 (S02E09 L=245) 448 131 0 ( 865/1119- 984/1199) -6.3 E13-E05 S01-S00
12 1820 1113 (N24W53 L=308) 378 28 1 (1797/1090-1838/1134) 90.0 W51-W56 N23-N24
13 498 1009 (S20E32 L=223) 988 234 2 ( 458/ 901- 543/1109) -57.5 E37-E27 S25-S15
14 814 960 (S15E10 L=244) 227 44 1 ( 791/ 943- 845/ 983) 0.0 E12-E08 S15-S14
15 1241 806 (S12W18 L=273) 195 39 0 (1217/ 787-1273/ 820) 56.3 W16-W21 S12-S11
16 799 784 (S25E07 L=248) 351 103 0 ( 741/ 761- 841/ 819) 0.0 E11-E03 S25-S25
17 1588 573 (S13W50 L=304) 468 114 1 (1567/ 525-1601/ 628) -56.3 W45-W54 S15-S11
18 585 573 (S45E18 L=236) 274 62 0 ( 565/ 537- 609/ 611) -38.7 E21-E15 S46-S43
19 956 362 (S47W22 L=277) 1561 269 3 ( 833/ 314-1056/ 401) 14.7 W10-W34 S46-S48
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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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