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| 20150420 - Filament data for 09 UTC |
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Available data for 20150420: »06 UTC »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC »13 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 907 1772 (N37E34 L= 16) 2817 583 4 ( 863/1649- 971/1925) -32.3 E53-E23 N28-N49
2 402 1515 (N07E56 L=354) 526 126 0 ( 388/1462- 419/1565) -50.2 E59-E53 N04-N10
3 1610 1509 (N43W26 L= 77) 331 60 1 (1591/1480-1632/1527) 53.1 W24-W28 N40-N44
4 1358 1407 (N26W09 L= 59) 353 118 0 (1327/1343-1376/1448) -51.3 W06-W10 N21-N28
5 1806 1370 (N41W47 L= 97) 1633 219 2 (1738/1308-1863/1423) -14.0 W39-W54 N38-N43
6 785 1340 (N06E22 L= 28) 412 44 0 ( 761/1306- 810/1374) -63.4 E23-E20 N04-N08
7 1852 1257 (N34W52 L=102) 756 148 1 (1808/1231-1877/1286) 36.9 W47-W55 N30-N37
8 1137 1138 (N04W03 L= 53) 203 26 0 (1119/1118-1154/1162) -71.6 W02-W04 N02-N05
9 1049 1150 (N02E02 L= 48) 205 107 0 ( 995/1140-1106/1159) 31.0 E04-W01 N00-N03
10 1673 1033 (N14W39 L= 89) 864 217 0 (1635/ 959-1728/1081) 76.0 W36-W43 N09-N17
11 1586 1024 (N11W33 L= 83) 470 84 1 (1560/ 979-1615/1070) -80.5 W30-W35 N07-N13
12 842 941 (S15E08 L= 42) 305 108 1 ( 819/ 886- 867/ 996) 90.0 E09-E07 S18-S10
13 1697 890 (N07W45 L= 95) 807 140 1 (1644/ 837-1736/ 946) 66.0 W41-W48 N02-N11
14 1835 892 (N12W58 L=108) 814 117 2 (1809/ 832-1862/ 939) 82.9 W55-W61 N07-N15
15 386 894 (S29E38 L= 12) 727 162 1 ( 321/ 845- 445/ 935) 38.7 E43-E33 S33-S25
16 690 850 (S24E15 L= 35) 583 181 0 ( 611/ 819- 785/ 896) 45.0 E19-E09 S27-S18
17 868 699 (S28W00 L= 50) 456 74 2 ( 834/ 666- 901/ 732) 63.4 E01-W02 S29-S25
18 649 625 (S39E13 L= 37) 433 70 0 ( 615/ 607- 693/ 650) 18.4 E15-E09 S40-S36
19 1186 296 (S42W40 L= 90) 367 43 0 (1157/ 276-1214/ 316) 11.3 W37-W42 S43-S41
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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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