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| 20140206 - Latest Filament data |
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Available data for 20140206: »11 UTC »12 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 383 1669 (N26E61 L= 8) 721 222 0 ( 350/1644- 429/1695) -15.3 E66-E55 N24-N28
2 876 1578 (N25E19 L= 50) 269 72 0 ( 839/1559- 917/1603) -9.5 E22-E16 N23-N26
3 414 1421 (N09E47 L= 22) 341 72 0 ( 387/1400- 444/1449) -18.4 E49-E43 N08-N11
4 763 1277 (N05E19 L= 49) 243 78 0 ( 715/1267- 801/1292) 21.8 E22-E17 N03-N05
5 154 1023 (S16E64 L= 5) 5155 735 13 ( 103/ 784- 199/1209) -85.6 E71-E58 S30-S04
6 1625 1092 (N08W36 L=105) 295 81 1 (1594/1051-1648/1116) -36.9 W33-W37 N05-N09
7 224 1071 (S13E56 L= 12) 394 91 1 ( 200/1041- 255/1099) 56.3 E58-E53 S14-S11
8 1707 1035 (N06W43 L=112) 249 124 1 (1658/1006-1751/1063) 35.5 W40-W47 N03-N08
9 774 979 (S13E14 L= 54) 389 160 0 ( 717/ 918- 852/1012) 36.9 E17-E09 S16-S09
10 381 809 (S28E41 L= 28) 1865 719 4 ( 178/ 705- 631/ 898) 19.7 E61-E22 S35-S20
11 1465 819 (S11W30 L= 99) 430 145 1 (1427/ 788-1530/ 867) -15.9 W27-W34 S13-S08
12 1131 771 (S19W11 L= 79) 340 101 0 (1115/ 703-1145/ 820) -66.8 W08-W12 S23-S16
13 1634 783 (S09W43 L=112) 274 70 1 (1605/ 760-1657/ 804) -21.8 W40-W45 S10-S08
14 873 776 (S23E05 L= 63) 352 104 0 ( 819/ 764- 934/ 796) 15.9 E08-E01 S24-S22
15 716 654 (S33E15 L= 54) 681 211 1 ( 650/ 589- 792/ 751) 53.1 E19-E10 S38-S25
16 1653 708 (S13W47 L=116) 424 80 2 (1619/ 678-1677/ 746) 45.0 W44-W48 S14-S10
17 1473 589 (S24W38 L=106) 512 221 0 (1429/ 500-1545/ 654) 90.0 W34-W41 S29-S18
18 1024 511 (S37W10 L= 78) 488 146 0 ( 963/ 476-1074/ 580) 58.0 W05-W12 S40-S32
19 1388 254 (S47W51 L=119) 407 82 0 (1372/ 224-1400/ 286) -38.7 W47-W53 S48-S44
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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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