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| 20150613 - Filament data for 08 UTC |
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Available data for 20150613: »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC »14 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 473 1661 (N34E55 L= 2) 1915 487 6 ( 430/1592- 532/1741) -29.1 E65-E47 N29-N39
2 891 1588 (N35E18 L= 39) 392 108 3 ( 840/1553- 932/1620) -20.6 E22-E14 N33-N36
3 1352 1578 (N41W18 L= 75) 476 57 1 (1318/1551-1378/1604) 0.0 W14-W19 N38-N43
4 697 1378 (N18E26 L= 31) 1779 450 6 ( 576/1222- 780/1524) -39.0 E38-E17 N09-N26
5 1075 1438 (N27E02 L= 55) 1011 228 3 (1004/1335-1158/1518) -39.8 E08-W04 N21-N31
6 1413 1436 (N31W22 L= 79) 483 95 1 (1384/1395-1445/1483) -51.3 W19-W24 N28-N34
7 1697 1108 (N14W45 L=102) 2011 592 7 (1632/ 975-1818/1315) -49.6 W39-W57 N04-N26
8 235 1240 (N04E61 L=356) 415 94 1 ( 223/1196- 245/1291) -71.6 E62-E59 N01-N07
9 1490 1197 (N17W28 L= 85) 765 302 1 (1396/1142-1537/1269) 41.6 W21-W31 N12-N21
10 1292 1148 (N11W15 L= 72) 298 114 1 (1237/1105-1342/1192) -29.7 W11-W18 N09-N13
11 1819 1132 (N16W57 L=113) 436 85 3 (1797/1108-1843/1171) -56.3 W54-W59 N15-N18
12 1872 1064 (N13W64 L=120) 2324 305 5 (1844/ 960-1913/1163) -71.6 W60-W69 N06-N18
13 1073 1071 (N04W02 L= 59) 544 164 2 ( 981/1048-1152/1095) 24.0 E02-W07 N01-N06
14 439 946 (S11E38 L= 19) 1291 455 3 ( 284/ 908- 616/1001) 2.1 E51-E24 S13-S08
15 1162 852 (S08W10 L= 67) 327 159 0 (1124/ 773-1204/ 931) 79.7 W09-W12 S13-S02
16 241 777 (S25E56 L= 1) 566 102 3 ( 217/ 745- 262/ 810) -45.0 E58-E53 S26-S22
17 1713 707 (S11W53 L=110) 651 162 1 (1686/ 668-1758/ 760) -32.0 W49-W58 S13-S07
18 1569 392 (S33W53 L=110) 410 96 1 (1550/ 367-1586/ 426) -38.7 W50-W55 S35-S30
19 1411 372 (S37W41 L= 98) 778 117 2 (1350/ 346-1467/ 401) 26.6 W36-W45 S39-S34
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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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