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| 20150512 - Filament data for 06 UTC |
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Available data for 20150512: »06 UTC »07 UTC »08 UTC »09 UTC »10 UTC »11 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
1 792 1835 (N43E46 L= 75) 525 117 2 ( 750/1817- 836/1851) 7.1 E49-E41 N41-N44
2 1345 1654 (N46W05 L=126) 1148 253 2 (1324/1568-1374/1744) -75.1 W02-W09 N38-N54
3 468 1669 (N23E59 L= 62) 1025 202 2 ( 447/1610- 496/1732) -48.4 E63-E55 N18-N27
4 873 1675 (N33E29 L= 92) 311 48 1 ( 848/1654- 891/1698) 90.0 E30-E27 N31-N34
5 1590 1606 (N51W30 L=151) 402 64 0 (1562/1591-1616/1621) 29.7 W26-W33 N48-N53
6 535 1547 (N17E46 L= 75) 513 147 2 ( 510/1498- 562/1619) -63.4 E48-E42 N13-N21
7 927 1569 (N27E21 L=101) 298 56 0 ( 903/1553- 958/1590) 0.0 E22-E18 N25-N28
8 621 1513 (N16E38 L= 83) 312 131 0 ( 594/1483- 655/1557) -23.2 E41-E34 N14-N18
9 998 1484 (N23E13 L=108) 234 64 1 ( 974/1463-1016/1519) -76.0 E14-E11 N21-N25
10 935 1386 (N16E14 L=107) 467 137 2 ( 917/1322- 963/1439) -56.3 E16-E11 N12-N19
11 211 1206 (S10E62 L= 59) 860 144 2 ( 183/1154- 240/1263) 90.0 E65-E59 S13-S06
12 1260 1232 (N14W09 L=130) 327 62 2 (1225/1208-1294/1261) 45.0 W07-W10 N12-N16
13 280 1218 (S08E55 L= 66) 519 74 3 ( 255/1186- 309/1239) 71.6 E57-E52 S09-S06
14 1089 1068 (N01W03 L=124) 186 42 1 (1063/1051-1116/1088) 18.4 W01-W04 N00-N02
15 1711 1007 (N13W44 L=166) 362 61 0 (1689/ 977-1738/1030) 53.1 W42-W46 N10-N14
16 611 776 (S27E20 L=101) 290 74 0 ( 574/ 758- 643/ 799) 26.6 E22-E18 S28-S25
17 1800 726 (S00W62 L=184) 638 119 0 (1762/ 663-1829/ 775) 74.1 W60-W64 S04-N03
18 785 579 (S35E04 L=117) 225 64 1 ( 763/ 561- 813/ 604) -33.7 E05-E01 S36-S33
19 1662 516 (S16W59 L=180) 955 161 3 (1619/ 464-1696/ 554) -81.9 W54-W61 S19-S12
20 1331 276 (S40W48 L=170) 1056 221 1 (1253/ 261-1423/ 295) 21.0 W42-W56 S42-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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