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| 20150131 - Latest Filament data |
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Available data for 20150131: »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 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 1199 1792 (N49W01 L= 10) 621 102 2 (1164/1755-1232/1826) -56.3 E02-W03 N45-N52
2 1069 1806 (N48E11 L=358) 330 44 0 (1045/1783-1097/1825) 53.1 E12-E08 N45-N50
3 1508 1590 (N38W27 L= 36) 511 90 0 (1483/1554-1542/1613) 50.2 W24-W30 N34-N40
4 584 1528 (N20E36 L=333) 276 60 2 ( 559/1504- 612/1554) 18.4 E37-E34 N18-N21
5 230 1469 (N14E67 L=302) 746 245 3 ( 200/1437- 261/1511) -33.7 E73-E62 N11-N17
6 507 1431 (N13E39 L=330) 286 61 2 ( 482/1403- 529/1458) -45.0 E41-E37 N11-N14
7 378 1405 (N10E49 L=320) 348 99 1 ( 343/1388- 427/1424) 15.9 E51-E44 N09-N11
8 441 1270 (N02E40 L=329) 291 86 3 ( 412/1247- 468/1292) 14.0 E42-E38 N01-N03
9 1891 1170 (N17W61 L= 70) 2226 393 6 (1844/1092-1930/1236) -37.9 W55-W66 N13-N21
10 1391 1155 (N07W20 L= 29) 204 53 1 (1374/1121-1408/1179) -76.0 W19-W21 N04-N08
11 359 1136 (S06E45 L=324) 361 48 1 ( 337/1107- 380/1166) -36.9 E46-E42 S07-S04
12 748 1098 (S05E17 L=352) 370 133 0 ( 685/1044- 791/1149) -35.5 E21-E14 S07-S02
13 718 942 (S14E18 L=351) 505 127 0 ( 670/ 901- 794/ 984) 35.5 E20-E13 S17-S11
14 147 892 (S21E64 L=305) 1521 200 2 ( 111/ 845- 198/ 948) 29.1 E68-E58 S24-S18
15 1344 881 (S10W21 L= 30) 440 134 1 (1294/ 827-1398/ 934) 66.8 W18-W23 S13-S06
16 1852 874 (S01W61 L= 70) 555 138 0 (1811/ 816-1887/ 924) 49.4 W57-W64 S05-N02
17 1028 818 (S18W03 L= 12) 206 71 1 ( 987/ 807-1070/ 832) 0.0 W00-W05 S18-S17
18 500 703 (S31E32 L=337) 472 93 2 ( 464/ 674- 545/ 737) -31.0 E35-E28 S33-S29
19 1802 577 (S19W66 L= 75) 973 152 5 (1767/ 534-1838/ 630) 56.3 W63-W70 S21-S15
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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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