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| 20150422 - Filament data for 13 UTC |
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Available data for 20150422: »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 1120 1811 (N48E24 L=358) 468 57 1 (1088/1794-1153/1827) 53.1 E26-E21 N45-N50
2 1228 1632 (N37E06 L= 15) 2101 391 6 (1150/1471-1318/1798) -38.4 E20-W04 N28-N48
3 419 1681 (N19E65 L=316) 2065 167 4 ( 362/1637- 473/1730) 58.0 E69-E61 N14-N23
4 622 1587 (N17E42 L=340) 682 212 0 ( 597/1518- 655/1675) -48.4 E45-E36 N13-N22
5 520 1590 (N15E50 L=332) 522 91 2 ( 476/1569- 556/1621) 51.3 E52-E46 N12-N17
6 366 1495 (N06E58 L=324) 802 150 1 ( 294/1419- 415/1546) 53.1 E61-E55 N00-N09
7 471 1485 (N07E48 L=334) 529 149 0 ( 423/1446- 502/1520) 45.0 E50-E45 N04-N09
8 1809 1393 (N43W48 L= 70) 461 51 0 (1793/1369-1826/1415) 45.0 W45-W50 N40-N44
9 1673 1282 (N29W34 L= 56) 755 179 0 (1605/1201-1710/1360) -37.9 W27-W38 N24-N32
10 777 1036 (S11E14 L= 8) 254 114 0 ( 718/ 993- 822/1080) 60.3 E16-E12 S14-S07
11 1833 914 (N13W57 L= 79) 2387 399 5 (1800/ 770-1872/1053) -66.4 W51-W64 N04-N20
12 167 927 (S32E60 L=322) 563 127 0 ( 146/ 883- 199/ 967) 63.4 E61-E56 S34-S28
13 1538 930 (N04W32 L= 54) 229 13 0 (1519/ 909-1555/ 949) 71.6 W31-W33 N02-N05
14 194 795 (S40E56 L=325) 759 190 2 ( 148/ 778- 227/ 819) 18.4 E61-E52 S40-S37
15 1281 773 (S12W22 L= 43) 542 205 0 (1209/ 702-1381/ 811) 55.0 W19-W26 S17-S07
16 1014 792 (S18W06 L= 28) 268 89 2 ( 955/ 779-1060/ 809) 26.6 W02-W08 S19-S16
17 1036 648 (S26W12 L= 33) 676 182 0 ( 942/ 626-1123/ 678) 37.9 W05-W16 S28-S21
18 1214 495 (S29W29 L= 51) 454 94 0 (1164/ 473-1269/ 521) 14.0 W24-W32 S30-S27
19 924 459 (S41W13 L= 34) 247 55 0 ( 906/ 440- 951/ 486) -18.4 W10-W14 S41-S38
20 1019 455 (S38W19 L= 41) 227 31 0 ( 995/ 441-1047/ 469) 33.7 W17-W20 S39-S36
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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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