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| 20150424 - Filament data for 12 UTC |
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Available data for 20150424: »07 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 1381 1697 (N49W03 L=359) 355 87 0 (1351/1676-1411/1720) 21.8 W00-W06 N46-N51
2 647 1619 (N20E42 L=314) 620 124 1 ( 588/1582- 683/1671) 66.8 E45-E40 N16-N24
3 1601 1476 (N40W26 L= 22) 316 64 0 (1576/1443-1624/1509) -45.0 W23-W28 N37-N41
4 1008 1356 (N13E10 L=346) 771 300 1 ( 928/1218-1103/1471) -30.5 E17-W00 N07-N18
5 803 1349 (N08E21 L=334) 452 249 0 ( 691/1285- 901/1437) 63.4 E26-E18 N01-N15
6 1603 1366 (N32W28 L= 23) 912 162 4 (1548/1326-1651/1404) 14.0 W23-W31 N28-N35
7 1622 1290 (N28W30 L= 26) 310 58 1 (1595/1260-1638/1315) -56.3 W28-W31 N26-N29
8 1850 1035 (N20W55 L= 51) 661 108 2 (1814/1000-1878/1070) 50.2 W51-W57 N17-N23
9 1617 983 (N10W36 L= 32) 292 54 1 (1596/ 963-1640/1009) -14.0 W34-W38 N08-N10
10 1859 951 (N16W59 L= 54) 596 87 1 (1841/ 914-1885/ 981) -53.1 W56-W61 N13-N17
11 374 836 (S32E38 L=317) 809 208 0 ( 342/ 765- 446/ 882) 52.1 E41-E32 S37-S28
12 1099 817 (S14W10 L= 6) 356 156 0 (1013/ 779-1173/ 854) 53.1 W06-W13 S18-S10
13 1773 807 (N05W55 L= 51) 403 90 2 (1752/ 777-1790/ 849) 78.7 W53-W57 N02-N07
14 363 722 (S40E39 L=317) 928 215 1 ( 294/ 688- 444/ 778) -8.1 E45-E30 S41-S37
15 1603 624 (S10W48 L= 44) 957 231 0 (1505/ 543-1668/ 715) 74.1 W44-W51 S17-S03
16 1381 675 (S14W31 L= 27) 262 92 0 (1343/ 657-1413/ 698) 11.3 W27-W32 S15-S12
17 1353 609 (S18W32 L= 28) 302 141 0 (1284/ 595-1414/ 627) 35.5 W27-W35 S20-S15
18 1343 483 (S26W37 L= 33) 1369 284 3 (1214/ 453-1460/ 521) 19.4 W27-W44 S28-S21
19 1260 325 (S38W42 L= 37) 362 99 0 (1234/ 307-1296/ 354) 0.0 W38-W45 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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