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| 20140612 - Filament data for 08 UTC |
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Available data for 20140612: »06 UTC »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 1052 1763 (N52E12 L=196) 375 56 1 (1025/1743-1077/1781) 36.9 E13-E09 N49-N54
2 357 1553 (N25E60 L=148) 1442 215 4 ( 323/1469- 397/1634) -74.7 E63-E56 N19-N30
3 1523 1413 (N32W31 L=238) 727 192 0 (1440/1374-1599/1449) -4.8 W24-W37 N29-N33
4 558 1339 (N14E35 L=173) 448 107 0 ( 544/1286- 574/1392) -66.8 E36-E33 N10-N17
5 1143 1294 (N19W04 L=212) 223 50 0 (1118/1270-1172/1316) -26.6 W02-W06 N17-N19
6 1888 1095 (N15W66 L=273) 2438 322 9 (1860/1016-1924/1200) -57.5 W61-W72 N10-N21
7 1817 1119 (N16W57 L=264) 656 127 4 (1793/1076-1842/1157) 56.3 W54-W59 N12-N18
8 202 903 (S17E60 L=148) 2180 400 5 ( 154/ 810- 263/ 978) 74.7 E66-E52 S23-S12
9 1840 858 (N00W63 L=271) 2026 247 2 (1813/ 757-1861/ 969) -57.5 W60-W69 S05-N06
10 355 925 (S14E44 L=163) 329 72 2 ( 327/ 894- 377/ 957) -76.0 E46-E42 S15-S11
11 1005 865 (S09W01 L=208) 197 80 0 ( 990/ 827-1017/ 911) 90.0 W00-W01 S11-S06
12 329 772 (S24E47 L=161) 530 111 1 ( 294/ 727- 365/ 809) -45.0 E50-E43 S26-S21
13 1591 667 (S14W44 L=251) 1743 384 2 (1473/ 512-1707/ 782) 62.2 W38-W51 S25-S06
14 850 721 (S20E07 L=200) 366 127 1 ( 803/ 697- 922/ 756) -14.0 E10-E02 S21-S18
15 1446 734 (S12W31 L=238) 512 125 0 (1387/ 719-1503/ 748) 6.3 W26-W35 S12-S10
16 1652 630 (S16W50 L=257) 986 237 5 (1589/ 591-1724/ 664) 9.5 W44-W57 S18-S13
17 1279 637 (S20W22 L=229) 234 43 0 (1251/ 619-1310/ 656) 45.0 W20-W23 S21-S18
18 620 533 (S36E23 L=184) 483 155 0 ( 567/ 511- 665/ 584) 32.0 E27-E19 S38-S31
19 1606 528 (S23W50 L=257) 498 130 2 (1575/ 494-1641/ 567) -45.0 W46-W53 S25-S20
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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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