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| 20140330 - Filament data for 12 UTC |
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Available data for 20140330: »06 UTC »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC »13 UTC »14 UTC »15 UTC »16 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 557 1587 (N14E46 L= 57) 300 59 0 ( 543/1559- 569/1621) -63.4 E47-E44 N11-N15
2 901 1525 (N18E22 L= 82) 776 211 0 ( 875/1432- 923/1617) -63.4 E24-E17 N12-N24
3 310 1575 (N08E70 L= 34) 807 139 2 ( 290/1537- 343/1599) 78.7 E74-E66 N05-N10
4 1276 1516 (N29W00 L=104) 581 102 1 (1244/1457-1301/1562) -45.0 E02-W03 N25-N31
5 1090 1388 (N15E07 L= 97) 563 175 0 (1063/1312-1107/1470) -56.3 E10-E04 N10-N19
6 506 1365 (S01E40 L= 63) 369 93 1 ( 477/1336- 542/1400) -9.5 E43-E37 S01-N01
7 876 1108 (S06E10 L= 93) 581 131 0 ( 836/1049- 903/1181) -83.7 E12-E08 S10-S01
8 1617 1139 (N17W32 L=135) 260 72 0 (1597/1099-1642/1170) 78.7 W30-W32 N14-N19
9 303 927 (S30E45 L= 58) 3371 613 5 ( 148/ 773- 419/1111) 50.0 E61-E38 S42-S17
10 1631 976 (N09W37 L=140) 248 62 1 (1600/ 955-1663/ 994) 21.8 W34-W39 N06-N09
11 1853 944 (N15W57 L=160) 458 58 1 (1831/ 915-1870/ 973) 90.0 W54-W58 N12-N16
12 625 784 (S31E18 L= 86) 972 267 2 ( 553/ 680- 700/ 892) 72.6 E21-E15 S38-S22
13 1711 836 (N04W48 L=151) 1006 308 2 (1584/ 793-1800/ 891) 33.7 W38-W53 S01-N09
14 954 795 (S21W03 L=106) 644 192 0 ( 861/ 740-1036/ 854) 61.4 E01-W05 S26-S15
15 1176 724 (S19W17 L=121) 484 116 0 (1115/ 689-1243/ 754) 54.5 W14-W20 S22-S15
16 1678 716 (S03W50 L=153) 316 43 0 (1655/ 693-1705/ 736) 53.1 W47-W51 S05-S01
17 960 618 (S31W09 L=112) 218 73 0 ( 925/ 606-1007/ 628) 38.7 W06-W11 S32-S28
18 1548 566 (S15W47 L=150) 365 80 0 (1512/ 545-1582/ 589) 36.9 W44-W48 S16-S13
19 467 522 (S53E28 L= 75) 396 71 1 ( 444/ 499- 500/ 543) 29.7 E31-E24 S55-S51
20 1722 498 (S12W66 L=170) 510 130 2 (1701/ 474-1750/ 525) 90.0 W63-W70 S14-S10
21 1287 444 (S30W36 L=140) 1348 232 2 (1178/ 406-1398/ 483) 42.3 W30-W42 S34-S24
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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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