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| 20140613 - Filament data for 07 UTC |
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Available data for 20140613: »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 1210 1764 (N55W05 L=199) 323 83 1 (1196/1736-1232/1792) 71.6 W03-W07 N52-N58
2 1332 1710 (N52W17 L=212) 316 62 0 (1304/1691-1359/1727) 26.6 W14-W20 N50-N54
3 455 1587 (N29E52 L=143) 728 139 1 ( 424/1525- 495/1649) -77.5 E54-E50 N24-N33
4 723 1396 (N20E25 L=170) 790 246 2 ( 692/1285- 765/1497) -77.0 E27-E21 N13-N26
5 1616 1409 (N32W39 L=234) 468 78 3 (1591/1374-1641/1439) 59.0 W36-W41 N29-N34
6 1697 1386 (N32W46 L=241) 496 58 1 (1673/1353-1720/1410) -56.3 W44-W48 N29-N33
7 1038 1337 (N20E03 L=192) 210 112 0 ( 986/1320-1100/1351) 15.9 E06-W01 N18-N21
8 1586 1217 (N19W35 L=230) 251 59 0 (1559/1187-1613/1251) -36.9 W33-W37 N17-N21
9 1782 1076 (N13W53 L=248) 1029 278 5 (1735/ 967-1819/1187) -63.4 W48-W57 N05-N19
10 1533 1061 (N09W32 L=227) 296 58 1 (1507/1033-1555/1087) -33.7 W30-W34 N07-N10
11 278 879 (S17E51 L=143) 1287 280 4 ( 205/ 786- 337/ 963) -39.3 E59-E45 S23-S12
12 174 901 (S17E63 L=131) 685 111 3 ( 164/ 845- 190/ 956) 81.9 E64-E61 S20-S13
13 408 773 (S22E40 L=155) 314 57 1 ( 382/ 746- 426/ 796) -45.0 E41-E38 S24-S20
14 498 759 (S22E32 L=163) 365 106 2 ( 461/ 730- 536/ 796) 51.3 E35-E29 S24-S19
15 1724 650 (S14W56 L=251) 4913 768 12 (1597/ 449-1823/ 789) 65.6 W48-W66 S28-S05
16 1391 555 (S24W31 L=226) 929 191 2 (1327/ 495-1477/ 631) 32.2 W27-W35 S28-S18
17 1695 511 (S23W59 L=254) 572 135 1 (1677/ 469-1718/ 549) -71.6 W56-W62 S26-S20
18 776 490 (S37E11 L=184) 524 90 1 ( 733/ 468- 817/ 515) 29.7 E14-E07 S38-S34
19 1316 299 (S44W38 L=232) 386 56 1 (1293/ 278-1338/ 318) -11.3 W35-W40 S45-S42
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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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