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| 20140115 - Filament data for 10 UTC |
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Available data for 20140115: »08 UTC »09 UTC »10 UTC »12 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 1056 1538 (N28E01 L=358) 396 88 2 (1027/1505-1094/1566) -26.6 E03-W01 N25-N29
2 1758 1411 (N25W51 L= 51) 1806 318 5 (1687/1322-1868/1491) -29.4 W45-W62 N20-N30
3 1645 1406 (N24W41 L= 40) 355 78 1 (1609/1374-1677/1425) -18.4 W37-W43 N21-N24
4 1385 1263 (N12W21 L= 20) 287 108 0 (1344/1239-1435/1299) -18.4 W18-W24 N10-N13
5 1476 1245 (N12W27 L= 26) 303 143 1 (1436/1196-1503/1291) -71.6 W24-W28 N08-N14
6 1715 1120 (N06W45 L= 44) 1228 310 7 (1637/1062-1786/1212) -28.3 W38-W51 N03-N11
7 1111 1144 (N03W05 L= 4) 259 64 2 (1070/1121-1148/1169) 36.9 W02-W06 N01-N04
8 391 1101 (S02E42 L=318) 282 57 0 ( 373/1069- 408/1134) -63.4 E43-E40 S04-N00
9 1477 1098 (N03W27 L= 27) 313 117 0 (1421/1066-1524/1133) 35.5 W23-W30 N00-N05
10 213 900 (S14E58 L=302) 2599 448 10 ( 181/ 697- 254/1079) 70.8 E63-E53 S26-S03
11 841 986 (S08E11 L=349) 307 57 2 ( 825/ 948- 859/1028) 90.0 E11-E09 S10-S05
12 1286 923 (S09W16 L= 16) 478 275 0 (1155/ 884-1422/ 970) 23.6 W08-W24 S12-S05
13 471 886 (S15E35 L=324) 243 92 1 ( 455/ 841- 490/ 937) 80.5 E36-E33 S17-S11
14 685 868 (S15E20 L=339) 485 128 2 ( 638/ 843- 756/ 903) 14.0 E23-E15 S17-S13
15 1734 736 (S16W52 L= 51) 1550 408 10 (1657/ 604-1823/ 871) 64.8 W45-W57 S24-S07
16 967 812 (S18E02 L=357) 278 99 2 ( 917/ 790-1023/ 856) -26.6 E05-W01 S18-S15
17 1133 714 (S23W09 L= 8) 726 280 1 (1059/ 621-1207/ 824) 61.7 W04-W12 S28-S15
18 1428 782 (S16W27 L= 27) 323 107 0 (1397/ 745-1474/ 804) 11.3 W25-W30 S18-S14
19 503 606 (S33E36 L=324) 757 274 3 ( 468/ 510- 539/ 705) 65.2 E40-E32 S39-S26
20 1299 556 (S32W22 L= 22) 2774 634 5 (1004/ 429-1582/ 689) 30.1 W02-W40 S42-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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