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| 20140330 - Filament data for 15 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
1 924 1510 (N18E20 L= 82) 719 204 0 ( 897/1420- 949/1605) -63.4 E22-E16 N12-N24
2 321 1567 (N08E68 L= 34) 1302 141 4 ( 285/1525- 360/1600) 39.8 E72-E63 N05-N10
3 1297 1509 (N29W02 L=104) 614 103 2 (1262/1447-1323/1559) -50.2 E01-W05 N25-N31
4 1113 1374 (N15E05 L= 97) 566 178 0 (1078/1305-1130/1464) -48.8 E09-E02 N10-N19
5 520 1367 (S00E39 L= 62) 422 111 2 ( 482/1323- 560/1408) -15.9 E43-E35 S02-N01
6 1643 1142 (N18W34 L=135) 270 82 1 (1617/1109-1669/1171) 78.7 W31-W34 N15-N20
7 899 1097 (S06E09 L= 93) 501 93 1 ( 865/1043- 925/1154) -81.9 E09-E07 S09-S02
8 311 911 (S31E45 L= 57) 3135 634 7 ( 158/ 760- 437/1098) 50.0 E60-E36 S42-S17
9 1652 967 (N09W39 L=140) 333 89 1 (1620/ 944-1690/ 986) 31.0 W36-W41 N06-N10
10 1867 937 (N15W59 L=161) 483 66 2 (1844/ 906-1886/ 966) -71.6 W56-W60 N13-N16
11 1696 829 (N03W47 L=148) 1162 381 1 (1561/ 790-1814/ 881) 24.2 W35-W55 S01-N09
12 640 769 (S31E16 L= 85) 809 257 0 ( 567/ 672- 712/ 867) 68.2 E20-E13 S38-S23
13 974 784 (S21W04 L=106) 752 205 1 ( 871/ 719-1057/ 841) 57.5 W00-W07 S27-S15
14 1199 707 (S19W19 L=121) 551 152 0 (1128/ 666-1286/ 737) 48.8 W16-W23 S22-S14
15 1693 709 (S03W51 L=153) 339 57 1 (1668/ 683-1718/ 733) 63.4 W49-W53 S05-S01
16 1564 556 (S15W48 L=150) 400 78 0 (1527/ 535-1597/ 582) 53.1 W45-W50 S16-S12
17 1295 435 (S31W37 L=139) 1339 249 3 (1187/ 393-1416/ 474) 37.6 W31-W44 S35-S25
18 1548 412 (S23W56 L=158) 468 74 1 (1512/ 382-1580/ 443) 68.2 W54-W58 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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