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| 20140330 - Filament data for 06 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
1 522 1601 (N14E50 L= 57) 340 66 0 ( 508/1573- 536/1636) -59.0 E51-E48 N11-N16
2 859 1539 (N18E25 L= 82) 615 218 0 ( 836/1450- 878/1633) -63.4 E27-E20 N12-N24
3 1235 1537 (N29E03 L=104) 488 95 0 (1201/1483-1259/1576) -50.2 E05-W00 N25-N31
4 961 1535 (N21E19 L= 88) 213 68 1 ( 928/1517- 994/1553) 14.0 E20-E16 N18-N21
5 1046 1413 (N16E10 L= 97) 471 161 0 (1019/1339-1070/1492) -60.9 E13-E07 N10-N19
6 468 1379 (S01E44 L= 63) 375 109 0 ( 431/1342- 502/1416) -8.1 E47-E40 S02-N01
7 835 1146 (S05E14 L= 93) 439 114 0 ( 806/1087- 856/1206) -74.1 E15-E12 S08-S01
8 1599 1180 (N19W30 L=136) 359 97 0 (1569/1140-1635/1206) 63.4 W28-W32 N15-N21
9 283 946 (S29E48 L= 59) 3865 736 5 ( 127/ 777- 393/1155) 52.1 E63-E40 S42-S15
10 1593 999 (N09W34 L=140) 312 81 1 (1563/ 975-1633/1020) 45.0 W31-W36 N06-N10
11 1011 984 (S09W00 L=107) 218 109 0 ( 975/ 926-1037/1010) -36.9 E02-W03 S11-S07
12 591 798 (S31E21 L= 86) 832 264 2 ( 528/ 688- 662/ 919) 72.6 E23-E18 S38-S22
13 1732 876 (N07W48 L=154) 436 99 0 (1689/ 845-1762/ 909) 56.3 W45-W49 N03-N09
14 903 812 (S22E01 L=106) 539 185 1 ( 819/ 763- 992/ 877) 61.4 E04-W02 S26-S15
15 1152 752 (S18W15 L=122) 413 193 0 (1068/ 710-1264/ 776) 45.0 W11-W20 S22-S13
16 1647 730 (S04W47 L=153) 264 80 0 (1615/ 703-1677/ 748) 63.4 W44-W49 S06-S02
17 1524 589 (S15W44 L=151) 268 79 0 (1489/ 574-1557/ 612) 45.0 W41-W46 S16-S12
18 1704 486 (S14W65 L=172) 439 72 1 (1683/ 465-1730/ 510) 63.4 W62-W67 S15-S11
19 1253 466 (S30W33 L=140) 1174 210 5 (1144/ 426-1372/ 499) 36.9 W27-W39 S34-S25
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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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