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| 20140321 - Latest Filament data |
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Available data for 20140321: »06 UTC »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »13 UTC »14 UTC »15 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 730 1579 (N17E34 L=187) 269 90 1 ( 699/1543- 755/1603) -31.0 E36-E31 N14-N18
2 663 1535 (N13E36 L=185) 256 57 2 ( 632/1517- 692/1555) 45.0 E37-E34 N11-N14
3 381 1480 (N04E55 L=166) 538 87 2 ( 354/1448- 412/1512) 76.0 E57-E53 N02-N06
4 505 1452 (N05E44 L=177) 443 56 2 ( 482/1424- 531/1474) -11.3 E46-E41 N02-N06
5 1240 1389 (N19W02 L=223) 336 65 1 (1209/1363-1265/1419) 63.4 W00-W03 N16-N21
6 246 1266 (S11E59 L=161) 1444 337 7 ( 219/1156- 272/1368) -53.1 E63-E53 S17-S04
7 1605 1125 (N15W31 L=252) 707 268 2 (1539/1041-1670/1241) -28.3 W24-W37 N12-N19
8 311 1161 (S16E50 L=171) 436 97 2 ( 270/1113- 339/1198) 80.5 E53-E47 S19-S13
9 971 1065 (S06E04 L=217) 429 188 0 ( 875/1031-1035/1087) 18.4 E09-W00 S08-S04
10 778 1018 (S14E14 L=207) 336 154 0 ( 718/ 944- 815/1063) -39.8 E18-E10 S17-S11
11 927 953 (S13E04 L=217) 204 96 0 ( 868/ 920- 968/ 975) 0.0 E07-W00 S14-S12
12 709 859 (S24E14 L=206) 302 148 0 ( 634/ 836- 766/ 897) 45.0 E18-E11 S27-S20
13 447 812 (S34E32 L=188) 555 162 1 ( 377/ 791- 512/ 833) 9.5 E38-E26 S35-S32
14 1053 655 (S27W13 L=233) 441 182 0 ( 961/ 637-1142/ 687) 20.0 W06-W17 S28-S23
15 1417 620 (S17W36 L=256) 1252 433 2 (1225/ 585-1588/ 653) 19.8 W23-W48 S22-S13
16 1702 546 (S12W61 L=282) 1549 298 8 (1669/ 479-1741/ 618) -53.1 W55-W67 S15-S07
17 1782 526 (S09W73 L=293) 836 94 0 (1758/ 488-1805/ 557) -76.0 W69-W77 S11-S07
18 1617 455 (S19W59 L=279) 1046 331 1 (1562/ 388-1667/ 518) -3.4 W50-W67 S21-S16
19 1414 466 (S26W43 L=264) 1001 309 4 (1271/ 443-1538/ 491) 27.9 W33-W50 S30-S20
20 1345 323 (S36W48 L=269) 720 208 1 (1258/ 297-1421/ 348) 12.1 W40-W54 S38-S33
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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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