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| 20141128 - Latest Filament data |
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Available data for 20141128: »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 1474 1703 (N34W49 L=182) 431 77 1 (1441/1676-1493/1726) -33.7 W46-W51 N31-N35
2 1087 1449 (N25W12 L=145) 1167 318 3 ( 968/1376-1195/1529) -45.0 W06-W18 N20-N32
3 561 1496 (N39E24 L=109) 497 95 1 ( 514/1472- 606/1513) -14.0 E28-E20 N36-N40
4 1720 1446 (N13W57 L=189) 833 96 1 (1681/1405-1752/1477) -59.0 W52-W60 N10-N15
5 1053 1226 (N12W05 L=138) 613 201 3 ( 967/1170-1155/1277) -48.4 W00-W10 N07-N16
6 1581 1040 (S08W34 L=167) 298 108 1 (1524/1013-1626/1060) -29.7 W30-W37 S09-S05
7 1251 936 (S08W12 L=144) 494 185 0 (1208/ 856-1289/1033) 52.1 W07-W14 S11-S02
8 1625 906 (S16W36 L=168) 601 157 1 (1587/ 836-1659/ 985) 49.4 W32-W38 S19-S12
9 184 954 (N11E61 L= 72) 1012 281 4 ( 116/ 919- 251/ 971) -14.0 E69-E53 N08-N12
10 1581 923 (S15W33 L=165) 263 74 1 (1556/ 894-1606/ 947) -76.0 W30-W34 S16-S12
11 272 903 (N07E52 L= 80) 308 56 2 ( 253/ 879- 293/ 924) 45.0 E54-E50 N05-N07
12 1466 725 (S24W23 L=155) 1109 327 0 (1294/ 680-1590/ 791) 2.6 W10-W32 S26-S22
13 1547 635 (S32W28 L=161) 1797 298 2 (1411/ 535-1673/ 749) 20.9 W17-W38 S36-S26
14 864 694 (S15E16 L=117) 216 92 0 ( 810/ 682- 910/ 706) -9.5 E18-E12 S15-S14
15 1831 676 (S36W55 L=188) 722 180 1 (1802/ 659-1874/ 704) -18.4 W51-W60 S37-S33
16 919 649 (S19E13 L=119) 273 104 0 ( 890/ 623- 953/ 690) -45.0 E14-E11 S20-S16
17 398 509 (S18E54 L= 79) 418 104 1 ( 379/ 464- 426/ 548) -90.0 E55-E51 S21-S15
18 543 484 (S22E43 L= 89) 437 119 3 ( 521/ 438- 568/ 534) 50.2 E46-E41 S25-S19
19 408 434 (S23E57 L= 75) 480 76 1 ( 373/ 406- 448/ 463) -51.3 E59-E54 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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