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| 20140330 - Filament data for 16 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
1 575 1680 (N20E50 L= 51) 382 132 0 ( 548/1637- 596/1717) -35.5 E54-E47 N17-N22
2 933 1509 (N18E19 L= 82) 750 198 1 ( 905/1418- 958/1600) -57.5 E22-E15 N13-N24
3 307 1541 (N06E68 L= 34) 2244 247 7 ( 256/1471- 369/1599) 66.0 E73-E63 N01-N10
4 1302 1506 (N29W02 L=104) 683 124 2 (1268/1443-1329/1564) -54.5 E01-W05 N25-N32
5 1121 1371 (N15E04 L= 97) 531 188 0 (1086/1299-1138/1460) -53.1 E08-E01 N10-N19
6 514 1381 (N01E41 L= 61) 305 54 1 ( 486/1357- 540/1411) 0.0 E43-E38 N00-N02
7 907 1101 (S06E09 L= 93) 517 108 2 ( 875/1045- 932/1162) -82.9 E09-E06 S09-S01
8 315 904 (S31E44 L= 57) 3217 642 8 ( 160/ 759- 447/1073) 45.0 E60-E35 S42-S18
9 1664 970 (N09W40 L=141) 399 120 1 (1626/ 940-1699/1013) 71.6 W37-W42 N06-N12
10 1868 938 (N15W59 L=160) 537 76 1 (1846/ 904-1886/ 977) -76.0 W56-W61 N13-N17
11 1753 833 (N05W51 L=153) 791 223 2 (1656/ 792-1815/ 880) 39.3 W44-W55 N00-N09
12 650 769 (S31E16 L= 86) 811 272 2 ( 576/ 670- 728/ 877) 69.4 E19-E12 S38-S22
13 982 783 (S21W05 L=106) 679 198 0 ( 879/ 724-1064/ 840) 57.5 W00-W07 S26-S15
14 1694 710 (S03W51 L=153) 330 57 1 (1673/ 685-1718/ 733) 56.3 W49-W53 S04-S01
15 1171 692 (S20W18 L=120) 306 65 1 (1134/ 661-1206/ 721) 59.0 W16-W19 S22-S17
16 1566 558 (S15W49 L=150) 384 66 1 (1528/ 537-1597/ 580) 36.9 W46-W50 S16-S13
17 1719 521 (S11W65 L=166) 496 129 1 (1691/ 487-1738/ 545) -63.4 W60-W68 S13-S09
18 1301 435 (S31W38 L=139) 1456 294 4 (1188/ 390-1415/ 473) 37.6 W31-W44 S35-S25
19 1536 407 (S24W56 L=157) 538 85 1 (1500/ 380-1577/ 440) 71.6 W53-W57 S26-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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