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| 20141116 - Latest Filament data |
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Available data for 20141116: »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC »13 UTC »14 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 867 1454 (N31W00 L=291) 229 70 0 ( 827/1437- 909/1467) -11.3 E02-W03 N30-N32
2 1313 1272 (N10W22 L=313) 704 181 2 (1229/1239-1406/1305) -21.8 W17-W27 N07-N12
3 920 1211 (N15E02 L=288) 1223 324 1 ( 757/1170-1073/1243) -9.0 E12-W07 N10-N18
4 1000 1115 (N08W00 L=291) 212 76 0 ( 970/1076-1034/1154) 36.9 E01-W03 N06-N09
5 1778 1003 (S16W49 L=339) 581 107 1 (1756/ 948-1797/1059) 50.2 W45-W51 S18-S12
6 169 995 (N18E61 L=229) 1142 278 1 ( 110/ 955- 229/1022) -4.1 E68-E54 N15-N19
7 452 950 (N10E37 L=254) 477 145 0 ( 396/ 878- 503/1014) -66.0 E39-E34 N05-N14
8 309 851 (N07E50 L=240) 583 91 1 ( 290/ 806- 342/ 890) 59.0 E52-E47 N04-N09
9 1253 854 (S12W09 L=300) 215 51 0 (1229/ 826-1280/ 877) 45.0 W07-W11 S13-S10
10 1257 646 (S24W06 L=296) 976 228 1 (1183/ 542-1326/ 730) 36.9 E01-W11 S29-S19
11 515 647 (S08E40 L=250) 286 55 1 ( 496/ 624- 537/ 677) -90.0 E41-E38 S10-S06
12 664 583 (S15E32 L=258) 645 156 3 ( 598/ 525- 734/ 641) -60.9 E35-E28 S20-S10
13 460 606 (S10E46 L=245) 706 133 2 ( 415/ 575- 508/ 636) -7.1 E49-E41 S12-S07
14 340 528 (S12E60 L=230) 2509 432 12 ( 275/ 469- 409/ 604) -56.3 E66-E54 S16-S07
15 455 535 (S14E49 L=241) 400 81 2 ( 433/ 507- 483/ 560) 21.8 E51-E46 S15-S12
16 626 496 (S20E38 L=252) 920 265 1 ( 518/ 412- 674/ 537) -56.3 E44-E33 S25-S15
17 1111 346 (S42E13 L=278) 488 110 1 (1087/ 301-1130/ 384) 76.0 E14-E10 S45-S37
18 800 260 (S40E39 L=251) 361 73 0 ( 783/ 231- 823/ 288) 68.2 E41-E36 S42-S37
19 1022 211 (S50E28 L=263) 790 143 1 ( 994/ 170-1064/ 248) 22.6 E33-E21 S53-S47
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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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