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| 20141116 - Filament data for 08 UTC |
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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
1 697 1550 (N42E10 L=283) 323 76 0 ( 670/1515- 733/1576) 53.1 E12-E06 N39-N43
2 1767 1530 (N14W68 L= 1) 1357 279 4 (1742/1469-1799/1572) 24.4 W62-W74 N10-N16
3 821 1439 (N31E03 L=290) 314 105 0 ( 764/1425- 875/1451) -15.9 E07-W00 N29-N32
4 1279 1249 (N10W20 L=313) 841 132 4 (1189/1218-1388/1277) -28.6 W14-W25 N05-N12
5 871 1193 (N16E05 L=288) 1353 329 2 ( 703/1148-1031/1226) -11.3 E16-W04 N11-N18
6 952 1095 (N08E03 L=291) 180 87 0 ( 919/1053- 986/1132) 31.0 E05-W00 N06-N09
7 1744 963 (S17W45 L=338) 644 123 0 (1714/ 885-1769/1021) 45.0 W41-W47 S21-S13
8 133 993 (N18E65 L=228) 936 226 0 ( 89/ 968- 185/1014) -14.0 E71-E59 N16-N19
9 380 985 (N13E41 L=252) 319 72 2 ( 348/ 954- 404/1009) -36.9 E43-E39 N11-N15
10 280 840 (N07E53 L=240) 598 87 2 ( 253/ 811- 315/ 868) 0.0 E56-E49 N05-N08
11 1352 797 (S17W14 L=308) 267 121 0 (1342/ 733-1376/ 849) 66.8 W12-W16 S21-S14
12 1211 651 (S23W03 L=296) 1320 290 3 (1130/ 505-1291/ 759) 54.5 E05-W08 S30-S15
13 560 587 (S13E39 L=254) 1090 322 5 ( 463/ 476- 651/ 667) -74.1 E44-E35 S20-S06
14 411 562 (S11E51 L=242) 1985 382 6 ( 337/ 499- 474/ 627) 12.1 E59-E45 S15-S07
15 308 532 (S11E63 L=230) 2043 281 7 ( 262/ 468- 362/ 599) -63.4 E67-E58 S15-S07
16 674 550 (S17E33 L=261) 385 90 1 ( 643/ 505- 700/ 586) 51.3 E34-E29 S20-S15
17 555 502 (S18E43 L=250) 407 108 1 ( 492/ 486- 599/ 514) -14.0 E47-E39 S19-S16
18 1079 325 (S42E16 L=277) 554 163 2 (1050/ 281-1106/ 375) 69.4 E18-E12 S45-S37
19 1001 200 (S51E30 L=263) 971 190 2 ( 972/ 158-1033/ 248) 52.1 E35-E24 S55-S46
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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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