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| 20140930 - Filament data for 08 UTC |
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Available data for 20140930: »05 UTC »06 UTC »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 1445 1712 (N32W54 L=247) 990 189 2 (1384/1688-1515/1731) -20.0 W48-W59 N28-N34
2 1687 1563 (N15W64 L=257) 674 127 2 (1654/1530-1714/1591) -59.0 W60-W68 N12-N17
3 1026 1433 (N29W12 L=206) 340 91 1 ( 977/1409-1072/1463) 0.0 W08-W16 N28-N30
4 1502 1416 (N14W40 L=234) 2689 557 6 (1250/1376-1715/1446) -20.9 W23-W57 N06-N20
5 723 1263 (N28E12 L=182) 544 131 1 ( 685/1212- 774/1320) -82.9 E13-E08 N24-N32
6 1862 1202 (S09W63 L=256) 2217 340 6 (1817/1101-1911/1264) 84.3 W57-W72 S15-S04
7 1158 1072 (N06W09 L=202) 867 277 3 (1122/ 995-1233/1210) 85.6 W05-W12 N00-N13
8 1823 1107 (S13W54 L=248) 682 126 4 (1793/1059-1852/1159) -90.0 W50-W57 S16-S09
9 1768 1081 (S12W48 L=242) 1109 306 4 (1725/ 972-1832/1150) -81.3 W44-W52 S20-S07
10 1688 1054 (S11W41 L=234) 562 98 3 (1666/1002-1709/1105) 81.9 W38-W43 S14-S07
11 327 949 (N19E47 L=146) 386 60 0 ( 314/ 908- 341/ 992) 78.7 E48-E45 N16-N21
12 1539 788 (S21W24 L=217) 1833 410 3 (1440/ 631-1579/ 942) -90.0 W20-W26 S31-S09
13 465 550 (S07E49 L=144) 680 120 1 ( 425/ 516- 522/ 595) -60.3 E51-E45 S10-S03
14 278 531 (S05E70 L=123) 1014 166 2 ( 242/ 504- 333/ 571) -16.7 E74-E62 S07-S02
15 697 475 (S17E36 L=158) 624 252 0 ( 652/ 395- 740/ 566) 33.7 E42-E29 S20-S10
16 430 495 (S10E55 L=139) 327 115 0 ( 414/ 459- 463/ 543) -90.0 E56-E51 S12-S06
17 489 486 (S11E50 L=143) 471 85 0 ( 450/ 464- 533/ 517) -38.7 E52-E46 S13-S08
18 843 306 (S32E35 L=158) 2327 623 4 ( 684/ 186-1018/ 452) 16.1 E56-E18 S37-S25
19 574 380 (S20E49 L=144) 348 82 0 ( 532/ 366- 605/ 393) -26.6 E52-E46 S21-S18
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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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