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| 20140612 - Filament data for 10 UTC |
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Available data for 20140612: »06 UTC »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 1070 1764 (N53E10 L=196) 389 92 1 (1035/1736-1106/1783) 50.2 E12-E06 N49-N55
2 371 1583 (N27E60 L=146) 844 145 1 ( 342/1543- 407/1633) 80.5 E62-E56 N24-N30
3 1662 1559 (N45W48 L=254) 638 142 1 (1626/1540-1688/1583) 24.0 W43-W52 N43-N47
4 1531 1413 (N32W31 L=238) 761 183 1 (1449/1373-1608/1450) -4.4 W24-W37 N29-N33
5 574 1342 (N14E34 L=173) 367 93 1 ( 560/1295- 594/1390) -71.6 E35-E32 N11-N17
6 1891 1097 (N15W66 L=272) 2614 281 5 (1867/1013-1926/1205) -67.4 W62-W73 N10-N22
7 1824 1120 (N16W57 L=264) 487 124 2 (1797/1088-1847/1148) 45.0 W54-W60 N13-N17
8 1850 902 (N03W63 L=270) 2569 341 6 (1806/ 781-1897/1027) -57.3 W56-W68 S04-N10
9 191 893 (S18E61 L=145) 1508 249 4 ( 138/ 838- 230/ 992) -39.3 E69-E56 S21-S12
10 237 926 (S15E56 L=151) 556 126 2 ( 206/ 883- 276/ 966) -51.3 E59-E51 S17-S12
11 1022 861 (S09W02 L=208) 194 62 0 (1008/ 825-1036/ 897) 90.0 W01-W02 S11-S06
12 357 783 (S23E44 L=162) 804 198 3 ( 308/ 722- 414/ 819) 16.7 E48-E38 S26-S19
13 1612 666 (S14W45 L=252) 2375 460 7 (1486/ 511-1738/ 780) 62.2 W39-W55 S25-S06
14 908 721 (S19E04 L=203) 594 222 0 ( 818/ 694-1028/ 753) 4.8 E09-W03 S21-S16
15 1469 732 (S12W33 L=239) 304 91 0 (1431/ 718-1514/ 746) 11.3 W30-W36 S12-S10
16 1674 631 (S16W52 L=258) 900 174 2 (1623/ 604-1732/ 663) 18.4 W47-W58 S17-S13
17 1296 634 (S20W23 L=229) 250 39 0 (1269/ 616-1322/ 655) 33.7 W21-W24 S21-S18
18 634 534 (S36E22 L=184) 482 152 1 ( 581/ 504- 679/ 588) 32.0 E26-E18 S38-S31
19 1609 539 (S22W50 L=256) 323 86 1 (1588/ 509-1625/ 568) 90.0 W47-W51 S24-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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