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| 20140417 - Filament data for 08 UTC |
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Available data for 20140417: »06 UTC »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC »13 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 448 1641 (N16E59 L=169) 1742 351 4 ( 325/1543- 537/1707) 49.8 E66-E54 N07-N21
2 929 1575 (N23E22 L=206) 265 90 0 ( 908/1540- 959/1614) -80.5 E23-E21 N20-N26
3 643 1570 (N16E40 L=188) 285 98 0 ( 611/1531- 666/1597) -23.2 E43-E36 N13-N16
4 584 1437 (N06E38 L=190) 503 109 2 ( 537/1415- 636/1462) 33.7 E41-E35 N04-N09
5 1497 1287 (N23W21 L=249) 644 167 1 (1449/1212-1534/1376) -41.6 W15-W24 N19-N27
6 1187 1301 (N14W01 L=229) 457 154 2 (1124/1245-1230/1368) 84.3 W00-W02 N09-N19
7 413 1152 (S14E41 L=187) 1434 450 1 ( 266/1046- 490/1322) 65.8 E51-E37 S22-S02
8 752 1036 (S12E16 L=212) 253 104 1 ( 702/1019- 807/1048) 33.7 E18-E12 S14-S10
9 856 842 (S20E04 L=224) 205 50 0 ( 827/ 817- 887/ 866) -14.0 E06-E02 S20-S18
10 1248 798 (S11W19 L=247) 209 65 1 (1211/ 781-1278/ 813) 26.6 W16-W20 S12-S10
11 827 759 (S26E04 L=224) 243 80 0 ( 812/ 716- 846/ 798) -53.1 E05-E01 S27-S23
12 254 765 (S41E50 L=178) 625 136 0 ( 220/ 744- 304/ 795) 6.3 E53-E44 S42-S39
13 1098 631 (S25W16 L=244) 510 193 0 (1004/ 565-1163/ 702) -12.1 W08-W22 S27-S23
14 930 599 (S32W07 L=235) 1093 282 0 ( 795/ 524-1066/ 700) -5.2 E04-W18 S33-S29
15 1550 586 (S14W46 L=274) 620 66 1 (1517/ 550-1591/ 616) 59.0 W43-W48 S16-S11
16 1058 242 (S51W37 L=265) 2755 464 6 ( 994/ 155-1140/ 345) -14.0 W24-W52 S56-S45
17 1427 316 (S32W54 L=282) 411 44 0 (1408/ 295-1455/ 331) 71.6 W51-W55 S33-S30
18 1348 279 (S37W51 L=279) 792 126 1 (1318/ 239-1379/ 317) -39.8 W47-W54 S40-S35
19 1200 244 (S45W46 L=274) 847 135 1 (1170/ 212-1239/ 289) -11.3 W40-W50 S47-S42
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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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