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| 20140331 - Filament data for 07 UTC |
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Available data for 20140331: »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
1 323 1598 (N10E70 L= 23) 1117 285 4 ( 287/1530- 344/1641) -38.7 E77-E64 N05-N13
2 1045 1456 (N18E11 L= 82) 687 228 1 (1023/1351-1066/1557) -59.7 E14-E07 N12-N24
3 342 1483 (N03E59 L= 33) 684 140 1 ( 296/1443- 383/1526) 50.2 E63-E56 N00-N06
4 1412 1473 (N31W10 L=103) 468 70 1 (1381/1430-1433/1507) -53.1 W08-W12 N28-N33
5 1216 1362 (N17W01 L= 94) 774 238 0 (1131/1247-1260/1461) -36.9 E06-W06 N11-N21
6 667 1285 (S01E27 L= 66) 205 62 0 ( 642/1259- 688/1310) -14.0 E29-E25 S02-N00
7 1764 1102 (N20W44 L=137) 550 110 2 (1725/1072-1806/1129) 45.0 W40-W47 N17-N22
8 1040 1035 (S06W01 L= 94) 335 73 0 (1015/ 991-1065/1079) 90.0 W00-W01 S08-S02
9 390 866 (S32E37 L= 56) 2860 650 8 ( 203/ 751- 536/1018) 41.5 E55-E28 S43-S19
10 1744 909 (N09W48 L=141) 372 105 1 (1710/ 883-1781/ 932) 45.0 W45-W50 N06-N11
11 756 717 (S31E07 L= 86) 984 268 1 ( 676/ 616- 850/ 823) 73.6 E10-E04 S39-S22
12 1793 766 (N03W58 L=151) 1111 310 0 (1688/ 733-1870/ 821) 33.7 W48-W64 S01-N09
13 1096 718 (S21W13 L=106) 784 209 2 ( 984/ 667-1171/ 780) 57.5 W08-W16 S26-S15
14 1354 711 (S14W28 L=121) 406 161 0 (1295/ 667-1419/ 766) -10.3 W22-W33 S15-S12
15 1692 578 (S10W58 L=151) 1837 342 5 (1591/ 481-1799/ 684) 62.1 W53-W64 S17-N00
16 1298 639 (S19W28 L=120) 423 108 0 (1245/ 604-1364/ 670) 54.5 W25-W30 S22-S15
17 1126 559 (S29W21 L=114) 240 83 0 (1080/ 548-1169/ 572) 31.0 W18-W23 S30-S27
18 1403 381 (S30W48 L=141) 2065 308 3 (1282/ 340-1532/ 440) 49.8 W40-W53 S35-S22
19 1564 350 (S25W62 L=155) 469 60 0 (1537/ 320-1597/ 373) 78.7 W59-W63 S27-S22
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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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