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| 20150608 - Filament data for 08 UTC |
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Available data for 20150608: »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 1136 1684 (N46E04 L=119) 1424 288 5 (1091/1605-1180/1774) -70.3 E07-W01 N39-N54
2 611 1721 (N39E47 L= 76) 458 109 0 ( 589/1685- 633/1748) -26.6 E51-E43 N36-N40
3 521 1544 (N25E45 L= 78) 1986 332 5 ( 399/1473- 622/1668) 54.5 E53-E40 N19-N35
4 1482 1580 (N44W28 L=151) 718 156 0 (1419/1559-1534/1608) 26.6 W21-W33 N41-N47
5 552 1415 (N17E38 L= 85) 521 146 1 ( 492/1378- 594/1472) 50.2 E41-E35 N14-N20
6 1464 1424 (N32W25 L=148) 392 109 0 (1439/1376-1480/1466) -90.0 W22-W26 N28-N34
7 920 1301 (N15E11 L=112) 287 107 0 ( 865/1289- 977/1315) 7.1 E14-E06 N14-N16
8 686 1253 (N09E24 L= 98) 308 89 1 ( 665/1219- 710/1287) -53.1 E25-E22 N06-N11
9 1173 1218 (N14W06 L=129) 565 128 1 (1111/1180-1211/1267) 26.6 W02-W08 N10-N16
10 1107 1163 (N10W03 L=126) 211 52 1 (1077/1141-1133/1178) -18.4 W01-W04 N08-N10
11 1263 1044 (N05W14 L=137) 510 147 1 (1217/ 970-1293/1105) -49.4 W10-W16 N00-N08
12 231 968 (S14E56 L= 67) 769 206 0 ( 203/ 876- 245/1063) 80.5 E58-E54 S20-S08
13 384 1007 (S10E42 L= 81) 404 113 2 ( 341/ 982- 419/1023) 0.0 E45-E39 S11-S09
14 1631 918 (N02W41 L=164) 566 109 2 (1611/ 868-1660/ 971) -51.3 W39-W44 N00-N05
15 806 895 (S11E11 L=111) 379 171 0 ( 717/ 877- 882/ 918) 16.7 E17-E07 S11-S08
16 1173 799 (S11W12 L=135) 727 172 1 (1124/ 729-1215/ 885) -60.9 W09-W15 S15-S06
17 1607 741 (S09W43 L=166) 377 103 0 (1582/ 681-1641/ 784) 74.1 W41-W44 S12-S05
18 1714 686 (S11W54 L=177) 420 66 1 (1689/ 650-1738/ 715) 63.4 W52-W55 S12-S08
19 675 565 (S34E18 L=105) 305 66 2 ( 643/ 548- 706/ 586) 21.8 E20-E15 S35-S32
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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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