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| 20150423 - Filament data for 06 UTC |
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Available data for 20150423: »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 1220 1764 (N48E13 L=359) 432 82 2 (1181/1745-1262/1782) 26.6 E15-E09 N45-N50
2 495 1683 (N20E58 L=315) 1936 206 4 ( 433/1635- 571/1755) 68.2 E62-E53 N16-N26
3 1369 1533 (N35W07 L= 19) 3108 662 12 (1264/1366-1451/1711) -39.3 E06-W16 N25-N45
4 731 1552 (N18E33 L=339) 727 212 1 ( 709/1476- 771/1634) -45.0 E37-E27 N13-N22
5 480 1595 (N14E53 L=319) 555 116 2 ( 449/1562- 507/1633) -78.7 E55-E49 N11-N16
6 566 1456 (N08E40 L=332) 445 131 4 ( 526/1400- 598/1515) 90.0 E41-E38 N03-N11
7 474 1478 (N07E48 L=325) 530 103 1 ( 439/1446- 511/1510) 45.0 E50-E45 N04-N09
8 1780 1195 (N27W45 L= 57) 453 81 1 (1755/1145-1798/1238) -59.0 W42-W47 N24-N29
9 648 1094 (S11E23 L=349) 224 56 0 ( 621/1061- 669/1132) 90.0 E24-E22 S13-S08
10 1718 1042 (N16W43 L= 55) 470 100 3 (1697/ 999-1744/1090) -38.7 W39-W45 N14-N18
11 1888 922 (N15W63 L= 76) 2870 379 7 (1845/ 809-1923/1037) -42.7 W58-W73 N10-N22
12 268 932 (S29E49 L=323) 1052 292 0 ( 206/ 850- 356/1000) 47.5 E55-E41 S35-S23
13 879 946 (S13E06 L= 6) 357 143 0 ( 801/ 911- 942/ 986) 53.1 E09-E03 S17-S09
14 1563 876 (N02W36 L= 48) 275 102 0 (1516/ 861-1610/ 892) 26.6 W32-W38 N00-N03
15 1161 825 (S12W13 L= 25) 226 81 0 (1121/ 804-1191/ 852) 36.9 W10-W14 S13-S09
16 289 764 (S39E46 L=326) 460 79 3 ( 261/ 740- 314/ 790) -11.3 E49-E43 S41-S37
17 1401 706 (S12W31 L= 43) 669 204 1 (1308/ 630-1495/ 750) 59.7 W28-W36 S18-S06
18 1103 725 (S19W13 L= 25) 412 176 2 (1011/ 709-1189/ 745) 20.0 W07-W18 S21-S16
19 1179 589 (S25W22 L= 35) 637 179 0 (1089/ 573-1264/ 610) 33.7 W16-W26 S27-S21
20 1332 437 (S29W39 L= 51) 318 87 1 (1294/ 424-1377/ 453) 18.4 W36-W42 S29-S26
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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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