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| 20140827 - Filament data for 11 UTC |
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Available data for 20140827: »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
1 562 1558 (N51E25 L=255) 297 68 2 ( 540/1534- 578/1580) -53.1 E27-E23 N48-N52
2 1576 1503 (N21W50 L=330) 893 151 3 (1516/1472-1632/1526) -32.0 W45-W53 N18-N23
3 1124 1474 (N31W18 L=298) 616 140 4 (1077/1415-1159/1514) -81.9 W15-W19 N27-N34
4 1556 1396 (N16W43 L=324) 1130 231 4 (1474/1309-1643/1461) -59.7 W39-W47 N08-N20
5 594 1313 (N33E23 L=258) 1499 365 4 ( 523/1173- 663/1453) -68.2 E28-E19 N23-N43
6 1779 1389 (N09W63 L=344) 1261 169 3 (1735/1318-1826/1449) -68.2 W61-W66 N03-N13
7 1746 1296 (N05W55 L=336) 1245 281 5 (1699/1163-1791/1401) 59.7 W47-W60 S01-N11
8 1272 1322 (N19W22 L=302) 500 110 1 (1226/1258-1311/1362) -81.9 W19-W23 N14-N21
9 1751 1052 (S09W48 L=329) 1030 245 0 (1694/ 997-1827/1129) -55.0 W44-W55 S13-S03
10 907 1093 (N13E05 L=275) 201 60 0 ( 875/1072- 945/1109) 14.0 E07-E03 N12-N14
11 189 1010 (N20E61 L=219) 3277 490 6 ( 103/ 901- 268/1086) -36.9 E71-E53 N12-N24
12 149 903 (N13E69 L=211) 576 82 2 ( 128/ 879- 170/ 923) -11.3 E72-E66 N11-N14
13 1786 875 (S20W48 L=329) 396 90 1 (1751/ 840-1811/ 912) 26.6 W44-W51 S21-S18
14 1376 740 (S17W15 L=296) 1517 308 2 (1289/ 613-1432/ 903) 47.0 W07-W21 S23-S08
15 445 828 (N06E41 L=240) 353 64 2 ( 421/ 801- 465/ 862) 71.6 E42-E39 N04-N07
16 457 641 (S06E45 L=236) 849 217 3 ( 382/ 614- 532/ 670) -4.8 E51-E39 S07-S04
17 305 488 (S14E68 L=212) 748 129 2 ( 280/ 450- 329/ 512) -59.0 E71-E64 S17-S12
18 800 454 (S23E28 L=253) 534 84 2 ( 763/ 424- 833/ 484) 9.5 E30-E24 S25-S21
19 1220 383 (S38E02 L=278) 388 46 0 (1191/ 363-1254/ 401) -26.6 E04-W00 S40-S36
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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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