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| 20150706 - Filament data for 08 UTC |
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Available data for 20150706: »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 1214 1631 (N44W15 L=128) 1109 273 6 (1163/1546-1253/1697) 71.6 W11-W18 N37-N49
2 1544 1606 (N41W44 L=157) 1071 184 3 (1509/1543-1577/1664) 59.0 W41-W47 N36-N46
3 463 1543 (N35E46 L= 66) 348 65 1 ( 444/1520- 492/1563) -11.3 E48-E43 N33-N36
4 1718 1460 (N30W55 L=167) 641 159 3 (1693/1423-1740/1500) 50.2 W51-W57 N27-N33
5 733 1447 (N30E21 L= 91) 316 96 2 ( 712/1403- 747/1493) -80.5 E22-E19 N26-N32
6 421 1395 (N25E45 L= 67) 359 78 1 ( 397/1357- 455/1428) 68.2 E46-E42 N22-N27
7 1356 1308 (N21W22 L=134) 461 112 2 (1311/1265-1417/1341) -39.8 W19-W25 N18-N23
8 1822 1226 (N15W60 L=173) 519 76 1 (1799/1200-1849/1259) -38.7 W57-W63 N13-N17
9 512 1223 (N15E35 L= 78) 383 59 0 ( 486/1189- 556/1248) 36.9 E36-E31 N12-N16
10 1376 1216 (N15W23 L=135) 349 128 2 (1312/1188-1424/1246) 14.0 W18-W26 N13-N17
11 635 1181 (N12E25 L= 87) 243 93 0 ( 616/1131- 666/1232) 71.6 E26-E23 N09-N15
12 544 1176 (N12E32 L= 80) 223 100 -1 ( 517/1152- 562/1197) -33.7 E33-E30 N10-N13
13 1303 1120 (N09W17 L=130) 578 263 0 (1224/1072-1445/1188) -26.6 W12-W26 N06-N13
14 320 1027 (N02E49 L= 63) 537 148 0 ( 268/ 984- 353/1089) 36.9 E54-E45 S01-N05
15 243 720 (S18E59 L= 53) 526 99 1 ( 229/ 674- 261/ 765) 80.5 E60-E57 S21-S15
16 512 647 (S22E35 L= 77) 413 110 0 ( 467/ 624- 563/ 682) -15.9 E38-E31 S23-S19
17 340 612 (S25E51 L= 61) 672 215 1 ( 282/ 592- 403/ 640) 13.0 E57-E44 S26-S22
18 820 377 (S41E16 L= 96) 1365 268 2 ( 728/ 323- 924/ 452) 30.1 E25-E06 S46-S34
19 1535 368 (S42W46 L=158) 1171 212 2 (1454/ 338-1613/ 412) 8.1 W38-W53 S44-S38
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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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