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| 20150210 - Filament data for 12 UTC |
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Available data for 20150210: »07 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
1 796 1871 (N47E41 L=197) 890 167 1 ( 773/1833- 820/1912) -63.4 E45-E36 N43-N51
2 1063 1532 (N25E07 L=232) 839 171 1 (1017/1449-1120/1592) 74.7 E08-E04 N18-N29
3 420 1448 (N10E47 L=191) 888 195 0 ( 361/1361- 496/1527) 70.0 E50-E43 N04-N15
4 1678 1496 (N36W39 L=277) 701 105 1 (1637/1473-1720/1516) 12.5 W34-W43 N34-N38
5 1389 1429 (N24W16 L=254) 1029 190 0 (1331/1326-1441/1514) -48.0 W10-W20 N18-N29
6 1744 1467 (N36W45 L=283) 784 99 0 (1712/1442-1771/1494) 40.6 W41-W48 N33-N39
7 1767 1291 (N24W46 L=284) 347 79 0 (1740/1276-1797/1312) -11.3 W43-W48 N23-N25
8 1698 1215 (N18W40 L=278) 1098 176 2 (1664/1141-1725/1300) 78.7 W37-W42 N13-N23
9 426 1097 (S11E39 L=199) 1624 360 3 ( 343/ 921- 497/1265) 72.3 E43-E36 S22-N00
10 1220 1202 (N07W08 L=247) 517 91 0 (1176/1157-1261/1245) -26.6 W05-W11 N04-N09
11 141 1176 (S08E69 L=169) 872 182 3 ( 122/1135- 169/1230) -40.6 E74-E64 S10-S04
12 1906 1048 (N13W63 L=301) 546 78 0 (1885/1020-1927/1077) 53.1 W60-W65 N11-N15
13 118 930 (S23E67 L=171) 584 73 0 ( 101/ 902- 130/ 964) 90.0 E69-E65 S24-S20
14 188 818 (S30E59 L=180) 1528 435 0 ( 127/ 711- 251/ 918) 42.7 E66-E52 S35-S23
15 1365 789 (S14W25 L=263) 2817 676 1 (1040/ 728-1650/ 833) 14.0 W04-W45 S18-S08
16 776 661 (S32E10 L=229) 963 332 1 ( 617/ 630- 933/ 688) 23.6 E21-W00 S36-S28
17 567 610 (S39E25 L=213) 412 68 1 ( 536/ 580- 596/ 639) 59.0 E28-E22 S41-S36
18 470 571 (S43E34 L=204) 876 162 3 ( 401/ 539- 523/ 615) -16.7 E40-E29 S45-S40
19 1727 479 (S23W64 L=303) 2315 298 4 (1642/ 429-1801/ 529) 29.7 W56-W70 S26-S17
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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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