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| 20140416 - Filament data for 09 UTC |
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Available data for 20140416: »05 UTC »06 UTC »07 UTC »08 UTC »09 UTC »10 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
1 775 1635 (N23E34 L=207) 315 140 1 ( 743/1574- 812/1687) -77.5 E35-E32 N18-N27
2 507 1623 (N16E53 L=188) 334 90 1 ( 484/1591- 524/1646) -18.4 E55-E49 N14-N17
3 466 1518 (N08E50 L=191) 889 201 4 ( 387/1481- 545/1569) 48.4 E56-E45 N04-N13
4 1226 1517 (N29E03 L=238) 262 41 1 (1199/1496-1249/1533) 18.4 E04-E01 N27-N30
5 1315 1388 (N23W07 L=247) 447 107 1 (1295/1346-1336/1448) -45.0 W03-W08 N20-N26
6 275 1178 (S15E54 L=187) 1136 304 0 ( 185/1091- 340/1310) 65.0 E60-E49 S21-S06
7 898 1179 (S00E11 L=230) 246 120 1 ( 876/1122- 928/1237) -45.0 E13-E08 S02-N02
8 267 1202 (S14E55 L=186) 328 56 0 ( 245/1171- 287/1233) 68.2 E56-E53 S16-S11
9 837 939 (S15E08 L=233) 205 77 1 ( 808/ 896- 855/ 973) -53.1 E09-E06 S17-S13
10 674 870 (S23E16 L=225) 494 89 3 ( 640/ 799- 712/ 936) -69.4 E18-E14 S27-S19
11 803 893 (S19E09 L=232) 387 68 0 ( 779/ 847- 821/ 928) -53.1 E11-E06 S20-S16
12 185 792 (S41E57 L=184) 607 152 1 ( 156/ 772- 219/ 814) 0.0 E60-E53 S41-S38
13 1406 693 (S13W32 L=273) 364 105 0 (1354/ 652-1452/ 729) 66.8 W29-W33 S16-S09
14 804 668 (S32E03 L=238) 327 98 0 ( 743/ 641- 840/ 693) 8.1 E07-W00 S32-S30
15 1687 497 (S13W63 L=304) 553 118 1 (1661/ 454-1705/ 556) -56.3 W59-W65 S16-S10
16 825 394 (S49W09 L=250) 665 160 0 ( 800/ 340- 872/ 457) -32.5 W05-W16 S52-S44
17 946 310 (S51W24 L=265) 1130 252 4 ( 917/ 240- 982/ 390) -47.5 W18-W30 S56-S44
18 1238 355 (S37W39 L=280) 362 69 0 (1217/ 328-1261/ 384) -21.8 W36-W41 S37-S35
19 1078 308 (S46W33 L=274) 487 73 2 (1050/ 278-1103/ 342) -51.3 W29-W35 S47-S42
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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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