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| 20140707 - Latest Filament data |
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Available data for 20140707: »05 UTC »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
1 820 1277 (N19E13 L=220) 547 122 1 ( 790/1244- 877/1324) -33.7 E15-E09 N17-N22
2 1548 1253 (N17W36 L=270) 594 176 0 (1519/1169-1567/1319) 78.7 W33-W37 N11-N21
3 1376 1281 (N19W23 L=257) 324 70 0 (1337/1256-1410/1305) 21.8 W20-W25 N17-N20
4 1444 1158 (N11W27 L=261) 507 182 1 (1376/1135-1532/1200) -15.3 W22-W33 N10-N14
5 511 1168 (N12E34 L=200) 228 91 0 ( 470/1154- 549/1181) 0.0 E37-E31 N10-N12
6 1642 1130 (N09W42 L=276) 407 71 0 (1620/1100-1666/1166) -90.0 W40-W43 N07-N11
7 136 1123 (N07E73 L=161) 1050 182 2 ( 116/1096- 162/1165) -24.0 E77-E68 N05-N09
8 358 955 (S02E46 L=188) 1266 222 3 ( 288/ 912- 441/1015) -8.7 E52-E38 S04-N01
9 795 976 (N00E14 L=220) 295 65 1 ( 771/ 935- 812/1005) -63.4 E15-E13 S02-N02
10 1442 850 (S07W27 L=261) 222 89 0 (1426/ 816-1478/ 876) 45.0 W25-W29 S09-S05
11 1034 809 (S10W01 L=235) 573 171 2 ( 991/ 724-1079/ 874) 68.2 E02-W03 S15-S05
12 1761 780 (S13W54 L=287) 1134 136 1 (1724/ 712-1794/ 849) 66.0 W50-W56 S17-S08
13 1502 787 (S12W31 L=265) 299 96 0 (1478/ 747-1525/ 836) -71.6 W29-W33 S14-S08
14 659 680 (S18E24 L=210) 267 63 0 ( 624/ 650- 688/ 708) -45.0 E26-E22 S20-S16
15 1414 583 (S25W27 L=261) 261 76 0 (1397/ 547-1430/ 631) 90.0 W26-W28 S27-S21
16 1642 583 (S26W46 L=280) 450 64 0 (1610/ 563-1671/ 613) 36.9 W43-W48 S27-S23
17 306 530 (S31E59 L=175) 537 109 1 ( 292/ 500- 332/ 558) 68.2 E60-E55 S33-S28
18 369 469 (S35E54 L=179) 510 87 0 ( 350/ 434- 385/ 503) 68.2 E56-E52 S37-S32
19 1092 409 (S38W05 L=239) 542 141 0 (1038/ 376-1143/ 460) 45.0 W01-W08 S40-S33
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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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