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| 20240314 - Filament data for 09 UTC |
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Available data for 20240314: »05 UTC »06 UTC »07 UTC »08 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
1 813 1794 (N35E42 L=299) 538 66 0 ( 794/1761- 833/1828) -56.3 E44-E38 N31-N37
2 623 1743 (N26E52 L=289) 844 189 3 ( 542/1703- 708/1775) 48.4 E57-E45 N21-N30
3 714 1712 (N26E42 L=299) 321 53 1 ( 699/1679- 734/1742) -59.0 E43-E40 N23-N28
4 1013 1524 (N21E15 L=326) 729 234 0 ( 919/1454-1100/1552) 4.8 E19-E07 N18-N23
5 784 1434 (N10E25 L=316) 607 243 1 ( 749/1333- 819/1535) -45.0 E30-E19 N04-N15
6 607 1363 (N02E33 L=308) 294 69 1 ( 588/1333- 636/1397) -36.9 E35-E30 N00-N03
7 1711 1328 (N31W37 L= 18) 1265 195 3 (1645/1256-1772/1393) -17.1 W30-W44 N27-N33
8 1430 1160 (N11W19 L= 0) 631 171 0 (1409/1076-1463/1236) -78.7 W17-W21 N06-N16
9 461 1167 (S12E38 L=303) 469 148 0 ( 402/1148- 533/1189) 21.8 E42-E32 S14-S10
10 1626 1071 (N12W34 L= 15) 767 232 0 (1574/ 974-1680/1166) -33.7 W28-W40 N08-N16
11 207 1103 (S21E61 L=280) 686 112 0 ( 160/1056- 235/1148) 36.9 E66-E57 S23-S17
12 654 966 (S20E20 L=321) 390 103 0 ( 604/ 948- 703/1000) 45.0 E23-E17 S21-S16
13 432 904 (S28E35 L=305) 428 119 0 ( 374/ 883- 490/ 933) 21.8 E40-E30 S30-S25
14 601 727 (S35E19 L=322) 823 192 2 ( 532/ 685- 675/ 766) 38.7 E24-E14 S38-S30
15 1736 531 (S12W67 L= 48) 567 113 0 (1689/ 494-1782/ 567) 54.5 W64-W70 S15-S08
16 1356 485 (S27W39 L= 20) 1274 227 3 (1263/ 441-1457/ 543) 54.0 W34-W42 S32-S20
17 1521 319 (S30W66 L= 47) 638 120 1 (1468/ 292-1582/ 344) 49.4 W61-W70 S33-S26
18 1128 328 (S44W35 L= 16) 398 56 0 (1096/ 313-1165/ 342) 18.4 W31-W37 S45-S42
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Download FITS filament maps as tar archive
» All Filament Data of 20240314 ...
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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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