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| 20230928 - Filament data for 10 UTC |
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Available data for 20230928: »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 1029 1776 (N52W34 L= 68) 390 46 1 (1007/1748-1051/1802) 51.3 W30-W36 N49-N54
2 1179 1760 (N45W42 L= 77) 819 103 1 (1143/1726-1225/1783) -51.3 W37-W46 N42-N47
3 1690 1532 (N14W64 L= 98) 854 119 3 (1635/1514-1748/1552) -12.1 W57-W71 N11-N16
4 1119 1367 (N23W15 L= 49) 346 88 1 (1084/1337-1155/1402) 9.5 W12-W18 N21-N25
5 1777 1310 (N00W58 L= 92) 756 137 3 (1746/1240-1799/1370) 81.9 W56-W60 S04-N03
6 853 1157 (N19E06 L= 28) 637 193 2 ( 794/1093- 912/1241) 24.4 E11-W00 N16-N21
7 1199 1139 (N08W13 L= 47) 263 71 3 (1175/1117-1221/1172) 45.0 W11-W14 N07-N10
8 282 1050 (N25E51 L=343) 1987 286 9 ( 242/ 930- 326/1165) 85.9 E55-E47 N18-N32
9 477 1066 (N22E33 L= 1) 760 253 3 ( 374/ 978- 543/1100) -45.0 E41-E28 N15-N26
10 1869 940 (S24W58 L= 92) 724 102 0 (1837/ 896-1891/ 993) 29.7 W53-W61 S25-S21
11 1551 855 (S17W27 L= 61) 1138 360 1 (1393/ 832-1721/ 882) -20.6 W16-W40 S22-S12
12 1140 767 (S11E00 L= 34) 223 43 0 (1121/ 740-1160/ 797) 45.0 E01-W01 S11-S09
13 1845 773 (S34W54 L= 89) 536 69 0 (1810/ 757-1883/ 792) -21.0 W49-W62 S36-S31
14 1041 585 (S19E11 L= 23) 260 118 0 (1031/ 521-1055/ 635) 60.3 E13-E09 S22-S15
15 698 521 (S14E34 L= 0) 805 258 0 ( 658/ 417- 740/ 625) 38.2 E41-E27 S19-S08
16 599 434 (S17E45 L=349) 328 67 1 ( 563/ 420- 632/ 454) -36.9 E46-E42 S18-S15
17 491 328 (S23E63 L=331) 1074 119 3 ( 456/ 289- 534/ 380) 74.1 E67-E60 S26-S18
18 576 332 (S24E54 L=340) 475 102 0 ( 527/ 313- 604/ 357) -18.4 E57-E49 S25-S22
19 772 308 (S30E41 L=353) 807 133 1 ( 728/ 253- 819/ 350) 22.6 E46-E34 S34-S27
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Download FITS filament maps as tar archive
» All Filament Data of 20230928 ...
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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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