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| 20230310 - Filament data for 08 UTC |
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Available data for 20230310: »07 UTC »08 UTC »10 UTC »11 UTC »12 UTC »13 UTC »14 UTC »15 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 722 1765 (N30E45 L=140) 1899 348 0 ( 641/1665- 811/1825) -81.9 E51-E35 N21-N36
2 1142 1727 (N39E14 L=171) 647 127 1 (1096/1670-1173/1779) -32.5 E20-E09 N35-N42
3 711 1637 (N21E37 L=148) 368 86 2 ( 671/1606- 733/1662) -18.4 E40-E34 N19-N23
4 333 1512 (N06E62 L=123) 936 120 1 ( 285/1475- 377/1563) 50.2 E66-E58 N03-N10
5 1702 1398 (N35W36 L=221) 812 276 1 (1658/1265-1734/1502) -68.2 W32-W40 N26-N41
6 237 1129 (S18E57 L=128) 339 85 1 ( 217/1084- 256/1166) 59.0 E59-E55 S20-S15
7 1822 1067 (N18W52 L=237) 752 153 0 (1800/1000-1844/1143) 90.0 W49-W55 N14-N23
8 436 971 (S24E36 L=149) 458 118 2 ( 409/ 937- 482/1013) -18.4 E38-E32 S25-S21
9 656 909 (S22E19 L=166) 538 200 1 ( 602/ 818- 686/ 987) -48.8 E24-E16 S27-S18
10 182 867 (S34E64 L=121) 1022 153 1 ( 146/ 804- 206/ 934) 33.7 E72-E59 S38-S30
11 1416 838 (S07W27 L=212) 298 61 0 (1398/ 799-1433/ 875) -78.7 W25-W28 S09-S04
12 310 812 (S36E47 L=138) 384 110 0 ( 285/ 766- 346/ 864) -39.8 E49-E43 S38-S32
13 1585 657 (S11W45 L=230) 1002 248 1 (1482/ 595-1691/ 705) 47.5 W40-W51 S17-S05
14 1719 646 (S08W57 L=242) 374 39 2 (1700/ 623-1741/ 670) -45.0 W54-W59 S08-S06
15 1292 521 (S28W32 L=217) 475 136 0 (1229/ 496-1351/ 554) 39.8 W28-W35 S30-S24
16 1498 392 (S28W55 L=240) 1732 292 1 (1363/ 357-1625/ 425) 15.9 W44-W72 S32-S24
17 596 345 (S64E15 L=170) 1421 183 5 ( 525/ 304- 687/ 391) 4.8 E26-E02 S66-S60
18 1184 345 (S42W37 L=222) 1133 175 4 (1110/ 318-1262/ 378) 33.7 W29-W42 S44-S37
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Download FITS filament maps as tar archive
» All Filament Data of 20230310 ...
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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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