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| 20230515 - Filament data for 07 UTC |
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Available data for 20230515: »06 UTC »07 UTC »08 UTC »09 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
1 811 1837 (N45E49 L=346) 1820 164 3 ( 734/1788- 875/1874) -2.6 E62-E38 N41-N47
2 1198 1796 (N54E13 L= 21) 360 62 1 (1167/1770-1220/1820) -15.9 E17-E10 N51-N55
3 1333 1736 (N53W02 L= 37) 399 54 1 (1307/1709-1356/1756) -53.1 W00-W04 N50-N55
4 1453 1665 (N51W16 L= 50) 930 121 3 (1410/1614-1504/1703) -33.7 W11-W21 N47-N53
5 1555 1618 (N51W28 L= 62) 775 97 3 (1518/1577-1592/1655) -63.4 W23-W32 N46-N53
6 983 1594 (N31E18 L= 16) 589 149 0 ( 934/1535-1033/1645) -24.4 E23-E12 N27-N33
7 736 1538 (N21E32 L= 3) 586 165 1 ( 711/1453- 770/1612) -70.0 E33-E28 N15-N26
8 1638 1567 (N49W37 L= 72) 999 99 4 (1603/1534-1680/1609) -12.5 W33-W43 N45-N52
9 1379 1521 (N37W11 L= 45) 1307 344 0 (1301/1449-1483/1574) 3.8 W05-W20 N29-N40
10 602 1463 (N13E38 L=357) 561 132 0 ( 587/1405- 628/1532) -41.2 E41-E33 N10-N17
11 419 1424 (N07E50 L=344) 524 82 2 ( 387/1390- 460/1454) 68.2 E52-E47 N04-N09
12 1010 1329 (N15E08 L= 26) 348 112 1 ( 972/1302-1074/1363) 0.0 E10-E03 N12-N16
13 1761 1248 (N29W47 L= 82) 1033 180 1 (1704/1183-1819/1307) -21.0 W41-W54 N26-N31
14 150 1151 (S14E71 L=323) 990 86 2 ( 112/1122- 193/1173) 10.6 E80-E64 S15-S11
15 227 969 (S23E57 L=337) 2147 378 1 ( 193/ 849- 306/1127) -60.6 E61-E47 S29-S13
16 1867 1072 (N21W61 L= 96) 478 101 1 (1829/1049-1906/1107) -4.4 W55-W68 N20-N22
17 777 942 (S13E13 L= 22) 227 84 2 ( 726/ 926- 817/ 958) 11.3 E15-E10 S14-S11
18 419 797 (S30E36 L=358) 347 104 0 ( 387/ 754- 465/ 828) 45.0 E39-E32 S33-S27
19 731 725 (S27E11 L= 23) 355 158 0 ( 650/ 711- 804/ 738) 26.6 E16-E06 S29-S24
20 1114 485 (S32W21 L= 55) 1765 388 4 ( 919/ 456-1279/ 533) 25.6 W07-W31 S37-S25
21 655 264 (S67E10 L= 25) 1441 178 3 ( 580/ 230- 747/ 302) 6.3 E23-W04 S70-S64
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Download FITS filament maps as tar archive
» All Filament Data of 20230515 ...
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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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