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| 20230111 - Filament data for 07 UTC |
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Available data for 20230111: »07 UTC »08 UTC »09 UTC »10 UTC »11 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 1401 1648 (N39W27 L=256) 1960 285 4 (1287/1579-1535/1703) -22.8 W17-W37 N34-N43
2 884 1533 (N27E12 L=217) 265 56 0 ( 851/1513- 919/1553) -14.0 E13-E09 N26-N28
3 307 1497 (N25E59 L=170) 1705 165 4 ( 260/1431- 360/1549) 40.6 E65-E53 N19-N28
4 1661 1419 (N24W44 L=273) 414 78 1 (1645/1383-1692/1460) -68.2 W42-W46 N21-N26
5 1491 1163 (N06W29 L=258) 284 44 2 (1463/1140-1510/1193) 45.0 W26-W30 N05-N08
6 229 969 (S09E57 L=172) 316 60 1 ( 212/ 942- 251/ 998) -36.9 E58-E54 S10-S06
7 478 934 (S11E35 L=194) 421 132 0 ( 433/ 883- 515/ 991) 45.0 E38-E32 S13-S07
8 337 878 (S14E47 L=182) 395 56 0 ( 310/ 854- 366/ 907) -36.9 E49-E44 S15-S12
9 270 844 (S16E54 L=175) 484 93 1 ( 244/ 794- 287/ 888) -90.0 E56-E51 S19-S13
10 903 788 (S19E07 L=222) 336 127 1 ( 858/ 758- 962/ 840) 39.8 E09-E03 S20-S15
11 1703 760 (S16W49 L=278) 430 96 1 (1683/ 722-1731/ 799) -59.0 W46-W51 S18-S13
12 448 622 (S30E42 L=187) 1186 198 5 ( 410/ 531- 497/ 711) -85.2 E44-E38 S36-S24
13 1716 637 (S24W55 L=284) 591 104 3 (1688/ 585-1747/ 676) 80.5 W51-W57 S26-S20
14 1348 598 (S29W25 L=254) 632 115 3 (1305/ 559-1378/ 652) 63.4 W21-W26 S31-S25
15 205 618 (S30E73 L=156) 799 49 1 ( 184/ 591- 223/ 650) 20.0 E81-E68 S31-S27
16 1105 594 (S30W07 L=236) 658 228 1 ( 999/ 574-1206/ 634) 13.0 W00-W14 S31-S27
17 642 538 (S36E27 L=202) 435 134 1 ( 580/ 522- 704/ 558) -5.7 E31-E21 S36-S34
18 847 504 (S38E11 L=218) 236 64 1 ( 819/ 474- 871/ 533) 53.1 E13-E09 S39-S35
19 573 287 (S56E49 L=180) 481 43 1 ( 548/ 268- 600/ 310) 9.5 E55-E43 S57-S53
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Download FITS filament maps as tar archive
» All Filament Data of 20230111 ...
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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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