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| 20240527 - Filament data for 06 UTC |
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Available data for 20240527: »05 UTC »06 UTC »07 UTC »08 UTC »09 UTC »12 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 902 1709 (N40E27 L= 58) 283 38 0 ( 882/1693- 922/1728) 71.6 E29-E25 N38-N42
2 1245 1612 (N41W03 L= 88) 454 91 0 (1202/1594-1298/1628) 26.6 W00-W06 N38-N42
3 500 1556 (N21E49 L= 36) 1838 318 5 ( 376/1509- 614/1603) 26.6 E59-E41 N16-N25
4 960 1542 (N29E16 L= 70) 349 138 0 ( 907/1514-1021/1587) -16.7 E20-E10 N28-N31
5 1606 1367 (N32W34 L=120) 323 36 1 (1583/1346-1625/1387) 45.0 W32-W36 N30-N33
6 1336 1268 (N19W15 L=100) 350 90 2 (1297/1246-1375/1292) -9.5 W11-W17 N17-N20
7 1389 1163 (N14W20 L=105) 206 63 0 (1362/1138-1416/1178) 0.0 W17-W21 N12-N15
8 192 989 (S19E62 L= 23) 2729 342 5 ( 116/ 860- 259/1137) 36.2 E82-E55 S27-S08
9 1781 1041 (N15W53 L=138) 445 77 0 (1760/1010-1800/1079) 68.2 W50-W54 N12-N17
10 1053 1014 (S01W02 L= 87) 677 181 3 ( 961/ 987-1128/1041) 24.0 E03-W06 S04-N00
11 789 830 (S17E11 L= 75) 609 258 0 ( 667/ 796- 903/ 855) 25.0 E18-E03 S21-S13
12 1399 688 (S14W30 L=116) 1045 287 1 (1282/ 598-1500/ 763) 54.5 W25-W35 S21-S07
13 415 676 (S35E38 L= 47) 1011 236 1 ( 346/ 598- 511/ 742) 35.8 E47-E29 S41-S28
14 1750 650 (S09W61 L=146) 1791 195 3 (1710/ 570-1786/ 737) -79.7 W57-W64 S14-S03
15 1680 614 (S13W55 L=141) 859 114 2 (1649/ 555-1715/ 659) -60.3 W52-W58 S16-S09
16 329 572 (S44E52 L= 33) 417 41 0 ( 309/ 553- 352/ 592) -14.0 E55-E48 S46-S42
17 1471 501 (S24W43 L=128) 818 231 1 (1400/ 465-1528/ 573) 53.1 W37-W46 S26-S18
18 1184 525 (S28W22 L=107) 264 31 0 (1158/ 512-1215/ 539) 14.0 W19-W23 S29-S27
19 960 474 (S37W08 L= 93) 315 82 0 ( 921/ 458-1002/ 496) 38.7 W05-W10 S38-S34
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Download FITS filament maps as tar archive
» All Filament Data of 20240527 ...
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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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