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| 20230711 - Filament data for 07 UTC |
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Available data for 20230711: »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
1 845 1828 (N64E24 L=336) 406 74 0 ( 814/1806- 879/1843) 29.7 E26-E19 N61-N65
2 956 1818 (N63E07 L=353) 425 49 1 ( 939/1792- 978/1839) 51.3 E09-E04 N59-N65
3 338 1441 (N30E57 L=303) 638 139 1 ( 294/1404- 378/1469) 12.5 E62-E52 N27-N31
4 1696 1380 (N24W53 L= 53) 1053 202 3 (1613/1312-1773/1436) -33.7 W46-W59 N19-N27
5 1324 1371 (N25W21 L= 21) 412 191 0 (1248/1314-1385/1404) -36.9 W16-W25 N21-N27
6 290 1328 (N22E58 L=302) 497 87 1 ( 268/1296- 328/1370) -26.6 E61-E52 N20-N24
7 1532 1339 (N22W37 L= 36) 295 74 0 (1499/1313-1552/1368) 31.0 W33-W38 N20-N24
8 764 1287 (N20E17 L=343) 429 167 1 ( 698/1256- 814/1346) 32.0 E21-E13 N18-N24
9 355 1105 (N08E47 L=313) 362 61 1 ( 334/1076- 379/1138) -45.0 E48-E44 N06-N10
10 1749 864 (S08W52 L= 51) 518 52 0 (1722/ 838-1773/ 888) 26.6 W49-W54 S09-S06
11 1799 788 (S14W59 L= 58) 2260 306 8 (1722/ 711-1860/ 888) 84.8 W50-W68 S18-S07
12 1649 718 (S17W44 L= 44) 617 187 2 (1607/ 658-1687/ 774) 54.5 W41-W46 S21-S13
13 1421 697 (S18W26 L= 26) 631 149 3 (1354/ 665-1495/ 740) 21.8 W21-W31 S19-S14
14 280 688 (S18E58 L=301) 408 15 0 ( 263/ 667- 296/ 709) 45.0 E60-E56 S19-S16
15 481 660 (S19E39 L=321) 335 79 0 ( 460/ 632- 497/ 701) 51.3 E41-E37 S21-S16
16 1743 652 (S22W56 L= 56) 531 78 1 (1704/ 623-1771/ 678) 18.4 W51-W59 S24-S20
17 1783 611 (S26W64 L= 64) 1468 138 3 (1722/ 582-1846/ 642) 0.0 W55-W76 S27-S23
18 836 457 (S34E15 L=345) 2625 351 10 ( 740/ 383- 953/ 583) -28.1 E21-E06 S39-S24
19 582 310 (S47E46 L=314) 550 92 0 ( 572/ 266- 594/ 358) 34.7 E53-E40 S51-S42
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Download FITS filament maps as tar archive
» All Filament Data of 20230711 ...
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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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