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| 20240818 - Filament data for 09 UTC |
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Available data for 20240818: »07 UTC »08 UTC »09 UTC »10 UTC »11 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 1736 1552 (N21W72 L=137) 694 54 1 (1712/1524-1756/1577) 12.5 W67-W78 N19-N21
2 1682 1395 (N14W54 L=119) 507 86 0 (1667/1353-1699/1446) 51.3 W51-W56 N11-N16
3 184 1325 (N37E73 L=353) 1198 85 3 ( 151/1288- 217/1361) -11.9 E86-E64 N34-N38
4 1472 1264 (N12W33 L= 98) 313 65 0 (1435/1243-1503/1286) -36.9 W30-W35 N10-N13
5 1815 1014 (S11W55 L=120) 512 80 1 (1798/ 977-1838/1054) -90.0 W53-W57 S13-S08
6 1614 975 (S08W36 L=102) 548 147 2 (1552/ 929-1652/1019) -54.5 W32-W39 S11-S04
7 1907 992 (S15W67 L=133) 630 40 3 (1882/ 969-1930/1015) 9.5 W62-W72 S16-S14
8 1038 883 (S02E02 L= 64) 270 127 0 ( 981/ 854-1081/ 925) -45.0 E04-W00 S04-N01
9 244 751 (N01E62 L= 4) 403 53 0 ( 225/ 721- 264/ 778) -33.7 E63-E59 N00-N02
10 215 692 (S02E68 L=357) 842 93 1 ( 193/ 655- 245/ 723) -38.7 E73-E64 S04-N00
11 1081 618 (S19E04 L= 61) 450 160 1 (1061/ 547-1106/ 684) 77.5 E05-E01 S23-S14
12 289 605 (S08E63 L= 3) 1145 175 3 ( 249/ 564- 319/ 678) 38.7 E68-E58 S11-S03
13 1725 639 (S33W45 L=110) 648 78 0 (1682/ 621-1762/ 657) -18.4 W40-W49 S34-S31
14 801 532 (S19E24 L= 42) 477 150 0 ( 778/ 464- 824/ 606) 52.1 E27-E20 S23-S14
15 463 531 (S15E49 L= 17) 706 174 1 ( 426/ 454- 493/ 599) 73.3 E52-E47 S19-S09
16 1351 546 (S29W12 L= 78) 569 92 0 (1326/ 498-1379/ 592) 56.3 W09-W14 S32-S26
17 367 502 (S16E60 L= 6) 573 111 0 ( 351/ 451- 389/ 545) 35.0 E65-E54 S19-S12
18 690 307 (S34E43 L= 23) 1113 215 1 ( 629/ 234- 742/ 399) 29.7 E55-E34 S39-S27
19 588 356 (S29E48 L= 18) 631 100 2 ( 537/ 329- 641/ 381) -5.7 E53-E42 S30-S26
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Download FITS filament maps as tar archive
» All Filament Data of 20240818 ...
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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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