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| 20240215 - Filament data for 13 UTC |
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Available data for 20240215: »10 UTC »11 UTC »12 UTC »13 UTC »14 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 503 1713 (N27E57 L=291) 2324 244 7 ( 439/1622- 568/1812) -74.1 E65-E52 N20-N36
2 445 1710 (N27E64 L=284) 706 93 0 ( 419/1671- 473/1752) -66.8 E66-E61 N23-N30
3 1336 1667 (N41W08 L=355) 1013 249 4 (1237/1611-1443/1706) -7.1 W00-W16 N38-N43
4 472 1559 (N16E49 L=299) 840 205 0 ( 417/1486- 536/1635) 80.5 E50-E47 N10-N22
5 580 1512 (N15E38 L=309) 278 75 1 ( 564/1482- 604/1543) 76.0 E39-E36 N12-N16
6 715 1365 (N08E25 L=322) 206 56 1 ( 693/1341- 736/1390) 76.0 E25-E23 N05-N09
7 1362 1297 (N16W15 L= 2) 396 93 0 (1313/1263-1403/1318) -9.5 W11-W17 N14-N16
8 1724 1268 (N23W42 L= 29) 282 54 0 (1701/1241-1745/1294) -45.0 W39-W44 N21-N24
9 1184 1254 (N09W05 L=352) 264 51 1 (1164/1226-1209/1282) -71.6 W03-W06 N07-N11
10 326 1112 (S13E48 L=300) 613 178 1 ( 264/1041- 387/1155) 41.6 E52-E42 S17-S09
11 1416 1117 (N06W21 L= 9) 208 49 1 (1392/1092-1431/1149) 90.0 W19-W22 N04-N08
12 1640 1075 (N09W37 L= 24) 412 106 0 (1626/1024-1672/1117) 80.5 W35-W38 N06-N12
13 497 998 (S17E33 L=315) 254 98 0 ( 486/ 943- 509/1043) 90.0 E33-E31 S20-S14
14 381 749 (S34E42 L=306) 853 242 1 ( 282/ 702- 463/ 825) 25.3 E53-E33 S38-S28
15 1769 722 (S07W58 L= 45) 399 56 1 (1751/ 690-1794/ 746) 90.0 W55-W60 S09-S05
16 1755 595 (S14W63 L= 51) 2137 252 11 (1663/ 543-1832/ 660) 28.1 W55-W73 S19-S09
17 1471 542 (S25W41 L= 29) 950 228 2 (1428/ 444-1519/ 654) -70.3 W38-W44 S31-S17
18 1777 535 (S16W71 L= 59) 828 71 2 (1756/ 502-1798/ 565) -76.0 W67-W75 S18-S14
19 1564 371 (S32W62 L= 49) 561 59 1 (1536/ 346-1599/ 389) 56.3 W57-W65 S33-S29
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Download FITS filament maps as tar archive
» All Filament Data of 20240215 ...
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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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