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| 20240519 - Latest Filament data |
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Available data for 20240519: »05 UTC »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
1 715 1792 (N40E51 L=137) 1727 185 4 ( 652/1726- 788/1854) -12.7 E69-E38 N36-N43
2 775 1627 (N29E33 L=155) 1031 214 2 ( 662/1583- 856/1670) 48.0 E39-E28 N23-N33
3 1604 1515 (N43W33 L=221) 1986 270 3 (1530/1399-1654/1603) -60.3 W26-W39 N34-N48
4 444 1475 (N12E50 L=137) 719 114 0 ( 415/1424- 483/1522) 81.9 E51-E48 N08-N15
5 1167 1395 (N23W00 L=188) 1011 328 4 (1041/1308-1242/1505) -23.6 E10-W06 N18-N27
6 1452 1460 (N35W19 L=206) 423 161 1 (1389/1415-1521/1487) -4.8 W13-W25 N33-N35
7 1586 1269 (N25W32 L=219) 2212 516 4 (1511/1024-1675/1458) -54.7 W23-W41 N12-N36
8 1062 1295 (N14E04 L=184) 355 130 1 (1013/1258-1118/1334) -8.1 E07-W00 N12-N15
9 1850 1173 (N26W60 L=247) 1335 128 2 (1819/1112-1872/1232) -76.0 W55-W62 N22-N30
10 328 1070 (S14E48 L=140) 1429 315 5 ( 248/ 994- 402/1131) 23.2 E55-E41 S18-S09
11 213 925 (S25E59 L=128) 580 82 0 ( 194/ 876- 228/ 971) 74.1 E62-E56 S28-S21
12 1636 925 (N06W41 L=228) 291 43 1 (1615/ 904-1666/ 944) 11.3 W38-W43 N04-N06
13 551 887 (S20E27 L=161) 411 120 2 ( 508/ 853- 589/ 939) 60.3 E29-E24 S23-S16
14 1486 709 (S10W36 L=224) 317 55 0 (1463/ 684-1508/ 734) -14.0 W34-W38 S11-S08
15 1462 644 (S14W37 L=224) 444 116 1 (1435/ 606-1492/ 691) -23.2 W33-W40 S16-S11
16 1363 615 (S18W31 L=219) 509 131 0 (1297/ 596-1404/ 655) 45.0 W27-W34 S20-S15
17 391 602 (S43E41 L=146) 1341 175 3 ( 306/ 572- 460/ 630) 9.0 E53-E33 S45-S39
18 1542 497 (S21W50 L=238) 393 106 0 (1493/ 468-1587/ 519) 39.8 W47-W53 S24-S18
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Download FITS filament maps as tar archive
» All Filament Data of 20240519 ...
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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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