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| 20240517 - Filament data for 05 UTC |
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Available data for 20240517: »05 UTC »06 UTC »07 UTC »09 UTC »10 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 1245 1611 (N40E00 L=218) 1103 209 2 (1187/1527-1288/1682) -39.3 E07-W04 N34-N44
2 683 1485 (N17E33 L=185) 1174 469 3 ( 543/1367- 837/1635) -17.4 E51-E19 N12-N24
3 1159 1464 (N27E02 L=216) 868 402 0 (1058/1294-1212/1603) -43.3 E13-W05 N17-N34
4 732 1558 (N23E33 L=185) 277 88 0 ( 704/1525- 760/1599) -29.7 E36-E29 N21-N25
5 1072 1368 (N19E05 L=213) 298 124 0 (1049/1313-1089/1424) -82.9 E06-E03 N14-N22
6 1523 1282 (N25W26 L=244) 661 222 1 (1495/1199-1581/1335) -63.4 W23-W30 N19-N28
7 147 1164 (S12E73 L=145) 2471 228 7 ( 117/1078- 175/1268) -50.7 E81-E65 S16-S05
8 214 1166 (S11E62 L=156) 1900 191 5 ( 165/1108- 265/1216) -12.1 E69-E55 S13-S07
9 1774 1065 (N18W50 L=268) 805 165 0 (1756/ 989-1791/1142) -77.5 W47-W52 N12-N22
10 220 1012 (S20E58 L=160) 1050 143 1 ( 180/ 948- 246/1079) 56.3 E63-E55 S24-S15
11 747 969 (S12E15 L=203) 420 136 2 ( 699/ 939- 790/1007) -9.5 E18-E12 S13-S09
12 1161 925 (S05W10 L=228) 407 181 0 (1086/ 866-1208/ 971) -18.4 W05-W14 S07-S03
13 895 768 (S20E02 L=216) 559 237 1 ( 785/ 734- 991/ 793) 28.6 E08-W03 S24-S16
14 313 706 (S38E48 L=170) 3138 351 7 ( 164/ 665- 452/ 759) 6.3 E87-E33 S43-S32
15 1778 561 (S11W72 L=290) 631 44 0 (1742/ 544-1805/ 577) 11.3 W66-W77 S12-S09
16 681 406 (S51E10 L=208) 580 120 0 ( 632/ 383- 739/ 438) 0.0 E15-E03 S52-S49
17 1618 403 (S24W66 L=284) 581 63 0 (1597/ 384-1648/ 434) -10.3 W60-W71 S25-S22
18 1565 369 (S28W64 L=282) 516 45 1 (1542/ 349-1592/ 389) -7.1 W59-W67 S28-S26
19 1491 338 (S32W59 L=277) 677 45 1 (1470/ 311-1518/ 370) -20.6 W54-W63 S33-S30
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Download FITS filament maps as tar archive
» All Filament Data of 20240517 ...
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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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