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| 20240420 - Filament data for 08 UTC |
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Available data for 20240420: »06 UTC »08 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
1 809 1768 (N34E42 L=172) 374 50 1 ( 793/1746- 830/1797) -18.4 E45-E39 N32-N35
2 572 1677 (N21E53 L=161) 490 107 1 ( 555/1633- 599/1720) -45.0 E56-E47 N18-N24
3 723 1650 (N23E39 L=174) 357 167 0 ( 674/1589- 756/1678) -24.0 E43-E34 N19-N25
4 661 1521 (N13E37 L=177) 239 124 0 ( 635/1475- 693/1554) -23.2 E39-E32 N11-N15
5 957 1482 (N19E17 L=196) 414 158 0 ( 910/1419- 990/1546) -29.1 E22-E13 N15-N21
6 1480 1439 (N33W17 L=230) 506 177 0 (1446/1353-1499/1501) -60.9 W12-W18 N26-N36
7 384 1353 (S03E50 L=163) 1631 262 4 ( 313/1259- 438/1457) 77.0 E53-E46 S09-N04
8 1683 1389 (N37W35 L=248) 324 44 0 (1662/1358-1698/1412) -76.0 W32-W36 N34-N38
9 256 1349 (S05E63 L=151) 798 147 2 ( 242/1266- 277/1407) -56.3 E67-E58 S10-S01
10 1262 1272 (N15W07 L=220) 240 80 0 (1226/1242-1300/1292) 0.0 W04-W09 N14-N16
11 1750 1121 (N22W44 L=258) 371 87 0 (1727/1076-1767/1151) -45.0 W41-W46 N19-N23
12 387 993 (S23E40 L=173) 664 171 2 ( 319/ 933- 436/1062) 48.4 E45-E37 S27-S18
13 953 904 (S14E01 L=213) 598 204 3 ( 890/ 870-1030/ 945) -7.1 E04-W04 S15-S11
14 1081 867 (S12W08 L=221) 493 155 1 (1049/ 803-1112/ 924) -60.3 W05-W10 S15-S08
15 1167 859 (S10W12 L=226) 347 97 1 (1119/ 834-1216/ 890) 45.0 W09-W14 S12-S07
16 953 861 (S16W01 L=214) 195 77 1 ( 917/ 846- 989/ 878) 26.6 E01-W03 S17-S14
17 730 732 (S30E09 L=204) 771 224 1 ( 644/ 703- 827/ 781) 13.0 E16-E03 S31-S26
18 636 440 (S53E09 L=204) 546 133 0 ( 587/ 413- 701/ 474) 4.8 E14-E02 S54-S50
19 1280 278 (S40W51 L=264) 384 66 2 (1260/ 242-1296/ 313) -26.6 W47-W55 S41-S37
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Download FITS filament maps as tar archive
» All Filament Data of 20240420 ...
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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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