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| 20240330 - Filament data for 07 UTC |
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Available data for 20240330: »07 UTC »08 UTC »09 UTC »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
1 511 1751 (N24E65 L= 66) 774 63 2 ( 481/1729- 541/1776) 63.4 E70-E60 N21-N26
2 827 1612 (N22E30 L=101) 1129 227 2 ( 793/1513- 871/1711) -55.3 E34-E24 N15-N28
3 1448 1629 (N44W09 L=140) 851 118 1 (1386/1599-1512/1652) 10.3 W03-W14 N41-N46
4 1273 1540 (N31E01 L=130) 456 70 1 (1241/1511-1312/1566) 0.0 E03-W02 N28-N32
5 1327 1321 (N19W09 L=140) 883 348 2 (1225/1271-1467/1401) 14.0 W01-W17 N15-N23
6 1815 1316 (N37W49 L=180) 776 80 1 (1790/1275-1839/1351) -26.6 W45-W52 N34-N38
7 1773 1170 (N25W45 L=176) 321 79 0 (1730/1141-1806/1188) 40.6 W40-W48 N21-N27
8 1639 1046 (N13W36 L=167) 823 225 0 (1554/ 995-1709/1136) -11.3 W27-W42 N11-N15
9 201 1051 (S25E61 L= 70) 399 85 0 ( 181/1006- 212/1089) -51.3 E63-E58 S27-S22
10 1775 1039 (N17W47 L=178) 437 78 0 (1739/1017-1801/1069) 38.7 W44-W49 N15-N19
11 785 805 (S25E08 L=123) 1321 211 5 ( 699/ 747- 878/ 867) 54.0 E12-E02 S30-S19
12 1873 828 (N10W66 L=197) 466 107 0 (1827/ 813-1908/ 862) 31.0 W59-W70 N07-N13
13 1693 640 (S06W55 L=186) 435 70 1 (1655/ 627-1731/ 653) 33.7 W52-W58 S08-S04
14 741 615 (S38E05 L=126) 554 132 1 ( 698/ 590- 813/ 647) 26.6 E08-W00 S39-S35
15 567 565 (S47E18 L=113) 1452 225 6 ( 507/ 514- 644/ 638) -8.1 E24-E10 S50-S41
16 1487 539 (S19W45 L=176) 639 114 2 (1452/ 508-1544/ 582) 6.3 W40-W49 S20-S16
17 847 518 (S41W06 L=137) 772 210 1 ( 749/ 480- 933/ 576) 50.7 W00-W09 S46-S34
18 1712 460 (S14W72 L=202) 3619 196 5 (1653/ 386-1781/ 522) 70.0 W63-W83 S19-S08
19 1581 438 (S20W59 L=190) 432 87 1 (1540/ 406-1614/ 472) 90.0 W57-W60 S23-S17
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Download FITS filament maps as tar archive
» All Filament Data of 20240330 ...
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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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