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| 20250320 - Filament data for 10 UTC |
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Available data for 20250320: »06 UTC »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC »13 UTC »14 UTC »15 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 1035 1755 (N37E23 L=100) 1132 189 2 ( 973/1693-1120/1790) 70.0 E26-E19 N30-N41
2 1150 1567 (N28E08 L=116) 233 98 0 (1137/1520-1169/1615) -81.9 E09-E06 N24-N31
3 1498 1497 (N34W16 L=140) 512 81 0 (1471/1459-1524/1537) -45.0 W13-W18 N31-N36
4 1680 1302 (N28W34 L=158) 593 132 0 (1644/1247-1712/1359) -35.5 W30-W37 N25-N30
5 960 1326 (N08E11 L=112) 587 181 2 ( 866/1296-1045/1350) 26.6 E16-E06 N05-N10
6 489 1221 (S09E37 L= 87) 407 130 0 ( 452/1168- 514/1283) 90.0 E38-E35 S12-S05
7 376 1178 (S13E44 L= 79) 272 52 0 ( 362/1143- 389/1208) -63.4 E45-E42 S15-S11
8 905 1099 (S06E08 L=115) 603 137 2 ( 860/1039- 944/1158) -35.5 E11-E04 S08-S03
9 639 1105 (S12E24 L=100) 410 84 1 ( 608/1071- 675/1140) 59.0 E25-E22 S14-S09
10 818 1052 (S11E12 L=112) 228 36 0 ( 791/1030- 841/1073) 56.3 E13-E10 S12-S09
11 885 989 (S12E07 L=117) 187 71 2 ( 855/ 968- 917/1025) 90.0 E08-E04 S14-S10
12 1816 952 (N12W53 L=176) 601 128 1 (1769/ 918-1867/ 978) 36.9 W49-W58 N08-N14
13 954 899 (S16E01 L=123) 444 153 2 ( 896/ 866-1031/ 937) 45.0 E03-W03 S18-S12
14 1810 821 (N05W57 L=180) 1118 185 3 (1767/ 751-1853/ 896) -15.9 W49-W63 N01-N08
15 1654 600 (S11W53 L=177) 507 100 2 (1625/ 550-1688/ 643) 90.0 W50-W54 S14-S07
16 1122 559 (S30W20 L=144) 230 47 1 (1087/ 541-1143/ 579) 14.0 W17-W21 S30-S28
17 1654 480 (S17W61 L=185) 1263 163 3 (1561/ 448-1720/ 506) 28.3 W54-W68 S21-S13
18 1415 377 (S30W50 L=173) 587 56 1 (1380/ 349-1450/ 408) 53.1 W47-W52 S32-S28
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Download FITS filament maps as tar archive
» All Filament Data of 20250320 ...
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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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