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| 20221030 - Filament data for 07 UTC |
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Available data for 20221030: »06 UTC »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 1160 1683 (N39W32 L=143) 439 72 0 (1122/1661-1188/1707) 0.0 W28-W34 N37-N40
2 1274 1641 (N33W37 L=148) 616 119 0 (1225/1592-1311/1671) -71.6 W33-W38 N28-N35
3 810 1624 (N46W04 L=115) 286 62 0 ( 776/1611- 846/1638) -18.4 W01-W07 N45-N47
4 1472 1556 (N22W45 L=156) 437 130 1 (1447/1502-1516/1596) 15.3 W40-W51 N19-N23
5 1327 1563 (N27W36 L=147) 311 71 1 (1294/1541-1348/1593) 9.5 W32-W38 N24-N28
6 426 1282 (N34E34 L= 77) 482 142 1 ( 381/1224- 480/1339) -48.4 E38-E29 N29-N38
7 771 1272 (N25E09 L=102) 326 109 1 ( 748/1225- 800/1323) -81.9 E10-E07 N21-N28
8 416 1154 (N26E36 L= 75) 286 101 3 ( 379/1124- 462/1181) 0.0 E39-E31 N24-N28
9 239 1069 (N25E54 L= 57) 679 133 1 ( 203/1044- 292/1111) -11.3 E58-E48 N23-N27
10 1913 1014 (S21W66 L=177) 631 93 0 (1900/ 968-1925/1058) -80.5 W63-W68 S24-S18
11 135 1000 (N23E70 L= 41) 962 98 3 ( 106/ 961- 164/1044) -45.0 E75-E64 N20-N25
12 935 771 (S07E11 L=100) 611 174 1 ( 896/ 684- 986/ 840) 41.2 E15-E06 S11-S04
13 1709 630 (S39W39 L=150) 1460 314 5 (1575/ 565-1829/ 718) 0.0 W25-W53 S40-S36
14 1097 506 (S27E10 L=101) 284 65 0 (1063/ 482-1127/ 527) 11.3 E12-E07 S28-S26
15 976 459 (S27E19 L= 92) 430 113 1 ( 926/ 439-1033/ 483) -33.7 E21-E15 S29-S24
16 760 404 (S25E35 L= 76) 725 180 1 ( 671/ 379- 845/ 430) -13.0 E41-E28 S26-S23
17 828 331 (S32E35 L= 76) 383 123 0 ( 785/ 301- 868/ 382) 16.7 E39-E29 S33-S29
18 1129 191 (S54E26 L= 86) 392 26 0 (1111/ 169-1147/ 209) 23.2 E29-E22 S55-S51
19 1039 124 (S58E44 L= 67) 638 52 1 (1016/ 104-1057/ 148) 14.0 E50-E37 S60-S54
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Download FITS filament maps as tar archive
» All Filament Data of 20221030 ...
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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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