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| 20241014 - Filament data for 08 UTC |
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Available data for 20241014: »06 UTC »07 UTC »08 UTC »09 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 1560 1616 (N21W56 L= 90) 3003 385 4 (1365/1529-1710/1673) -46.5 W44-W64 N11-N30
2 1741 1600 (N14W75 L=108) 1962 136 5 (1686/1548-1776/1652) -90.0 W67-W83 N10-N18
3 1804 1205 (S07W55 L= 89) 1551 247 4 (1772/1097-1848/1307) 42.3 W49-W61 S12-S02
4 219 1130 (N31E56 L=338) 818 132 1 ( 189/1065- 253/1183) -52.1 E60-E51 N26-N35
5 1879 1091 (S16W60 L= 94) 924 165 3 (1838/1059-1913/1129) -36.9 W55-W65 S19-S13
6 552 970 (N15E29 L= 5) 306 102 1 ( 519/ 931- 577/1014) -68.2 E30-E27 N12-N17
7 1304 929 (S07W13 L= 46) 310 119 0 (1262/ 880-1326/ 976) 38.7 W09-W14 S08-S04
8 519 916 (N12E32 L= 1) 355 113 1 ( 479/ 869- 544/ 953) 78.7 E34-E30 N09-N14
9 1506 853 (S17W23 L= 56) 275 122 0 (1472/ 810-1529/ 912) 33.7 W19-W25 S18-S14
10 1613 839 (S21W30 L= 64) 231 51 1 (1597/ 820-1642/ 862) 0.0 W28-W32 S22-S19
11 452 799 (N07E40 L=353) 378 137 0 ( 401/ 755- 498/ 851) 16.7 E45-E35 N05-N09
12 1661 777 (S27W33 L= 66) 574 178 1 (1597/ 728-1716/ 844) 15.3 W26-W38 S27-S23
13 1218 807 (S11W05 L= 38) 247 126 0 (1159/ 763-1261/ 831) -56.3 W02-W06 S14-S08
14 1109 703 (S14E04 L= 30) 422 172 1 (1040/ 669-1143/ 770) 14.0 E08-W00 S16-S10
15 603 531 (S11E39 L=354) 2609 601 7 ( 469/ 332- 709/ 742) 29.1 E61-E25 S21-S01
16 1292 689 (S20W06 L= 39) 352 49 1 (1270/ 659-1322/ 727) 76.0 W04-W07 S21-S17
17 377 441 (S12E63 L=330) 1943 177 3 ( 340/ 377- 428/ 539) 61.4 E72-E58 S16-S05
18 1261 422 (S36E04 L= 30) 643 160 0 (1212/ 380-1298/ 493) 40.6 E07-W00 S39-S31
19 1130 235 (S47E22 L= 11) 1125 167 2 (1076/ 177-1175/ 281) 18.4 E31-E16 S50-S41
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Download FITS filament maps as tar archive
» All Filament Data of 20241014 ...
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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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