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| 20231016 - Filament data for 07 UTC |
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Available data for 20231016: »06 UTC »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC »13 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 905 1791 (N57W26 L=184) 361 47 0 ( 876/1776- 929/1809) -9.5 W21-W28 N55-N58
2 1277 1775 (N41W50 L=209) 746 127 1 (1216/1741-1339/1805) -7.6 W42-W58 N39-N42
3 1503 1593 (N23W51 L=209) 1022 138 1 (1433/1567-1575/1626) -12.1 W45-W59 N21-N25
4 701 1479 (N41E08 L=150) 241 71 0 ( 663/1470- 738/1490) -9.5 E10-E04 N40-N42
5 574 1437 (N42E19 L=139) 573 131 1 ( 515/1404- 627/1471) -41.6 E24-E15 N38-N46
6 1201 1398 (N21W21 L=179) 264 105 0 (1162/1378-1255/1428) -45.0 W19-W23 N18-N24
7 1018 1248 (N18W06 L=164) 854 331 1 ( 884/1201-1176/1291) -15.5 E03-W15 N14-N20
8 1525 1120 (S03W31 L=190) 284 48 0 (1500/1100-1560/1145) -45.0 W29-W33 S04-S01
9 1624 981 (S13W35 L=193) 800 248 1 (1588/ 869-1659/1088) 85.9 W32-W36 S20-S06
10 405 1022 (N21E39 L=119) 311 55 0 ( 374/ 998- 439/1047) -38.7 E41-E36 N18-N22
11 788 1020 (N12E13 L=145) 363 157 1 ( 697/ 997- 833/1043) -14.0 E18-E10 N09-N14
12 1251 992 (S02W12 L=170) 197 81 0 (1203/ 977-1276/1010) 0.0 W08-W13 S02-N00
13 807 968 (N08E14 L=145) 342 140 1 ( 762/ 939- 872/1003) 8.1 E16-E09 N07-N09
14 532 859 (N09E33 L=125) 228 64 0 ( 513/ 824- 551/ 895) -90.0 E34-E32 N06-N10
15 296 827 (N12E53 L=105) 368 111 0 ( 262/ 809- 341/ 851) -7.1 E56-E48 N10-N13
16 1575 718 (S28W26 L=184) 407 139 1 (1535/ 663-1619/ 783) 32.0 W21-W30 S30-S24
17 1219 579 (S25E01 L=157) 298 88 0 (1172/ 559-1263/ 606) -9.5 E04-W02 S25-S24
18 893 413 (S26E27 L=132) 1488 324 5 ( 861/ 297- 932/ 580) 50.2 E35-E20 S35-S15
19 674 324 (S27E47 L=111) 371 62 0 ( 658/ 291- 693/ 355) 23.2 E50-E43 S29-S24
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Download FITS filament maps as tar archive
» All Filament Data of 20231016 ...
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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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