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| 20231127 - Filament data for 10 UTC |
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Available data for 20231127: »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 1115 1868 (N56W38 L= 1) 1000 108 3 (1082/1829-1155/1899) -80.5 W32-W46 N52-N59
2 1031 1828 (N55W26 L=349) 870 111 2 ( 977/1784-1077/1874) 18.4 W18-W33 N51-N58
3 1484 1774 (N38W61 L= 24) 2884 296 5 (1341/1701-1603/1827) -32.3 W49-W73 N31-N45
4 888 1582 (N38W02 L=325) 1028 268 2 ( 747/1556- 998/1603) -12.5 E08-W10 N35-N41
5 1237 1581 (N31W26 L=349) 228 66 0 (1203/1567-1269/1596) -26.6 W24-W28 N29-N32
6 506 1360 (N31E29 L=294) 1798 497 4 ( 294/1297- 756/1401) -16.7 E50-E10 N24-N37
7 1199 1353 (N17W17 L=340) 731 230 2 (1137/1308-1277/1395) -14.0 W12-W21 N14-N20
8 281 1243 (N27E50 L=273) 852 189 3 ( 241/1147- 314/1323) -58.4 E55-E45 N20-N33
9 983 1270 (N16W02 L=325) 527 225 0 ( 882/1244-1085/1291) -15.3 E03-W08 N13-N19
10 165 1244 (N29E66 L=257) 636 81 0 ( 137/1212- 197/1287) -24.8 E73-E60 N26-N32
11 585 1229 (N21E24 L=299) 434 179 0 ( 500/1208- 670/1252) -24.4 E29-E18 N18-N23
12 628 1065 (N10E23 L=300) 387 122 2 ( 581/1019- 668/1111) -56.3 E25-E20 N07-N13
13 1811 974 (S16W53 L= 16) 606 137 1 (1785/ 913-1825/1046) 63.4 W50-W55 S19-S11
14 359 823 (N01E47 L=276) 380 112 0 ( 318/ 784- 398/ 867) 14.0 E51-E42 N00-N02
15 461 673 (S09E43 L=280) 354 51 1 ( 435/ 645- 494/ 696) 21.8 E44-E39 S10-S08
16 586 609 (S15E36 L=287) 394 150 0 ( 534/ 576- 653/ 656) -54.5 E38-E31 S18-S11
17 710 415 (S30E35 L=288) 736 199 0 ( 693/ 320- 741/ 494) 53.1 E40-E29 S36-S24
18 868 449 (S31E22 L=301) 287 108 0 ( 830/ 410- 913/ 480) 20.6 E26-E18 S32-S29
19 594 270 (S38E57 L=266) 651 61 2 ( 563/ 242- 622/ 303) 14.0 E63-E51 S39-S35
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Download FITS filament maps as tar archive
» All Filament Data of 20231127 ...
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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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