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| 20231127 - Filament data for 09 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 1108 1871 (N56W38 L= 1) 765 78 3 (1077/1829-1142/1905) 28.3 W32-W45 N52-N59
2 1045 1842 (N56W28 L=351) 463 54 0 (1026/1814-1069/1872) 40.6 W25-W32 N52-N58
3 1480 1775 (N39W61 L= 24) 2676 306 4 (1342/1700-1600/1827) -33.7 W48-W73 N31-N45
4 889 1582 (N38W02 L=326) 930 267 1 ( 746/1556- 997/1603) -12.5 E08-W10 N35-N40
5 501 1356 (N31E30 L=294) 1836 496 3 ( 291/1254- 754/1401) -18.0 E51-E11 N24-N37
6 1201 1354 (N17W17 L=340) 711 233 5 (1136/1307-1280/1393) -18.4 W12-W22 N14-N20
7 1286 1301 (N13W21 L=344) 271 0 -1 (1223/1288-1328/1320) -8.1 W16-W23 N11-N13
8 272 1292 (N31E51 L=272) 383 78 1 ( 242/1253- 294/1316) -45.0 E55-E48 N27-N32
9 982 1269 (N16W02 L=325) 486 217 0 ( 882/1244-1079/1289) -15.3 E04-W07 N14-N19
10 165 1243 (N29E66 L=258) 576 90 0 ( 137/1213- 197/1287) -24.8 E73-E60 N26-N32
11 579 1228 (N21E24 L=299) 428 185 0 ( 494/1207- 671/1251) -22.6 E30-E18 N18-N23
12 627 1064 (N10E23 L=300) 358 118 1 ( 580/1018- 666/1109) -56.3 E25-E21 N07-N13
13 1808 977 (S16W53 L= 16) 495 115 0 (1782/ 932-1823/1041) 51.3 W50-W55 S18-S12
14 357 822 (N01E47 L=276) 352 94 0 ( 319/ 789- 393/ 865) 15.9 E50-E43 N00-N03
15 459 672 (S09E43 L=280) 319 50 1 ( 436/ 646- 491/ 696) 11.3 E44-E39 S10-S08
16 574 613 (S15E36 L=287) 289 107 0 ( 535/ 581- 621/ 654) -63.4 E38-E33 S17-S11
17 708 416 (S30E35 L=288) 668 203 1 ( 691/ 317- 739/ 493) 42.5 E41-E29 S36-S24
18 867 450 (S31E23 L=301) 243 84 0 ( 830/ 425- 904/ 476) 15.9 E26-E19 S31-S29
19 596 267 (S38E57 L=266) 570 75 0 ( 574/ 235- 617/ 303) 24.4 E63-E51 S40-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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