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| 20230727 - Filament data for 08 UTC |
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Available data for 20230727: »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
1 929 1869 (N71W05 L=152) 578 56 1 ( 913/1841- 954/1897) 45.0 W01-W09 N67-N76
2 1581 1561 (N33W53 L=201) 463 89 0 (1538/1543-1623/1576) -6.3 W48-W57 N31-N33
3 1119 1531 (N37W13 L=160) 375 95 0 (1071/1502-1158/1558) 20.6 W08-W16 N35-N38
4 1191 1518 (N35W18 L=166) 349 69 1 (1174/1484-1208/1553) 68.2 W16-W19 N32-N37
5 1550 1475 (N28W45 L=193) 799 178 0 (1512/1386-1582/1543) 74.7 W43-W46 N21-N32
6 1697 1474 (N25W60 L=207) 750 126 2 (1658/1420-1726/1525) 21.0 W52-W65 N22-N27
7 794 1361 (N28E13 L=135) 577 190 3 ( 760/1281- 847/1435) -74.7 E15-E09 N22-N33
8 393 1280 (N25E45 L=103) 2669 445 6 ( 278/1156- 563/1337) 6.6 E55-E29 N17-N29
9 1258 1263 (N18W17 L=165) 411 125 1 (1220/1223-1306/1305) -26.6 W14-W20 N15-N20
10 145 1198 (N20E76 L= 72) 824 107 2 ( 129/1154- 166/1252) 90.0 E79-E72 N17-N23
11 388 1069 (N12E43 L=104) 641 112 1 ( 346/1025- 431/1109) -32.0 E47-E39 N09-N14
12 493 1003 (N08E35 L=113) 312 57 1 ( 472/ 975- 527/1030) 14.0 E36-E32 N06-N09
13 1747 857 (S13W50 L=197) 531 46 0 (1720/ 829-1770/ 884) 90.0 W47-W52 S14-S11
14 676 795 (S06E24 L=124) 306 118 0 ( 622/ 756- 714/ 814) -26.6 E27-E21 S08-S04
15 246 732 (S09E62 L= 86) 744 82 1 ( 230/ 690- 274/ 776) 50.2 E64-E58 S11-S05
16 427 422 (S31E58 L= 90) 501 77 0 ( 412/ 383- 447/ 466) 50.2 E60-E54 S33-S27
17 847 400 (S35E20 L=128) 405 110 1 ( 791/ 386- 902/ 415) -14.0 E24-E15 S35-S32
18 1241 249 (S54W11 L=159) 453 50 0 (1216/ 233-1271/ 270) -26.6 W08-W14 S56-S51
19 951 185 (S57E22 L=126) 451 66 0 ( 914/ 172- 983/ 199) -7.1 E25-E17 S59-S55
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Download FITS filament maps as tar archive
» All Filament Data of 20230727 ...
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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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