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| 20230111 - Latest Filament data |
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Available data for 20230111: »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »13 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 597 1739 (N43E42 L=184) 365 30 0 ( 575/1717- 618/1762) 56.3 E43-E40 N40-N44
2 1460 1643 (N39W32 L=258) 2291 434 2 (1335/1531-1620/1716) -30.1 W21-W43 N31-N44
3 1229 1573 (N32W12 L=238) 275 77 1 (1194/1539-1262/1604) -38.7 W09-W14 N29-N33
4 346 1491 (N24E53 L=173) 975 165 4 ( 325/1414- 371/1566) -57.5 E59-E50 N18-N29
5 937 1531 (N27E08 L=218) 220 64 0 ( 903/1513- 972/1548) -21.8 E10-E05 N26-N28
6 1696 1422 (N24W48 L=274) 469 94 1 (1674/1383-1717/1473) -78.7 W44-W49 N22-N27
7 1550 1179 (N08W33 L=259) 330 96 1 (1534/1133-1566/1229) -78.7 W31-W33 N05-N10
8 425 1091 (S02E39 L=187) 235 69 2 ( 408/1054- 440/1126) -71.6 E40-E37 S03-N00
9 269 901 (S13E53 L=173) 753 189 3 ( 250/ 826- 292/ 985) 78.7 E55-E50 S17-S07
10 510 911 (S12E33 L=193) 365 125 0 ( 479/ 867- 547/ 966) 50.2 E35-E29 S14-S08
11 1088 806 (S17W05 L=231) 221 33 1 (1069/ 787-1111/ 825) -33.7 W03-W06 S18-S15
12 934 788 (S19E05 L=221) 248 123 2 ( 896/ 763- 986/ 824) 38.7 E07-E01 S20-S16
13 1731 755 (S16W51 L=278) 562 97 3 (1705/ 718-1761/ 796) 68.2 W49-W54 S18-S13
14 472 626 (S30E39 L=187) 955 157 3 ( 443/ 554- 511/ 708) -90.0 E41-E35 S34-S24
15 215 609 (S30E71 L=155) 1171 80 2 ( 188/ 570- 247/ 648) 12.5 E83-E64 S32-S28
16 1384 590 (S29W27 L=253) 546 132 1 (1336/ 559-1412/ 643) 59.0 W24-W29 S31-S25
17 1143 590 (S30W10 L=236) 575 221 1 (1038/ 572-1244/ 629) 12.1 W02-W16 S31-S27
18 879 496 (S38E08 L=218) 266 65 0 ( 844/ 473- 906/ 524) 31.0 E11-E06 S39-S35
19 616 302 (S54E40 L=186) 837 147 3 ( 551/ 256- 691/ 348) 15.1 E54-E28 S58-S50
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Download FITS filament maps as tar archive
» All Filament Data of 20230111 ...
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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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