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| 20250702 - Latest Filament data |
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Available data for 20250702: »05 UTC »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 1603 1684 (N48W61 L=248) 601 37 0 (1581/1655-1626/1706) 15.9 W54-W68 N45-N49
2 1231 1547 (N37W14 L=202) 399 76 0 (1199/1521-1269/1572) 9.5 W11-W17 N35-N39
3 1294 1482 (N33W19 L=206) 468 110 1 (1257/1448-1344/1519) -15.9 W15-W22 N30-N35
4 460 1476 (N29E45 L=142) 655 112 0 ( 431/1427- 506/1507) 68.2 E48-E41 N26-N31
5 565 1457 (N29E35 L=152) 445 102 1 ( 521/1439- 623/1479) -6.3 E39-E30 N27-N30
6 1307 1327 (N22W18 L=205) 332 73 0 (1291/1287-1327/1369) 80.5 W16-W19 N19-N25
7 318 1153 (N08E50 L=138) 657 143 1 ( 295/1095- 347/1225) -53.1 E53-E46 N04-N12
8 1674 1147 (N11W44 L=232) 507 98 0 (1629/1110-1709/1182) -39.8 W40-W47 N08-N13
9 1796 1137 (N10W56 L=243) 346 69 0 (1782/1096-1812/1166) -90.0 W54-W58 N07-N12
10 1728 987 (N01W48 L=236) 1080 210 1 (1696/ 906-1755/1076) -83.7 W45-W51 S03-N06
11 359 816 (S12E46 L=142) 274 72 1 ( 337/ 793- 374/ 843) 56.3 E47-E44 S13-S10
12 1618 757 (S13W41 L=228) 388 42 1 (1592/ 736-1644/ 779) 26.6 W39-W43 S14-S11
13 288 693 (S21E55 L=132) 678 114 1 ( 235/ 664- 333/ 735) 19.7 E63-E49 S22-S17
14 903 582 (S25E07 L=180) 970 104 1 ( 839/ 544- 985/ 639) -21.8 E11-E01 S27-S21
15 1771 574 (S25W64 L=251) 2286 171 2 (1697/ 517-1826/ 635) 48.8 W56-W72 S29-S21
16 709 585 (S26E21 L=167) 443 134 1 ( 644/ 559- 756/ 621) 26.6 E25-E17 S27-S23
17 1378 233 (S54W43 L=231) 652 92 1 (1349/ 216-1411/ 259) 53.1 W36-W49 S55-S50
18 1298 213 (S56W35 L=222) 818 77 3 (1272/ 185-1329/ 244) -26.6 W29-W41 S59-S52
19 1228 207 (S57W27 L=214) 1012 106 3 (1172/ 185-1269/ 243) 35.5 W19-W32 S59-S52
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Download FITS filament maps as tar archive
» All Filament Data of 20250702 ...
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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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