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| 20230220 - Latest Filament data |
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Available data for 20230220: »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 1095 1780 (N43E16 L= 43) 461 66 1 (1072/1742-1114/1811) -66.8 E18-E13 N39-N46
2 1182 1622 (N33E04 L= 55) 474 124 1 (1133/1592-1238/1664) -14.0 E08-W00 N31-N35
3 1651 1522 (N40W35 L= 94) 1324 135 2 (1614/1462-1679/1583) 59.7 W30-W38 N33-N45
4 1381 1518 (N31W12 L= 71) 933 176 2 (1318/1452-1444/1577) -24.4 W06-W17 N27-N34
5 1600 1295 (N22W30 L= 90) 272 65 1 (1575/1262-1615/1329) 90.0 W28-W31 N19-N24
6 501 1296 (S01E38 L= 22) 286 57 0 ( 482/1267- 527/1320) 63.4 E38-E36 S02-N00
7 1701 1058 (N11W42 L=101) 1632 456 3 (1662/ 847-1736/1238) -72.3 W36-W46 S01-N21
8 664 1204 (S04E25 L= 35) 257 62 1 ( 627/1176- 691/1223) -14.0 E27-E22 S04-S02
9 1874 1063 (N16W59 L=118) 2741 325 11 (1817/ 908-1913/1187) -53.7 W51-W65 N07-N22
10 1823 1066 (N15W53 L=112) 339 37 0 (1804/1040-1843/1094) -33.7 W50-W55 N13-N16
11 283 975 (S23E51 L= 9) 332 61 0 ( 268/ 945- 299/1016) -76.0 E51-E48 S24-S20
12 400 652 (S42E40 L= 19) 386 90 1 ( 365/ 618- 445/ 680) 29.1 E44-E35 S44-S39
13 1729 649 (S11W57 L=117) 618 86 1 (1702/ 604-1756/ 677) 78.7 W53-W60 S13-S08
14 1218 613 (S26W22 L= 81) 302 90 0 (1176/ 579-1260/ 640) -8.1 W18-W25 S27-S25
15 1433 530 (S25W40 L= 99) 949 180 2 (1365/ 471-1495/ 587) -4.1 W33-W47 S27-S23
16 1361 393 (S35W43 L=102) 782 160 0 (1293/ 370-1433/ 434) 4.1 W35-W49 S36-S33
17 1278 327 (S42W42 L=101) 466 79 1 (1256/ 276-1298/ 365) -20.0 W37-W48 S44-S39
18 1552 302 (S34W70 L=129) 651 99 1 (1503/ 286-1601/ 319) 32.0 W64-W74 S36-S31
19 1362 240 (S45W59 L=118) 910 77 2 (1331/ 194-1388/ 278) -21.0 W54-W67 S47-S41
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Download FITS filament maps as tar archive
» All Filament Data of 20230220 ...
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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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