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| 20230215 - Filament data for 11 UTC |
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Available data for 20230215: »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC »13 UTC »14 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 807 1735 (N34E33 L= 94) 982 142 1 ( 777/1663- 834/1801) -39.8 E39-E27 N28-N38
2 500 1744 (N30E61 L= 65) 1064 114 2 ( 465/1692- 539/1787) -17.7 E73-E51 N26-N33
3 676 1606 (N22E35 L= 91) 447 130 1 ( 620/1558- 734/1644) 56.3 E37-E32 N18-N25
4 1227 1617 (N34W01 L=127) 317 80 0 (1200/1595-1260/1643) -26.6 E01-W03 N32-N35
5 391 1572 (N16E57 L= 69) 491 112 1 ( 366/1547- 429/1612) -7.1 E60-E52 N14-N19
6 993 1472 (N19E11 L=115) 1613 482 5 ( 839/1377-1144/1605) -14.6 E23-W00 N14-N25
7 708 1377 (N08E26 L=101) 1328 383 1 ( 676/1221- 734/1582) -67.8 E31-E21 S01-N21
8 1514 1438 (N29W24 L=150) 800 253 0 (1468/1378-1604/1494) 35.0 W20-W30 N23-N32
9 1635 1377 (N28W34 L=160) 410 131 0 (1608/1315-1660/1432) -56.3 W31-W36 N24-N30
10 1015 914 (S13W02 L=128) 684 202 2 ( 937/ 886-1120/ 948) 29.1 E02-W07 S16-S10
11 871 851 (S20E06 L=120) 236 30 2 ( 848/ 824- 895/ 877) -71.6 E07-E04 S21-S18
12 592 832 (S26E24 L=102) 364 126 0 ( 531/ 806- 636/ 854) 0.0 E28-E20 S26-S24
13 555 694 (S35E26 L=100) 361 80 0 ( 525/ 674- 597/ 722) -9.5 E28-E22 S36-S33
14 1412 499 (S29W39 L=165) 1104 246 3 (1326/ 408-1477/ 578) -16.7 W29-W49 S32-S25
15 1223 529 (S31W25 L=151) 340 91 0 (1168/ 515-1265/ 543) 15.9 W20-W27 S32-S29
16 719 489 (S46E11 L=116) 717 104 2 ( 669/ 467- 788/ 521) 15.3 E15-E04 S47-S43
17 1410 373 (S36W47 L=174) 541 72 1 (1381/ 341-1451/ 405) 78.7 W44-W49 S38-S33
18 738 237 (S68E04 L=122) 971 137 3 ( 673/ 210- 799/ 265) -2.9 E15-W06 S69-S65
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Download FITS filament maps as tar archive
» All Filament Data of 20230215 ...
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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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