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| 20230215 - Filament data for 09 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
1 913 1566 (N24E18 L=109) 2583 671 7 ( 760/1387-1126/1802) -29.4 E40-E01 N15-N38
2 492 1741 (N30E61 L= 66) 1058 116 2 ( 458/1694- 535/1787) -17.7 E74-E52 N26-N33
3 661 1609 (N22E37 L= 91) 369 109 1 ( 612/1572- 705/1646) 66.8 E38-E34 N18-N25
4 1212 1620 (N34E01 L=127) 282 41 1 (1190/1597-1237/1644) 0.0 E02-W01 N32-N35
5 379 1572 (N16E59 L= 69) 398 67 0 ( 356/1552- 410/1597) -7.1 E62-E54 N14-N17
6 693 1386 (N08E27 L=100) 1259 369 1 ( 660/1231- 719/1583) -69.1 E32-E22 N00-N21
7 1472 1433 (N27W20 L=148) 503 128 1 (1453/1387-1503/1486) 76.0 W18-W22 N23-N31
8 1015 1406 (N15E08 L=119) 238 61 0 ( 985/1381-1043/1427) -14.0 E09-E05 N14-N16
9 1622 1384 (N28W33 L=160) 369 102 0 (1598/1330-1644/1424) -51.3 W30-W34 N24-N30
10 863 982 (S12E09 L=119) 214 121 1 ( 816/ 946- 906/1007) 45.0 E10-E05 S15-S10
11 990 912 (S14W00 L=127) 841 224 3 ( 934/ 837-1093/ 966) 58.0 E02-W05 S18-S10
12 859 857 (S19E07 L=121) 250 53 2 ( 836/ 830- 883/ 889) -56.3 E08-E05 S20-S17
13 589 835 (S26E24 L=103) 325 102 0 ( 543/ 805- 629/ 857) -18.4 E27-E21 S26-S24
14 543 699 (S35E27 L=100) 343 81 0 ( 512/ 680- 587/ 726) -9.5 E29-E23 S36-S33
15 1378 520 (S28W36 L=163) 966 205 0 (1311/ 449-1457/ 583) -14.0 W29-W45 S30-S25
16 1220 535 (S31W24 L=152) 338 91 0 (1179/ 520-1273/ 550) 26.6 W21-W27 S32-S29
17 710 491 (S46E11 L=116) 802 145 1 ( 646/ 465- 778/ 525) 9.5 E17-E05 S47-S43
18 1398 373 (S36W47 L=174) 604 101 2 (1366/ 334-1438/ 410) -80.5 W43-W49 S39-S33
19 737 239 (S68E04 L=123) 903 162 2 ( 675/ 215- 817/ 269) -2.6 E15-W08 S69-S64
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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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