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| 20221007 - Filament data for 08 UTC |
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Available data for 20221007: »05 UTC »06 UTC »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 840 1783 (N60W20 L= 74) 327 55 0 ( 826/1751- 856/1810) 24.0 W15-W24 N57-N62
2 623 1688 (N61E10 L= 44) 1693 242 2 ( 512/1638- 730/1738) -6.1 E25-W03 N58-N64
3 483 1620 (N60E30 L= 24) 343 41 1 ( 465/1598- 502/1647) -50.2 E32-E26 N57-N63
4 1336 1589 (N28W39 L= 93) 288 77 0 (1297/1568-1366/1607) -53.1 W37-W40 N26-N30
5 409 1562 (N58E40 L= 14) 427 71 0 ( 391/1524- 436/1593) 68.2 E42-E36 N54-N59
6 734 1503 (N42E05 L= 49) 672 186 1 ( 688/1424- 794/1570) -77.0 E06-E02 N35-N48
7 1123 1443 (N27W18 L= 73) 550 250 0 ( 999/1414-1222/1460) -33.7 W11-W23 N22-N31
8 830 1268 (N25E05 L= 49) 968 267 6 ( 710/1224- 941/1322) -28.3 E12-W01 N20-N28
9 825 1196 (N21E07 L= 47) 303 95 2 ( 784/1160- 852/1222) -63.4 E09-E04 N18-N22
10 965 1183 (N17W01 L= 55) 249 63 1 ( 936/1153- 984/1216) 63.4 W00-W02 N14-N18
11 641 1092 (N20E21 L= 33) 492 172 1 ( 572/1060- 726/1124) -33.7 E25-E16 N16-N22
12 1672 1025 (S12W39 L= 93) 396 147 2 (1647/ 975-1702/1090) 35.5 W36-W43 S14-S09
13 1807 913 (S23W49 L=103) 1424 322 0 (1700/ 833-1880/1042) 12.8 W38-W60 S27-S18
14 1649 892 (S19W34 L= 88) 535 90 1 (1620/ 850-1685/ 932) -71.6 W31-W36 S22-S16
15 1573 796 (S22W27 L= 81) 523 151 0 (1521/ 737-1618/ 856) 29.1 W22-W31 S24-S19
16 1563 644 (S32W24 L= 78) 354 115 0 (1519/ 624-1614/ 675) 0.0 W20-W28 S32-S29
17 1095 562 (S22E09 L= 45) 501 146 0 (1051/ 504-1143/ 617) 32.0 E12-E04 S24-S19
18 946 369 (S30E26 L= 28) 349 112 0 ( 891/ 349- 983/ 397) 7.1 E30-E22 S31-S28
19 892 181 (S44E45 L= 9) 431 57 1 ( 872/ 154- 913/ 206) 18.4 E50-E41 S46-S41
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Download FITS filament maps as tar archive
» All Filament Data of 20221007 ...
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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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