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| 20231006 - Filament data for 07 UTC |
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Available data for 20231006: »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
1 636 1557 (N50E12 L=279) 407 75 2 ( 609/1517- 661/1595) 51.3 E14-E08 N47-N52
2 871 1542 (N41W07 L=297) 589 105 2 ( 828/1509- 921/1572) -7.1 W02-W10 N38-N42
3 1003 1525 (N35W15 L=305) 487 82 1 ( 968/1492-1043/1551) 18.4 W12-W18 N33-N37
4 418 1525 (N54E37 L=253) 394 62 1 ( 394/1491- 434/1549) -68.2 E41-E34 N51-N56
5 324 1515 (N56E53 L=237) 645 105 0 ( 289/1479- 366/1536) 4.8 E60-E45 N54-N57
6 1685 1378 (N06W53 L=343) 845 110 2 (1641/1329-1722/1425) 18.4 W47-W56 N04-N08
7 1355 1336 (N14W28 L=318) 383 90 0 (1324/1310-1394/1369) -68.2 W26-W30 N11-N16
8 672 1214 (N26E16 L=274) 231 49 1 ( 653/1183- 697/1237) 71.6 E17-E14 N24-N27
9 179 1177 (N35E65 L=226) 849 84 1 ( 143/1143- 214/1205) -21.0 E72-E58 N32-N37
10 722 1127 (N20E15 L=275) 228 104 0 ( 674/1089- 746/1153) -59.0 E17-E13 N17-N22
11 1682 1056 (S11W41 L=331) 268 18 0 (1665/1035-1703/1074) 18.4 W39-W42 S11-S09
12 1841 958 (S22W54 L=345) 421 93 1 (1804/ 939-1869/ 988) 7.1 W49-W58 S23-S20
13 704 906 (N08E21 L=269) 361 116 0 ( 652/ 884- 760/ 925) -23.2 E24-E17 N06-N09
14 820 689 (S07E20 L=270) 299 68 0 ( 787/ 675- 866/ 709) -31.0 E22-E17 S08-S05
15 1001 612 (S16E13 L=278) 493 191 0 ( 951/ 583-1036/ 683) 29.7 E15-E08 S18-S12
16 1538 641 (S31W22 L=312) 265 103 0 (1520/ 585-1563/ 674) 45.0 W19-W24 S34-S29
17 1338 562 (S29W06 L=296) 921 240 2 (1260/ 493-1400/ 662) 30.3 W00-W12 S31-S24
18 1688 576 (S42W35 L=326) 1023 124 2 (1638/ 537-1720/ 623) 12.5 W29-W39 S44-S37
19 1048 222 (S46E29 L=261) 1471 222 1 ( 939/ 181-1125/ 275) 5.2 E41-E19 S47-S42
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Download FITS filament maps as tar archive
» All Filament Data of 20231006 ...
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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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