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| 20240830 - Latest Filament data |
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Available data for 20240830: »06 UTC »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 1199 1592 (N36W28 L=293) 1398 358 1 (1037/1537-1340/1622) -12.3 W15-W38 N32-N39
2 1524 1601 (N27W53 L=317) 854 124 1 (1454/1578-1590/1621) -12.1 W46-W60 N25-N29
3 1646 1529 (N19W59 L=323) 542 71 1 (1612/1496-1681/1561) -78.7 W55-W61 N16-N21
4 207 1307 (N39E66 L=198) 497 38 0 ( 185/1289- 235/1324) 7.1 E69-E61 N38-N40
5 1451 1274 (N11W32 L=296) 269 110 0 (1409/1236-1496/1303) -51.3 W29-W33 N07-N13
6 1055 1209 (N17W06 L=270) 431 152 0 (1017/1136-1079/1257) 82.9 W04-W07 N12-N20
7 527 1071 (N20E30 L=234) 327 83 1 ( 499/1050- 568/1103) -38.7 E32-E27 N17-N21
8 521 921 (N11E33 L=231) 415 162 0 ( 486/ 844- 562/ 991) -73.3 E34-E31 N05-N15
9 1878 819 (S28W61 L=325) 2906 212 6 (1816/ 746-1933/ 910) 18.4 W52-W73 S32-S24
10 641 753 (S01E29 L=235) 920 309 0 ( 576/ 638- 746/ 820) 21.8 E36-E21 S06-N02
11 1578 795 (S20W29 L=294) 234 54 0 (1554/ 771-1604/ 820) 26.6 W27-W31 S20-S18
12 482 638 (S05E43 L=221) 870 217 2 ( 408/ 593- 570/ 684) -35.0 E48-E37 S09-S01
13 462 552 (S10E48 L=216) 690 79 3 ( 421/ 520- 499/ 586) 0.0 E52-E45 S12-S08
14 306 518 (S11E67 L=197) 2016 129 5 ( 256/ 469- 355/ 567) -50.2 E74-E60 S14-S07
15 589 520 (S14E40 L=224) 365 81 0 ( 566/ 482- 611/ 564) 80.5 E41-E38 S17-S11
16 519 469 (S17E48 L=216) 1006 216 4 ( 476/ 399- 564/ 546) 36.9 E55-E41 S20-S11
17 1447 424 (S42W15 L=279) 1160 210 3 (1364/ 358-1532/ 505) 17.4 W07-W23 S45-S36
18 597 406 (S22E45 L=219) 694 90 1 ( 555/ 362- 622/ 448) -80.5 E47-E41 S25-S19
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Download FITS filament maps as tar archive
» All Filament Data of 20240830 ...
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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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