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| 20240411 - Filament data for 12 UTC |
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Available data for 20240411: »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
1 623 1828 (N32E65 L=265) 978 108 1 ( 591/1781- 652/1875) -39.8 E75-E59 N27-N37
2 939 1704 (N32E29 L=301) 1088 204 0 ( 854/1655-1018/1735) 45.0 E31-E23 N26-N35
3 790 1599 (N21E32 L=298) 450 110 0 ( 760/1550- 818/1641) -81.9 E34-E30 N16-N23
4 1520 1554 (N42W17 L=347) 488 60 0 (1487/1532-1551/1578) 45.0 W14-W19 N39-N44
5 583 1345 (N00E35 L=295) 421 105 1 ( 525/1328- 641/1359) 7.1 E39-E31 S01-N02
6 1441 1154 (N13W20 L=350) 207 60 0 (1415/1132-1470/1175) 53.1 W18-W21 N11-N15
7 307 1107 (S19E50 L=280) 358 39 0 ( 286/1085- 328/1130) -21.8 E52-E47 S20-S18
8 628 1089 (S13E25 L=305) 498 147 0 ( 570/1052- 689/1115) 6.3 E28-E19 S14-S11
9 1743 1013 (N15W45 L= 15) 1144 274 2 (1686/ 908-1818/1112) -29.7 W38-W54 N11-N19
10 1278 1043 (N02W13 L=343) 542 102 0 (1248/ 998-1324/1094) 80.5 W11-W14 N00-N06
11 1541 995 (N08W31 L= 0) 263 49 0 (1527/ 968-1556/1031) -56.3 W29-W32 N06-N09
12 267 962 (S29E52 L=278) 349 58 0 ( 254/ 935- 279/ 996) 76.0 E53-E50 S30-S26
13 509 923 (S25E29 L=301) 307 95 0 ( 494/ 879- 531/ 970) -51.3 E30-E26 S27-S22
14 269 856 (S35E51 L=279) 579 94 1 ( 239/ 832- 317/ 885) 6.3 E54-E45 S37-S33
15 1160 784 (S15W15 L=344) 308 98 0 (1116/ 764-1206/ 814) 45.0 W12-W16 S16-S12
16 1035 769 (S19W08 L=338) 232 100 0 ( 987/ 742-1078/ 807) -8.1 W04-W11 S20-S18
17 631 708 (S35E16 L=314) 726 199 0 ( 554/ 691- 741/ 732) 15.9 E21-E07 S37-S31
18 424 664 (S44E33 L=297) 612 73 1 ( 386/ 641- 472/ 692) 0.0 E37-E28 S45-S42
19 1409 438 (S26W46 L= 16) 2618 448 2 (1223/ 388-1619/ 502) 38.0 W34-W58 S34-S15
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Download FITS filament maps as tar archive
» All Filament Data of 20240411 ...
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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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