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| 20260614 - Filament data for 09 UTC |
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Available data for 20260614: »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
1 858 1561 (N32E20 L=270) 1285 291 0 ( 788/1426- 909/1671) -48.8 E28-E13 N23-N39
2 248 1458 (N17E70 L=220) 2247 241 8 ( 200/1376- 311/1555) 90.0 E76-E65 N11-N24
3 1519 1424 (N32W31 L=321) 672 185 1 (1486/1337-1572/1460) 52.1 W27-W35 N25-N34
4 271 1305 (N09E58 L=232) 691 149 1 ( 243/1239- 314/1373) -32.5 E63-E52 N05-N12
5 821 1303 (N15E16 L=274) 210 90 1 ( 794/1265- 850/1349) 68.2 E17-E14 N12-N18
6 1801 1223 (N22W56 L=346) 365 31 0 (1775/1205-1821/1239) 0.0 W52-W58 N20-N23
7 1525 1123 (N13W31 L=321) 257 104 0 (1495/1082-1548/1170) 63.4 W29-W32 N09-N15
8 201 1115 (S04E62 L=228) 456 66 1 ( 185/1075- 217/1154) 78.7 E63-E59 S06-S01
9 241 1095 (S04E56 L=234) 383 31 1 ( 227/1064- 256/1123) -76.0 E58-E54 S06-S02
10 1165 1080 (N06W08 L=298) 237 76 0 (1129/1067-1203/1106) -21.8 W05-W10 N05-N07
11 489 1085 (S02E35 L=255) 251 25 0 ( 472/1061- 508/1103) 56.3 E36-E33 S03-N00
12 189 983 (S12E62 L=228) 494 99 0 ( 144/ 965- 229/1002) 9.5 E68-E56 S13-S10
13 603 805 (S17E24 L=266) 362 97 2 ( 570/ 757- 635/ 849) 71.6 E26-E22 S20-S14
14 334 790 (S22E46 L=243) 521 87 0 ( 306/ 758- 371/ 836) -38.7 E48-E42 S23-S19
15 370 683 (S29E44 L=246) 299 90 0 ( 327/ 670- 411/ 695) 0.0 E48-E40 S29-S27
16 1045 589 (S26W07 L=297) 240 29 0 (1021/ 574-1068/ 608) 45.0 W05-W08 S26-S24
17 866 549 (S31E05 L=285) 301 85 0 ( 821/ 534- 910/ 563) 9.5 E07-E01 S31-S30
18 1438 374 (S36W44 L=334) 652 85 1 (1400/ 349-1472/ 405) 63.4 W40-W46 S37-S33
19 1289 378 (S38W31 L=321) 672 128 3 (1218/ 357-1349/ 398) -4.8 W24-W36 S39-S35
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Download FITS filament maps as tar archive
» All Filament Data of 20260614 ...
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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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