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| 20230309 - Filament data for 10 UTC |
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Available data for 20230309: »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC »13 UTC »14 UTC »15 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 595 1750 (N27E54 L=143) 3170 531 7 ( 451/1621- 715/1841) -87.1 E65-E42 N15-N35
2 1009 1772 (N39E26 L=171) 772 135 1 ( 970/1705-1035/1826) -33.7 E32-E20 N34-N42
3 455 1707 (N21E64 L=133) 604 57 0 ( 430/1681- 483/1743) -45.0 E68-E60 N19-N24
4 1588 1487 (N37W25 L=222) 420 100 0 (1571/1430-1602/1532) -74.1 W23-W26 N32-N39
5 1283 1329 (N17W07 L=204) 285 103 3 (1255/1289-1329/1368) 51.3 W05-W09 N13-N19
6 503 1234 (S07E36 L=160) 232 31 0 ( 488/1216- 524/1259) -45.0 E37-E34 S08-S05
7 1341 1238 (N13W13 L=209) 232 83 1 (1312/1215-1374/1254) 0.0 W10-W15 N11-N13
8 134 1182 (S16E73 L=123) 1278 130 3 ( 110/1115- 162/1241) 69.4 E80-E69 S19-S11
9 267 1138 (S17E54 L=143) 397 78 1 ( 237/1111- 294/1167) 53.1 E56-E51 S18-S14
10 303 1032 (S22E49 L=148) 391 39 0 ( 284/1004- 321/1064) -76.0 E50-E46 S24-S20
11 331 991 (S24E46 L=151) 270 53 1 ( 298/ 976- 356/1010) 0.0 E48-E43 S25-S22
12 221 962 (S28E57 L=139) 351 39 1 ( 200/ 942- 241/ 985) 26.6 E60-E54 S29-S26
13 1255 930 (S07W15 L=212) 268 51 2 (1229/ 899-1284/ 952) 76.0 W13-W16 S08-S04
14 1457 734 (S11W33 L=230) 735 208 1 (1362/ 679-1546/ 775) 51.3 W29-W38 S16-S06
15 1642 633 (S11W51 L=248) 309 102 0 (1622/ 597-1673/ 670) -76.0 W49-W53 S12-S08
16 1142 601 (S28W19 L=216) 584 256 0 (1017/ 574-1241/ 637) 28.3 W11-W24 S30-S22
17 1433 450 (S27W46 L=243) 1614 318 3 (1288/ 390-1573/ 492) 15.6 W34-W60 S31-S24
18 1071 407 (S42W24 L=221) 1087 200 1 ( 979/ 381-1168/ 440) 32.5 W18-W29 S44-S36
19 522 377 (S63E27 L=170) 1466 221 4 ( 428/ 333- 619/ 420) 1.9 E42-E12 S66-S59
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Download FITS filament maps as tar archive
» All Filament Data of 20230309 ...
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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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