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| 20230607 - Latest Filament data |
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Available data for 20230607: »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 1172 1860 (N65E08 L= 78) 5768 422 6 (1009/1774-1351/1931) -3.3 E43-W18 N58-N73
2 1103 1689 (N46E07 L= 79) 2117 383 5 ( 914/1627-1236/1738) 0.0 E25-W04 N42-N47
3 565 1662 (N33E50 L= 36) 1253 244 1 ( 499/1575- 660/1705) 74.7 E54-E42 N26-N37
4 366 1498 (N19E59 L= 28) 614 98 1 ( 345/1465- 405/1546) -21.8 E63-E53 N16-N22
5 361 1351 (N10E52 L= 35) 1162 228 3 ( 307/1272- 429/1426) -36.0 E60-E45 N05-N13
6 1532 1226 (N20W30 L=117) 729 159 1 (1483/1167-1587/1283) -29.1 W26-W35 N17-N22
7 1514 1145 (N15W30 L=116) 254 99 0 (1469/1116-1559/1166) 26.6 W26-W32 N12-N16
8 1605 1088 (N12W37 L=123) 258 39 0 (1582/1072-1632/1102) 0.0 W35-W39 N11-N13
9 1877 1051 (N14W65 L=152) 776 96 1 (1855/1012-1903/1093) -68.2 W62-W70 N12-N17
10 386 978 (S12E42 L= 44) 324 108 0 ( 348/ 936- 416/1022) 50.2 E44-E39 S15-S09
11 165 862 (S23E68 L= 18) 726 66 0 ( 147/ 832- 179/ 902) -63.4 E72-E65 S24-S20
12 288 776 (S27E52 L= 34) 393 89 0 ( 265/ 732- 311/ 819) 50.2 E55-E48 S29-S23
13 1183 665 (S19W16 L=102) 898 344 2 (1057/ 554-1282/ 778) 67.6 W09-W20 S28-S11
14 778 744 (S21E11 L= 75) 308 62 1 ( 745/ 714- 810/ 767) -11.3 E13-E08 S22-S19
15 607 704 (S26E23 L= 63) 636 158 2 ( 536/ 683- 674/ 740) 16.7 E28-E18 S27-S22
16 1710 651 (S12W56 L=142) 386 26 1 (1685/ 631-1732/ 668) 14.0 W53-W58 S13-S11
17 1475 504 (S25W42 L=128) 291 39 0 (1460/ 483-1494/ 529) -56.3 W39-W43 S26-S23
18 701 205 (S70E22 L= 65) 1030 95 0 ( 672/ 176- 742/ 250) -63.4 E27-E14 S74-S63
19 954 177 (S64W19 L=106) 659 79 0 ( 924/ 156- 994/ 209) -13.0 W13-W27 S66-S60
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Download FITS filament maps as tar archive
» All Filament Data of 20230607 ...
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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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