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| 20250730 - Filament data for 11 UTC |
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Available data for 20250730: »05 UTC »06 UTC »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 1412 1712 (N45W48 L=226) 1241 224 1 (1330/1661-1506/1764) 2.0 W37-W66 N42-N46
2 1184 1460 (N31W16 L=194) 814 175 2 (1106/1416-1257/1505) -33.7 W11-W20 N27-N34
3 1750 1434 (N20W62 L=240) 467 58 1 (1715/1416-1780/1449) -15.9 W58-W65 N19-N21
4 355 1355 (N31E49 L=129) 1970 362 5 ( 209/1319- 514/1394) 3.4 E68-E34 N28-N33
5 1776 1311 (N13W59 L=237) 664 146 1 (1713/1270-1839/1344) -28.6 W53-W65 N09-N15
6 210 1198 (N21E62 L=116) 1508 184 1 ( 176/1122- 242/1287) -37.6 E70-E56 N16-N26
7 111 1040 (N11E77 L=101) 885 86 2 ( 93/1001- 130/1071) 68.2 E82-E72 N08-N13
8 555 954 (N05E30 L=148) 363 92 1 ( 526/ 908- 581/1008) -71.6 E32-E28 N02-N08
9 1006 943 (N01E02 L=176) 224 99 0 ( 993/ 898-1028/ 994) 63.4 E02-W00 S01-N03
10 1685 838 (S14W43 L=221) 457 111 0 (1645/ 793-1713/ 892) 45.0 W39-W45 S16-S10
11 1283 863 (S07W14 L=192) 238 79 1 (1246/ 832-1308/ 883) 0.0 W11-W15 S08-S05
12 540 702 (S10E35 L=143) 281 74 0 ( 516/ 669- 562/ 740) -78.7 E35-E33 S12-S07
13 393 665 (S12E48 L=131) 307 53 1 ( 373/ 645- 418/ 689) -33.7 E49-E45 S13-S10
14 426 585 (S17E47 L=131) 870 101 2 ( 385/ 538- 476/ 623) -23.2 E50-E42 S20-S14
15 912 549 (S23E12 L=166) 570 134 1 ( 866/ 499- 957/ 607) 49.4 E15-E08 S26-S19
16 1107 424 (S34E01 L=177) 2967 538 8 ( 931/ 344-1245/ 594) 20.0 E13-W09 S39-S23
17 509 437 (S28E47 L=131) 621 78 0 ( 476/ 409- 552/ 472) -31.0 E48-E43 S30-S25
18 1543 329 (S51W42 L=220) 932 95 1 (1499/ 311-1598/ 348) -3.8 W35-W51 S52-S47
19 1292 246 (S54W14 L=192) 2079 271 3 (1182/ 207-1413/ 306) 7.1 W02-W27 S57-S49
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Download FITS filament maps as tar archive
» All Filament Data of 20250730 ...
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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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