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| 20220912 - Filament data for 10 UTC |
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Available data for 20220912: »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
1 881 1744 (N57W17 L= 39) 401 71 1 ( 849/1723- 909/1764) 7.1 W12-W20 N54-N58
2 1528 1600 (N25W54 L= 77) 952 207 1 (1449/1548-1612/1640) -45.0 W48-W58 N19-N29
3 533 1566 (N54E26 L=357) 327 53 1 ( 498/1546- 556/1587) -23.2 E30-E23 N51-N55
4 1356 1542 (N28W37 L= 60) 357 137 0 (1299/1498-1399/1571) -66.8 W34-W38 N23-N30
5 1365 1438 (N21W33 L= 56) 448 157 0 (1295/1394-1430/1462) -49.4 W28-W35 N17-N24
6 1351 1377 (N18W29 L= 52) 227 51 1 (1324/1357-1382/1392) -26.6 W27-W31 N17-N19
7 1143 1263 (N18W13 L= 36) 776 233 2 (1030/1203-1218/1327) -51.3 W08-W16 N12-N24
8 417 1153 (N28E38 L=345) 473 100 2 ( 369/1121- 462/1179) -18.4 E42-E33 N25-N30
9 870 1104 (N15E07 L= 16) 263 61 1 ( 848/1066- 886/1138) 45.0 E08-E05 N13-N17
10 1877 964 (S21W60 L= 83) 1475 232 2 (1838/ 851-1917/1057) 45.0 W54-W68 S26-S16
11 1182 951 (S01W07 L= 30) 855 232 1 (1132/ 855-1240/1044) 41.6 W03-W12 S05-N03
12 454 997 (N18E37 L=346) 280 67 0 ( 442/ 962- 468/1034) -90.0 E37-E35 N15-N20
13 1879 828 (S30W61 L= 84) 539 53 1 (1850/ 806-1906/ 843) -15.3 W55-W66 S31-S27
14 1350 703 (S20W11 L= 34) 436 150 0 (1276/ 660-1395/ 730) -35.5 W06-W13 S23-S17
15 1515 505 (S39W20 L= 43) 1036 195 2 (1439/ 433-1570/ 569) 24.8 W12-W25 S42-S35
16 1248 525 (S28W01 L= 24) 578 193 0 (1166/ 494-1329/ 568) -5.2 E04-W07 S29-S26
17 1395 408 (S42W09 L= 31) 344 54 0 (1376/ 388-1421/ 439) -90.0 W06-W10 S43-S38
18 1301 354 (S43E00 L= 22) 324 53 0 (1284/ 332-1325/ 385) -90.0 E01-W01 S45-S40
19 686 248 (S34E52 L=331) 821 100 0 ( 658/ 219- 735/ 288) 81.9 E55-E48 S37-S30
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Download FITS filament maps as tar archive
» All Filament Data of 20220912 ...
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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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