|
|
|
|
| 20240910 - Filament data for 06 UTC |
|
Available data for 20240910: »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 1132 1728 (N46W34 L=158) 323 46 1 (1116/1692-1148/1758) 33.7 W31-W37 N43-N47
2 1362 1563 (N28W39 L=162) 936 201 1 (1283/1504-1443/1602) 0.0 W30-W46 N26-N29
3 1479 1414 (N17W39 L=162) 572 176 1 (1401/1377-1549/1458) -4.4 W32-W45 N15-N17
4 1060 1348 (N25W11 L=134) 758 162 2 (1003/1302-1136/1376) -12.5 W06-W15 N22-N26
5 1772 1029 (S13W48 L=171) 5904 760 17 (1579/ 813-1887/1242) 18.4 W28-W67 S21-S03
6 1029 1164 (N15W04 L=127) 226 85 0 ( 998/1123-1052/1200) -78.7 W02-W04 N12-N17
7 1157 1099 (N08W09 L=132) 203 115 0 (1126/1056-1197/1146) 26.6 W06-W12 N06-N09
8 841 1029 (N12E10 L=113) 189 55 0 ( 808/1015- 863/1048) 0.0 E12-E08 N10-N12
9 543 969 (N15E30 L= 93) 472 85 1 ( 501/ 946- 583/1001) -33.7 E33-E27 N12-N16
10 759 897 (N06E18 L=105) 302 101 1 ( 732/ 847- 775/ 935) 78.7 E19-E16 N03-N08
11 1800 740 (S32W49 L=172) 785 163 0 (1739/ 703-1844/ 804) 8.7 W41-W54 S33-S29
12 823 751 (S04E18 L=105) 512 162 0 ( 755/ 697- 897/ 793) -58.0 E21-E14 S08-N00
13 1497 686 (S25W20 L=144) 681 126 3 (1463/ 642-1539/ 753) -83.7 W18-W23 S28-S19
14 1506 553 (S34W19 L=142) 1752 392 1 (1385/ 429-1597/ 714) 31.8 W07-W28 S39-S25
15 1153 554 (S23E04 L=119) 423 165 0 (1092/ 509-1207/ 615) 24.0 E09-W00 S24-S20
16 1656 480 (S46W34 L=157) 982 116 1 (1610/ 439-1700/ 525) 5.2 W28-W39 S50-S42
17 973 419 (S28E20 L=104) 417 123 0 ( 938/ 392-1025/ 471) -74.1 E21-E16 S30-S23
18 422 398 (S18E62 L= 61) 569 50 1 ( 404/ 367- 437/ 430) 39.8 E65-E59 S20-S15
|
Download FITS filament maps as tar archive
» All Filament Data of 20240910 ...
|
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.
|
|
|
|