|
|
|
|
| 20230311 - Filament data for 11 UTC |
|
Available data for 20230311: »06 UTC »07 UTC »08 UTC »10 UTC »11 UTC »12 UTC »13 UTC »14 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 890 1708 (N30E30 L=140) 1890 401 1 ( 813/1587- 985/1780) 82.4 E35-E22 N21-N36
2 1306 1661 (N40E01 L=169) 673 156 1 (1243/1600-1345/1714) -29.1 E06-W03 N36-N42
3 429 1660 (N17E63 L=107) 1597 186 5 ( 358/1630- 515/1693) 14.9 E72-E54 N14-N20
4 494 1474 (N06E45 L=125) 858 126 1 ( 429/1441- 547/1512) 50.2 E49-E41 N03-N09
5 1808 1403 (N40W50 L=220) 727 105 1 (1775/1354-1838/1440) -23.2 W45-W54 N37-N43
6 586 1220 (S06E30 L=139) 244 42 1 ( 557/1201- 607/1241) 45.0 E32-E28 S07-S04
7 1518 1192 (N15W24 L=194) 255 69 0 (1504/1153-1531/1228) 90.0 W23-W25 N13-N17
8 889 1125 (S05E10 L=160) 251 95 0 ( 876/1077- 907/1170) -68.2 E11-E09 S07-S02
9 1704 1006 (N11W42 L=212) 609 187 1 (1663/ 915-1741/1088) -45.0 W37-W47 N06-N15
10 848 870 (S20E06 L=164) 544 212 0 ( 759/ 794- 898/ 920) -20.0 E12-E01 S23-S18
11 294 830 (S35E49 L=121) 928 189 0 ( 234/ 777- 336/ 907) 39.8 E56-E44 S39-S29
12 463 759 (S36E31 L=138) 806 210 0 ( 427/ 676- 524/ 849) -45.0 E34-E25 S40-S30
13 1598 719 (S08W43 L=213) 533 108 0 (1561/ 682-1621/ 769) 90.0 W41-W45 S10-S04
14 1466 448 (S26W49 L=218) 851 200 1 (1376/ 418-1547/ 494) 48.4 W42-W52 S29-S20
15 1111 335 (S45W33 L=202) 404 85 0 (1089/ 298-1142/ 372) -56.3 W30-W35 S47-S41
16 670 309 (S64E04 L=166) 1448 170 2 ( 595/ 268- 738/ 360) 0.0 E15-W06 S67-S60
17 1568 332 (S28W69 L=239) 1785 165 3 (1490/ 304-1635/ 359) 11.3 W59-W84 S31-S25
18 1246 228 (S46W54 L=224) 2926 253 6 (1163/ 185-1351/ 299) 3.9 W39-W69 S50-S42
|
Download FITS filament maps as tar archive
» All Filament Data of 20230311 ...
|
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.
|
|
|
|