|
|
|
|
| 20230620 - Filament data for 06 UTC |
|
Available data for 20230620: »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
1 364 1616 (N32E70 L=208) 1170 99 1 ( 342/1563- 387/1663) -28.3 E81-E65 N28-N35
2 341 1480 (N23E60 L=218) 421 68 0 ( 314/1461- 377/1502) 0.0 E65-E55 N21-N24
3 525 1434 (N22E40 L=238) 372 55 0 ( 502/1400- 545/1465) 90.0 E41-E38 N19-N24
4 864 1243 (N14E12 L=266) 204 99 0 ( 823/1225- 913/1255) 9.5 E14-E08 N12-N14
5 1518 996 (N04W32 L=310) 960 228 0 (1435/ 941-1577/1080) 52.1 W26-W36 N00-N09
6 1004 995 (S00E01 L=277) 469 97 3 ( 961/ 970-1048/1039) 14.0 E03-W01 S01-N02
7 157 867 (S17E70 L=208) 1958 166 4 ( 137/ 778- 185/ 934) 70.0 E75-E64 S23-S12
8 1029 849 (S09W02 L=280) 399 138 1 ( 988/ 809-1085/ 872) 31.0 W00-W05 S11-S07
9 875 831 (S12E08 L=271) 304 60 1 ( 842/ 809- 912/ 848) 0.0 E09-E05 S12-S10
10 1135 801 (S11W09 L=287) 213 65 1 (1103/ 774-1162/ 827) -26.6 W06-W10 S12-S09
11 430 782 (S19E39 L=239) 331 66 1 ( 407/ 759- 449/ 817) -71.6 E41-E37 S20-S17
12 769 761 (S17E14 L=265) 233 49 0 ( 737/ 745- 792/ 780) 26.6 E16-E12 S18-S15
13 1683 710 (S12W50 L=329) 946 160 0 (1654/ 640-1725/ 779) 77.5 W48-W52 S16-S07
14 1056 723 (S17W05 L=283) 519 161 0 ( 980/ 701-1120/ 761) -6.3 W00-W09 S18-S15
15 300 714 (S25E53 L=225) 681 117 0 ( 252/ 694- 359/ 759) 19.7 E59-E45 S27-S21
16 1456 666 (S17W33 L=311) 618 196 0 (1403/ 634-1516/ 719) 39.8 W28-W36 S19-S13
17 1706 626 (S18W56 L=334) 973 123 3 (1671/ 562-1741/ 663) 66.8 W52-W59 S22-S15
18 1040 598 (S25W05 L=284) 219 64 0 (1016/ 566-1053/ 624) -53.1 W03-W06 S27-S23
19 898 509 (S33E04 L=275) 237 69 0 ( 860/ 496- 927/ 522) 21.8 E06-E01 S33-S31
|
Download FITS filament maps as tar archive
» All Filament Data of 20230620 ...
|
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.
|
|
|
|