|
|
|
|
| 20140331 - Filament data for 12 UTC |
|---|
|
Available data for 20140331: »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
1 334 1607 (N11E69 L= 21) 1964 342 5 ( 293/1542- 375/1663) -42.0 E76-E62 N06-N15
2 425 1566 (N10E56 L= 34) 706 113 1 ( 386/1540- 469/1598) 33.7 E60-E52 N07-N12
3 1081 1439 (N18E09 L= 82) 677 215 1 (1060/1343-1103/1542) -63.4 E11-E04 N12-N24
4 1451 1452 (N31W14 L=104) 479 77 1 (1425/1407-1478/1493) -51.3 W11-W15 N28-N33
5 1275 1298 (N15W06 L= 97) 632 186 0 (1246/1212-1296/1387) -63.4 W02-W08 N10-N20
6 1788 1085 (N20W47 L=137) 524 156 0 (1746/1043-1834/1106) 45.0 W43-W50 N16-N23
7 1084 1015 (S05W03 L= 94) 317 63 0 (1060/ 978-1104/1059) -78.7 W02-W04 S07-S02
8 515 925 (S25E28 L= 62) 941 176 0 ( 462/ 851- 565/1008) 74.7 E31-E25 S30-S19
9 1767 895 (N09W50 L=140) 552 128 2 (1735/ 865-1807/ 931) 56.3 W47-W53 N06-N12
10 316 795 (S38E43 L= 47) 1565 340 5 ( 225/ 746- 422/ 839) 22.8 E52-E33 S42-S33
11 1800 751 (N03W59 L=150) 1247 377 1 (1696/ 718-1892/ 808) 29.1 W49-W68 S01-N09
12 780 692 (S32E05 L= 85) 925 275 0 ( 706/ 600- 873/ 798) 72.6 E08-E02 S39-S23
13 1135 700 (S21W16 L=106) 620 172 0 (1041/ 651-1204/ 763) 65.6 W12-W17 S26-S15
14 1397 679 (S14W32 L=122) 276 115 1 (1358/ 654-1446/ 711) 0.0 W28-W35 S15-S13
15 1777 647 (S03W63 L=153) 401 47 0 (1754/ 620-1800/ 670) 76.0 W61-W64 S05-S01
16 1168 542 (S29W24 L=115) 274 80 0 (1122/ 526-1208/ 561) 45.0 W21-W26 S30-S26
17 1640 487 (S16W59 L=149) 445 61 0 (1610/ 466-1673/ 507) 53.1 W56-W61 S17-S13
18 573 471 (S54E16 L= 74) 318 40 0 ( 550/ 455- 604/ 488) 9.5 E18-E12 S54-S52
19 1399 354 (S31W49 L=139) 1862 264 5 (1285/ 314-1503/ 392) 39.8 W42-W55 S36-S26
|
|
Data will be available after one hour of observations. |
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.
|
|
|
|
