|
|
|
|
| 20140218 - Filament data for 10 UTC |
|---|
|
Available data for 20140218: »08 UTC »09 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
1 480 1621 (N20E51 L=221) 487 110 2 ( 447/1599- 532/1642) 0.0 E54-E46 N18-N21
2 203 1145 (S13E60 L=212) 4713 799 17 ( 119/ 955- 283/1278) 64.5 E69-E52 S24-S04
3 316 1234 (S06E51 L=221) 398 102 1 ( 301/1188- 330/1278) 90.0 E52-E48 S09-S03
4 330 1092 (S14E47 L=225) 350 106 2 ( 293/1073- 368/1122) 18.4 E49-E43 S15-S12
5 390 1080 (S14E41 L=230) 248 88 0 ( 350/1057- 426/1107) 38.7 E44-E38 S16-S12
6 919 1035 (S08E06 L=265) 324 85 0 ( 880/ 998- 948/1072) 71.6 E07-E05 S11-S05
7 402 1036 (S17E40 L=232) 258 63 0 ( 380/1009- 427/1063) 53.1 E41-E38 S18-S14
8 778 981 (S14E14 L=258) 409 151 1 ( 691/ 963- 844/ 996) 18.4 E18-E09 S16-S12
9 387 913 (S24E40 L=232) 324 85 2 ( 349/ 884- 406/ 936) -21.8 E43-E38 S26-S22
10 1223 790 (S16W17 L=288) 824 311 1 (1093/ 751-1372/ 868) 3.2 W07-W25 S18-S13
11 1289 835 (S12W19 L=291) 225 81 0 (1256/ 814-1335/ 864) 0.0 W16-W22 S13-S10
12 822 764 (S26E07 L=265) 1478 432 4 ( 644/ 674-1029/ 852) 39.0 E18-W03 S34-S16
13 1200 595 (S28W21 L=293) 304 93 0 (1154/ 581-1247/ 617) 18.4 W18-W24 S29-S26
14 1834 577 (S11W74 L=345) 726 61 1 (1813/ 546-1853/ 604) 90.0 W71-W76 S13-S09
15 615 536 (S45E19 L=252) 630 135 2 ( 592/ 485- 644/ 596) -60.3 E21-E16 S48-S40
16 1574 558 (S21W48 L=319) 477 54 0 (1542/ 528-1613/ 588) 63.4 W45-W49 S22-S18
17 946 500 (S40W07 L=279) 469 155 1 ( 874/ 471-1026/ 537) 45.0 W02-W11 S43-S35
18 738 450 (S49E08 L=264) 266 44 1 ( 711/ 433- 760/ 475) 11.3 E10-E05 S49-S46
19 1207 404 (S40W30 L=301) 523 108 1 (1141/ 378-1246/ 438) 56.3 W25-W31 S42-S36
|
|
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.
|
|
|
|
