|
|
|
|
| 20140401 - Filament data for 07 UTC |
|---|
|
Available data for 20140401: »06 UTC »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC »13 UTC »14 UTC »15 UTC »16 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 368 1595 (N11E64 L= 16) 1420 285 4 ( 318/1485- 421/1665) -81.3 E67-E61 N02-N15
2 801 1607 (N21E31 L= 49) 296 165 0 ( 756/1555- 826/1660) -29.1 E36-E27 N18-N23
3 1230 1374 (N19W02 L= 81) 807 287 0 (1206/1252-1261/1504) -68.2 E01-W06 N12-N27
4 1576 1374 (N30W24 L=104) 301 54 1 (1548/1350-1600/1397) -11.3 W21-W26 N28-N31
5 234 1316 (S09E63 L= 17) 908 173 4 ( 205/1285- 276/1357) -5.7 E67-E57 S10-S06
6 743 1281 (N00E23 L= 57) 405 134 0 ( 681/1244- 813/1304) 0.0 E26-E17 S01-N01
7 1422 1226 (N16W17 L= 97) 463 124 0 (1403/1169-1443/1294) -60.3 W14-W18 N12-N19
8 1238 929 (S06W14 L= 94) 482 99 1 (1215/ 871-1258/ 984) -74.1 W12-W15 S09-S02
9 168 961 (S31E59 L= 20) 1562 412 3 ( 88/ 938- 246/ 981) 10.0 E68-E51 S32-S28
10 665 891 (S23E17 L= 62) 694 128 3 ( 614/ 835- 711/ 944) 63.4 E19-E15 S27-S19
11 1825 865 (N10W57 L=137) 781 151 1 (1796/ 808-1842/ 944) -54.5 W54-W60 N06-N13
12 420 761 (S38E34 L= 46) 1377 307 3 ( 317/ 726- 540/ 811) 19.3 E43-E23 S42-S33
13 913 620 (S32W06 L= 85) 957 254 2 ( 831/ 540-1017/ 727) 76.0 W02-W08 S39-S23
14 1838 683 (N01W68 L=148) 999 269 1 (1780/ 663-1892/ 705) 17.4 W61-W77 S01-N04
15 1253 610 (S22W26 L=106) 466 143 0 (1177/ 578-1308/ 663) 60.9 W22-W28 S26-S17
16 1530 597 (S14W44 L=124) 351 117 0 (1493/ 579-1570/ 627) 0.0 W40-W47 S15-S12
17 1274 467 (S29W34 L=114) 381 58 1 (1238/ 452-1314/ 484) 21.8 W31-W36 S31-S27
18 1424 318 (S32W53 L=133) 443 54 1 (1393/ 305-1456/ 339) 21.8 W51-W56 S33-S30
|
|
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.
|
|
|
|
