|
|
|
|
| 20140207 - Latest Filament data |
|
Available data for 20140207: »12 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 447 1689 (N28E56 L=359) 1450 292 2 ( 382/1654- 502/1721) -7.6 E65-E49 N25-N30
2 588 1400 (N10E33 L= 22) 420 118 0 ( 552/1367- 630/1448) -29.7 E36-E29 N07-N12
3 985 1230 (N05E05 L= 50) 183 47 0 ( 953/1218-1010/1245) 0.0 E07-E03 N04-N06
4 1820 1041 (N10W53 L=109) 2460 534 5 (1759/ 916-1876/1187) 83.3 W47-W61 N02-N19
5 1769 1110 (N12W48 L=103) 306 32 0 (1755/1082-1782/1137) -76.0 W46-W48 N10-N14
6 224 1064 (S14E56 L=359) 932 139 3 ( 186/1007- 258/1125) -45.0 E61-E52 S17-S10
7 259 1029 (S16E52 L= 3) 920 241 1 ( 186/ 954- 312/1118) 45.0 E59-E48 S20-S09
8 301 961 (S19E48 L= 8) 1201 289 1 ( 238/ 841- 371/1076) 56.3 E53-E42 S27-S12
9 644 1044 (S11E23 L= 32) 200 44 0 ( 616/1026- 667/1061) 0.0 E25-E21 S11-S09
10 1040 941 (S11W02 L= 58) 277 87 0 ( 990/ 925-1087/ 957) 21.8 W00-W05 S12-S09
11 738 838 (S22E15 L= 41) 415 143 0 ( 652/ 797- 793/ 874) 0.0 E20-E10 S23-S19
12 458 768 (S30E35 L= 21) 1072 259 2 ( 358/ 720- 562/ 815) 22.4 E43-E26 S33-S25
13 1627 748 (S11W44 L= 99) 813 147 2 (1562/ 706-1685/ 807) 32.0 W40-W48 S14-S08
14 1323 742 (S18W23 L= 79) 245 63 1 (1299/ 704-1338/ 769) -45.0 W21-W24 S19-S15
15 1096 725 (S23W09 L= 65) 437 131 0 (1028/ 704-1154/ 747) 23.2 W05-W13 S24-S20
16 1704 646 (S15W54 L=109) 4859 802 15 (1557/ 479-1833/ 746) 63.4 W41-W69 S27-S07
17 879 597 (S34E02 L= 53) 393 74 1 ( 831/ 567- 916/ 629) -45.0 E05-W00 S36-S32
18 1142 456 (S39W20 L= 76) 849 211 0 (1054/ 426-1237/ 519) 38.7 W13-W24 S41-S32
19 965 465 (S42W07 L= 63) 267 41 1 ( 944/ 444- 986/ 490) -45.0 W05-W09 S43-S39
|
|
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.
|
|
|
|