|
|
|
|
| 20150114 - Filament data for 11 UTC |
|
Available data for 20150114: »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
1 916 1550 (N28E10 L=224) 241 60 1 ( 898/1514- 932/1582) -78.7 E11-E08 N25-N30
2 793 1486 (N23E18 L=217) 642 171 1 ( 700/1452- 858/1507) -9.5 E24-E12 N21-N24
3 700 1411 (N18E23 L=212) 216 55 0 ( 667/1389- 728/1431) -21.8 E25-E20 N16-N19
4 589 1366 (N15E30 L=205) 320 101 1 ( 575/1319- 604/1421) 90.0 E30-E28 N11-N18
5 344 1381 (N15E49 L=185) 299 61 0 ( 329/1349- 359/1409) -63.4 E50-E47 N13-N17
6 1878 1242 (N15W62 L=297) 2255 394 2 (1790/1131-1966/1355) -24.4 W53-W76 N09-N21
7 207 1294 (N10E61 L=173) 435 73 1 ( 184/1276- 228/1312) 9.5 E64-E58 N08-N11
8 1199 1262 (N11W09 L=244) 387 98 1 (1158/1225-1255/1308) -39.8 W06-W12 N08-N13
9 1580 1214 (N10W35 L=269) 524 149 2 (1511/1192-1647/1240) 0.0 W29-W39 N08-N12
10 394 1182 (N03E42 L=193) 241 56 1 ( 369/1162- 423/1195) 0.0 E43-E39 N01-N03
11 445 1064 (S04E37 L=197) 882 186 3 ( 425/ 976- 470/1170) -84.8 E38-E35 S09-N02
12 1772 1106 (N06W50 L=285) 314 113 2 (1747/1072-1814/1138) -26.6 W48-W54 N03-N07
13 842 1059 (S03E11 L=223) 222 50 2 ( 804/1042- 871/1079) -14.0 E13-E09 S04-S01
14 1861 981 (S01W61 L=295) 477 62 1 (1843/ 949-1882/1007) 63.4 W58-W63 S02-N00
15 156 869 (S15E65 L=170) 1854 346 8 ( 121/ 770- 192/ 971) -90.0 E69-E60 S21-S09
16 1587 911 (S08W37 L=271) 228 12 0 (1564/ 892-1606/ 926) 0.0 W34-W38 S08-S06
17 1130 757 (S20W08 L=242) 1125 258 0 (1029/ 662-1273/ 838) 40.6 W02-W16 S26-S14
18 1778 549 (S27W62 L=296) 1624 266 1 (1696/ 511-1843/ 617) 33.7 W53-W67 S30-S22
19 946 548 (S34E03 L=232) 214 41 1 ( 927/ 527- 971/ 570) -14.0 E04-W00 S35-S32
20 875 501 (S38E08 L=226) 251 85 0 ( 834/ 477- 912/ 528) 33.7 E11-E05 S39-S35
|
|
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.
|
|
|
|