|
|
|
|
| 20141217 - Filament data for 09 UTC |
|
Available data for 20141217: »07 UTC »09 UTC »10 UTC »11 UTC »12 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 1568 1640 (N32W49 L=293) 454 87 0 (1535/1625-1605/1655) 0.0 W45-W52 N31-N33
2 1674 1577 (N27W55 L=299) 450 90 0 (1651/1555-1709/1597) -36.9 W52-W58 N25-N28
3 308 1413 (N30E49 L=195) 1085 252 3 ( 243/1371- 379/1464) -26.6 E57-E41 N26-N34
4 1152 1432 (N22W12 L=256) 381 136 0 (1071/1415-1215/1454) -6.3 W07-W16 N21-N23
5 822 1309 (N18E10 L=234) 219 58 1 ( 790/1295- 860/1325) 0.0 E11-E07 N16-N18
6 1761 1267 (N07W53 L=297) 740 196 1 (1691/1239-1804/1312) -11.3 W47-W57 N05-N09
7 1195 1283 (N13W13 L=257) 211 44 0 (1166/1267-1228/1296) 18.4 W11-W14 N11-N13
8 178 1150 (N15E60 L=184) 929 198 4 ( 137/1096- 220/1201) 31.0 E65-E55 N11-N17
9 1018 1104 (N04W00 L=244) 180 47 0 (1003/1071-1032/1133) -90.0 W00-W01 N01-N05
10 1345 1067 (S02W20 L=264) 514 126 1 (1293/1032-1414/1109) -35.5 W16-W23 S04-N01
11 150 1060 (N10E64 L=180) 1227 212 3 ( 102/1017- 191/1101) 4.4 E71-E58 N07-N11
12 1429 994 (S07W24 L=268) 193 85 1 (1404/ 962-1446/1017) 56.3 W22-W25 S08-S04
13 171 983 (N05E62 L=182) 660 95 2 ( 147/ 950- 198/1016) -45.0 E65-E59 N02-N06
14 1822 798 (S22W56 L=300) 1514 209 3 (1784/ 716-1867/ 916) 63.4 W51-W60 S26-S14
15 1177 860 (S12W08 L=252) 340 53 1 (1154/ 828-1198/ 891) 56.3 W06-W09 S14-S10
16 1140 670 (S24W04 L=248) 755 272 1 (1023/ 607-1255/ 781) 31.0 E04-W11 S27-S17
17 335 604 (S19E54 L=190) 579 124 2 ( 306/ 569- 361/ 639) -53.1 E57-E50 S21-S17
18 358 509 (S26E56 L=189) 774 183 0 ( 323/ 470- 404/ 542) 16.7 E59-E49 S28-S24
19 1322 375 (S47W17 L=261) 493 59 2 (1284/ 349-1356/ 404) 0.0 W13-W20 S48-S44
20 963 344 (S45E14 L=230) 469 84 2 ( 931/ 314- 988/ 389) 39.8 E17-E10 S47-S41
|
|
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.
|
|
|
|