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| 20141218 - Filament data for 09 UTC |
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Available data for 20141218: »07 UTC »08 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
1 437 1444 (N30E38 L=193) 1016 249 1 ( 355/1394- 529/1489) -17.4 E46-E30 N26-N34
2 1353 1459 (N22W26 L=257) 470 170 0 (1264/1444-1426/1480) 0.0 W19-W31 N20-N23
3 1031 1344 (N18W03 L=234) 275 70 0 ( 982/1327-1072/1362) -21.8 W00-W05 N16-N19
4 1827 1292 (N08W61 L=292) 771 129 4 (1807/1247-1848/1351) 71.6 W57-W63 N05-N11
5 303 1291 (N22E48 L=183) 340 76 0 ( 278/1264- 330/1314) -38.7 E50-E45 N19-N23
6 270 1183 (N15E51 L=181) 378 72 2 ( 249/1153- 291/1219) -90.0 E52-E48 N13-N17
7 1246 1139 (N04W14 L=245) 349 93 0 (1232/1087-1263/1192) 80.5 W13-W15 N00-N06
8 659 1123 (N08E21 L=210) 206 69 0 ( 628/1099- 698/1165) 31.0 E23-E18 N06-N09
9 306 1086 (N09E47 L=184) 668 96 1 ( 264/1038- 337/1114) -39.8 E51-E44 N05-N10
10 1564 1081 (S02W34 L=265) 643 137 2 (1510/1039-1631/1113) -26.6 W30-W39 S05-N00
11 1601 967 (S09W36 L=267) 250 92 1 (1579/ 925-1626/ 993) 45.0 W34-W38 S11-S07
12 950 952 (S05E05 L=226) 204 97 0 ( 894/ 923- 995/ 980) -33.7 E08-E02 S06-S02
13 203 933 (N01E59 L=172) 716 164 0 ( 165/ 896- 243/ 979) 16.7 E64-E54 N00-N03
14 1390 887 (S12W21 L=252) 396 86 0 (1360/ 841-1411/ 925) -68.2 W19-W22 S15-S10
15 877 864 (S09E10 L=221) 185 28 0 ( 850/ 846- 896/ 881) 0.0 E11-E08 S10-S08
16 203 728 (S11E64 L=167) 5537 678 12 ( 100/ 589- 287/ 866) -62.1 E79-E56 S19-S02
17 1268 742 (S20W13 L=244) 503 165 1 (1217/ 683-1310/ 813) 60.3 W09-W15 S23-S15
18 1359 716 (S23W19 L=250) 803 186 1 (1286/ 629-1446/ 802) 45.0 W13-W24 S27-S18
19 485 537 (S26E43 L=188) 929 179 2 ( 433/ 501- 544/ 587) -7.1 E47-E38 S27-S22
20 1393 386 (S47W24 L=255) 1592 233 6 (1269/ 351-1489/ 447) 9.0 W12-W31 S49-S42
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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.
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