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| 20140705 - Filament data for 10 UTC |
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Available data for 20140705: »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 1222 1489 (N33W14 L=276) 223 56 0 (1191/1478-1254/1500) 0.0 W11-W16 N32-N34
2 425 1269 (N17E42 L=220) 952 160 3 ( 378/1218- 467/1334) 82.9 E46-E39 N13-N21
3 933 1199 (N14E06 L=256) 572 296 2 ( 881/1130-1010/1296) -51.3 E09-E01 N09-N20
4 949 1279 (N19E05 L=257) 248 47 2 ( 921/1259- 981/1295) -14.0 E07-E03 N17-N20
5 1109 1184 (N13W05 L=267) 421 175 0 (1048/1137-1162/1261) 48.8 W01-W08 N10-N18
6 1254 1154 (N11W14 L=276) 491 172 1 (1219/1092-1277/1241) -83.7 W12-W15 N07-N16
7 216 1191 (N11E62 L=200) 880 201 1 ( 167/1138- 245/1230) -35.5 E69-E57 N07-N13
8 1000 859 (S07E01 L=261) 286 107 0 ( 970/ 824-1050/ 879) 26.6 E03-W01 S09-S05
9 1080 777 (S12W04 L=266) 220 38 2 (1056/ 750-1099/ 803) -33.7 W02-W05 S13-S10
10 1407 747 (S14W25 L=287) 614 124 1 (1381/ 698-1442/ 799) 71.6 W23-W27 S16-S10
11 313 702 (S19E52 L=210) 1153 167 3 ( 261/ 628- 353/ 785) -70.0 E56-E48 S24-S13
12 1120 721 (S16W06 L=268) 217 52 0 (1093/ 692-1148/ 754) 53.1 W04-W08 S17-S13
13 1010 607 (S23E00 L=262) 567 191 2 ( 991/ 520-1029/ 673) 84.8 E01-W00 S29-S18
14 278 639 (S24E57 L=205) 561 105 0 ( 250/ 617- 307/ 670) -18.4 E60-E54 S25-S21
15 509 590 (S26E37 L=225) 480 150 1 ( 461/ 556- 545/ 634) 29.1 E41-E32 S28-S22
16 715 558 (S27E21 L=241) 422 134 0 ( 696/ 505- 746/ 608) 76.0 E22-E18 S31-S23
17 1276 558 (S26W18 L=280) 677 131 2 (1205/ 533-1330/ 591) 14.0 W13-W21 S28-S24
18 1070 489 (S32W04 L=266) 253 45 0 (1049/ 462-1088/ 515) 53.1 W02-W05 S33-S29
19 415 445 (S37E50 L=212) 799 201 3 ( 396/ 399- 438/ 490) 41.6 E55-E46 S41-S33
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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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