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| 20141116 - Filament data for 13 UTC |
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Available data for 20141116: »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC »13 UTC »14 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 856 1452 (N31E01 L=290) 240 97 0 ( 801/1435- 903/1465) -9.5 E04-W02 N30-N32
2 1310 1270 (N10W22 L=313) 726 192 2 (1222/1242-1411/1302) -24.4 W16-W27 N06-N12
3 916 1209 (N15E02 L=288) 1270 320 2 ( 748/1170-1072/1241) -15.5 E12-W06 N10-N18
4 995 1114 (N08W00 L=291) 207 84 0 ( 964/1076-1032/1152) 36.9 E02-W03 N06-N09
5 529 1120 (N18E28 L=263) 207 87 0 ( 485/1108- 572/1141) -8.1 E31-E24 N17-N19
6 1651 1028 (S11W39 L=329) 391 56 1 (1636/ 992-1668/1069) 78.7 W37-W40 S13-S08
7 1776 997 (S16W48 L=339) 586 99 0 (1754/ 945-1796/1048) 45.0 W45-W51 S18-S13
8 154 995 (N18E63 L=228) 922 231 1 ( 103/ 959- 205/1016) -14.0 E69-E57 N15-N19
9 448 949 (N10E37 L=254) 476 132 1 ( 395/ 882- 500/1010) -66.0 E39-E34 N05-N14
10 306 851 (N07E50 L=240) 620 89 1 ( 286/ 806- 338/ 889) 59.0 E53-E47 N04-N09
11 1249 855 (S12W09 L=300) 269 58 0 (1216/ 825-1281/ 877) 11.3 W06-W11 S12-S10
12 1257 651 (S24W06 L=296) 1159 224 3 (1177/ 538-1326/ 729) 33.7 E01-W11 S29-S19
13 606 564 (S15E37 L=254) 1708 538 6 ( 490/ 409- 678/ 677) -87.0 E41-E32 S25-S06
14 436 610 (S09E47 L=243) 323 61 1 ( 413/ 582- 460/ 638) 45.0 E49-E45 S10-S07
15 336 528 (S12E60 L=230) 2917 513 7 ( 275/ 461- 406/ 600) -56.3 E66-E54 S16-S07
16 708 563 (S17E30 L=261) 375 84 2 ( 678/ 522- 733/ 598) 78.7 E31-E27 S20-S15
17 1108 342 (S42E13 L=278) 498 98 1 (1085/ 299-1129/ 380) 74.1 E14-E10 S45-S38
18 799 259 (S40E39 L=251) 346 69 0 ( 781/ 232- 819/ 285) 76.0 E41-E37 S42-S37
19 1023 208 (S51E28 L=263) 844 145 2 ( 990/ 167-1062/ 248) 22.6 E33-E21 S54-S47
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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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