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| 20140930 - Filament data for 07 UTC |
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Available data for 20140930: »05 UTC »06 UTC »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 1443 1710 (N32W53 L=247) 913 185 2 (1379/1688-1511/1728) -21.8 W47-W58 N29-N34
2 1689 1550 (N15W63 L=257) 929 183 4 (1645/1504-1724/1590) -56.3 W59-W67 N11-N17
3 1025 1432 (N29W12 L=206) 295 77 0 ( 985/1405-1061/1461) 0.0 W09-W15 N28-N30
4 1475 1411 (N15W38 L=232) 2795 699 5 (1155/1372-1713/1439) -27.8 W19-W57 N05-N24
5 716 1251 (N27E12 L=181) 554 148 1 ( 681/1182- 749/1317) -90.0 E13-E10 N22-N31
6 1861 1199 (S09W62 L=256) 2379 369 8 (1820/1098-1913/1263) 84.8 W57-W72 S15-S04
7 1128 1137 (N10W09 L=203) 391 138 2 (1112/1063-1151/1210) 54.5 W06-W11 N06-N13
8 1818 1106 (S13W54 L=248) 685 127 2 (1789/1058-1846/1156) -81.9 W50-W56 S16-S09
9 1745 1128 (S09W48 L=242) 421 100 2 (1722/1101-1771/1151) 0.0 W45-W50 S10-S06
10 1679 1059 (S10W40 L=234) 437 95 0 (1658/ 998-1695/1101) 74.1 W39-W42 S14-S07
11 1170 1013 (N02W08 L=201) 449 81 2 (1120/ 992-1218/1040) -45.0 W05-W10 N00-N04
12 321 948 (N19E47 L=146) 388 76 0 ( 309/ 904- 335/ 990) 59.0 E49-E45 N16-N21
13 1527 792 (S21W23 L=217) 1927 421 3 (1418/ 628-1575/ 941) -90.0 W19-W26 S31-S09
14 457 550 (S07E50 L=144) 576 99 3 ( 421/ 514- 509/ 589) -56.3 E52-E46 S09-S03
15 694 483 (S16E36 L=158) 700 262 1 ( 648/ 393- 738/ 576) 45.0 E42-E30 S20-S10
16 271 530 (S05E71 L=123) 762 109 0 ( 244/ 507- 305/ 562) -31.0 E74-E66 S07-S03
17 430 489 (S10E55 L=139) 331 119 0 ( 410/ 457- 462/ 542) 80.5 E56-E52 S12-S06
18 926 344 (S31E28 L=166) 1327 338 3 ( 793/ 294-1012/ 446) 13.4 E39-E18 S34-S26
19 704 224 (S34E51 L=143) 753 187 3 ( 682/ 187- 734/ 265) 33.7 E56-E47 S37-S31
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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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