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| 20140706 - Filament data for 11 UTC |
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Available data for 20140706: »04 UTC »05 UTC »06 UTC »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC »13 UTC »14 UTC »15 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 908 1436 (N29E09 L=240) 271 68 0 ( 878/1411- 945/1456) -31.0 E10-E05 N27-N30
2 632 1264 (N18E26 L=222) 966 234 4 ( 576/1207- 721/1320) -33.7 E30-E19 N14-N21
3 1160 1276 (N19W09 L=257) 293 72 0 (1128/1244-1195/1298) 26.6 W06-W10 N17-N20
4 1324 1182 (N13W19 L=267) 379 147 0 (1270/1134-1371/1244) 49.4 W15-W22 N10-N17
5 338 1187 (N12E49 L=200) 418 143 0 ( 287/1157- 375/1212) -18.4 E53-E44 N10-N13
6 1175 1165 (N12W09 L=257) 288 96 0 (1140/1131-1232/1202) -38.7 W07-W13 N10-N14
7 1812 1100 (N07W58 L=306) 531 87 1 (1792/1064-1839/1137) -45.0 W55-W61 N04-N09
8 214 970 (S02E60 L=188) 1265 220 4 ( 160/ 948- 275/ 998) 7.6 E68-E53 S03-N00
9 1219 852 (S07W12 L=260) 261 71 0 (1196/ 816-1252/ 881) 76.0 W10-W14 S09-S05
10 924 848 (S08E06 L=242) 199 16 0 ( 902/ 835- 948/ 864) 0.0 E07-E04 S08-S06
11 1302 770 (S12W18 L=266) 292 91 1 (1263/ 744-1331/ 813) -36.9 W15-W19 S13-S09
12 817 768 (S13E13 L=235) 497 149 1 ( 763/ 731- 886/ 808) 32.0 E16-E08 S15-S10
13 1605 732 (S15W40 L=288) 861 135 6 (1563/ 691-1647/ 772) -51.3 W36-W43 S17-S12
14 464 690 (S19E39 L=209) 316 71 0 ( 434/ 660- 487/ 733) -53.1 E40-E37 S20-S16
15 1211 650 (S20W13 L=261) 234 35 0 (1188/ 625-1234/ 671) 56.3 W11-W14 S21-S18
16 913 573 (S26E07 L=241) 260 74 0 ( 890/ 539- 950/ 602) 45.0 E08-E04 S28-S23
17 1472 577 (S25W32 L=280) 263 61 0 (1440/ 563-1506/ 594) 21.8 W29-W34 S26-S24
18 660 553 (S28E26 L=223) 373 94 1 ( 619/ 536- 701/ 574) 9.5 E28-E22 S28-S25
19 921 486 (S32E07 L=241) 297 43 0 ( 895/ 463- 950/ 512) -45.0 E08-E04 S33-S29
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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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