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| 20140706 - Filament data for 10 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
1 903 1431 (N29E09 L=240) 244 62 0 ( 869/1410- 940/1451) -11.3 E11-E06 N27-N30
2 597 1273 (N18E29 L=220) 653 127 2 ( 572/1210- 642/1319) 90.0 E30-E25 N14-N21
3 1323 1207 (N15W19 L=268) 523 213 0 (1260/1134-1363/1301) 59.0 W14-W22 N10-N20
4 1155 1278 (N19W08 L=257) 290 52 0 (1118/1260-1186/1299) 11.3 W05-W10 N18-N20
5 1166 1166 (N12W09 L=258) 281 104 0 (1130/1130-1223/1205) -33.7 W06-W12 N10-N14
6 344 1184 (N12E48 L=201) 291 100 0 ( 309/1157- 371/1199) -18.4 E51-E45 N10-N12
7 1810 1096 (N07W58 L=306) 540 99 1 (1790/1053-1839/1136) -51.3 W55-W61 N04-N09
8 211 971 (S02E61 L=188) 1276 210 3 ( 157/ 951- 269/1001) 8.1 E68-E54 S03-N00
9 1211 849 (S07W12 L=261) 309 113 1 (1185/ 803-1255/ 885) -78.7 W10-W14 S10-S05
10 915 848 (S08E07 L=242) 190 20 0 ( 894/ 834- 937/ 864) -45.0 E07-E05 S08-S06
11 806 766 (S13E14 L=235) 506 146 2 ( 752/ 729- 874/ 808) 32.0 E17-E09 S15-S10
12 1296 768 (S12W18 L=266) 257 71 1 (1263/ 744-1323/ 798) -26.6 W15-W19 S13-S10
13 1600 730 (S15W40 L=289) 1066 218 6 (1557/ 680-1646/ 781) 29.7 W36-W43 S18-S12
14 457 692 (S19E39 L=209) 307 72 0 ( 431/ 662- 482/ 733) -53.1 E40-E37 S20-S16
15 1202 649 (S20W12 L=261) 229 55 0 (1176/ 623-1225/ 674) 45.0 W10-W13 S21-S18
16 907 574 (S26E08 L=241) 251 97 0 ( 883/ 534- 945/ 605) 51.3 E09-E04 S28-S23
17 654 551 (S28E26 L=223) 351 80 1 ( 619/ 532- 694/ 570) 9.5 E28-E22 S29-S26
18 912 487 (S32E08 L=241) 249 47 0 ( 893/ 463- 940/ 513) -45.0 E08-E05 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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