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| 20150422 - Filament data for 09 UTC |
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Available data for 20150422: »06 UTC »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC »13 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 1212 1626 (N36E07 L= 17) 2100 548 3 (1135/1448-1294/1802) -42.5 E21-W03 N26-N48
2 407 1682 (N18E67 L=317) 3143 215 2 ( 357/1634- 463/1733) 77.5 E70-E63 N14-N23
3 618 1555 (N15E41 L=343) 897 383 2 ( 568/1429- 689/1674) -37.4 E47-E30 N09-N22
4 441 1501 (N08E51 L=332) 857 223 3 ( 369/1447- 480/1567) 63.4 E55-E48 N03-N12
5 358 1513 (N07E60 L=324) 732 118 1 ( 310/1457- 395/1550) 66.8 E62-E57 N02-N09
6 1794 1401 (N43W46 L= 70) 490 95 1 (1772/1377-1821/1421) 35.5 W43-W50 N39-N44
7 1658 1266 (N27W33 L= 57) 770 208 1 (1600/1167-1688/1364) -51.3 W27-W36 N21-N31
8 1199 1178 (N08W06 L= 29) 207 41 0 (1184/1147-1219/1204) 90.0 W04-W06 N06-N09
9 752 1055 (S10E16 L= 8) 227 87 0 ( 707/1020- 792/1088) 63.4 E18-E14 S13-S07
10 1832 910 (N13W57 L= 81) 2635 433 5 (1789/ 769-1881/1055) -41.2 W49-W68 N06-N20
11 1435 964 (N03W25 L= 49) 282 146 0 (1369/ 942-1478/ 986) 45.0 W21-W27 N00-N05
12 1511 945 (N04W30 L= 54) 219 16 0 (1492/ 925-1529/ 966) 71.6 W29-W31 N02-N05
13 1257 791 (S11W20 L= 43) 470 184 0 (1188/ 729-1351/ 822) 52.1 W17-W24 S16-S07
14 180 800 (S40E58 L=326) 801 195 2 ( 136/ 786- 215/ 821) 16.7 E63-E53 S40-S37
15 977 809 (S18W03 L= 27) 228 102 0 ( 918/ 798-1027/ 817) 31.0 W00-W06 S19-S16
16 1003 663 (S26W09 L= 33) 642 169 1 ( 910/ 643-1087/ 687) 35.0 W03-W13 S28-S21
17 1173 513 (S29W25 L= 49) 311 53 1 (1140/ 495-1208/ 536) 9.5 W22-W28 S30-S28
18 901 473 (S41W10 L= 34) 235 24 1 ( 887/ 450- 918/ 494) -56.3 W08-W11 S42-S39
19 991 467 (S38W17 L= 40) 288 59 1 ( 952/ 452-1028/ 481) 31.0 W13-W18 S39-S36
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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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