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| 20140331 - Filament data for 09 UTC |
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Available data for 20140331: »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
1 327 1609 (N11E70 L= 22) 1452 257 3 ( 288/1562- 354/1645) -24.4 E77-E64 N08-N13
2 1058 1452 (N18E10 L= 82) 669 211 0 (1036/1357-1079/1555) -61.7 E13-E06 N12-N25
3 1426 1464 (N31W12 L=104) 521 71 2 (1397/1423-1449/1497) -45.0 W09-W13 N28-N32
4 1230 1355 (N17W02 L= 94) 788 242 2 (1150/1241-1274/1454) -36.9 E05-W07 N11-N21
5 636 1336 (N01E31 L= 61) 230 39 1 ( 619/1312- 653/1365) -33.7 E32-E29 N00-N02
6 172 1271 (S12E69 L= 23) 789 123 1 ( 148/1234- 198/1328) 90.0 E71-E66 S14-S08
7 1775 1096 (N20W45 L=137) 503 93 0 (1740/1075-1814/1115) 33.7 W42-W48 N18-N22
8 1057 1030 (S05W02 L= 94) 320 62 0 (1032/ 992-1081/1070) 90.0 W00-W02 S08-S02
9 394 859 (S32E37 L= 55) 2763 640 8 ( 213/ 747- 546/1015) 43.8 E54-E27 S43-S19
10 1804 762 (N04W59 L=151) 1127 277 1 (1713/ 727-1878/ 817) 32.7 W51-W66 N00-N09
11 756 699 (S32E07 L= 85) 896 242 0 ( 687/ 613- 836/ 808) 72.6 E09-E04 S39-S23
12 1109 713 (S21W14 L=106) 728 207 1 ( 994/ 660-1185/ 774) 54.0 W08-W16 S26-S15
13 1372 697 (S14W30 L=122) 290 120 1 (1334/ 663-1427/ 737) -7.1 W26-W34 S15-S12
14 1762 656 (S03W61 L=153) 404 83 0 (1729/ 628-1789/ 680) 45.0 W58-W62 S05-S01
15 1315 635 (S19W29 L=121) 420 103 0 (1260/ 602-1374/ 669) 54.5 W26-W31 S22-S15
16 1134 552 (S29W22 L=114) 220 69 0 (1094/ 542-1171/ 565) 36.9 W19-W23 S30-S27
17 1639 501 (S15W58 L=150) 566 114 1 (1598/ 481-1684/ 544) 56.3 W54-W60 S17-S11
18 552 480 (S54E18 L= 74) 277 20 0 ( 533/ 464- 576/ 497) 21.8 E20-E15 S55-S52
19 1403 372 (S30W48 L=140) 1660 256 4 (1298/ 337-1500/ 415) 36.9 W41-W53 S34-S24
20 1570 348 (S25W62 L=154) 619 55 1 (1539/ 313-1606/ 374) 78.7 W59-W64 S27-S22
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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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