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| 20140512 - Filament data for 05 UTC |
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Available data for 20140512: »04 UTC »05 UTC »06 UTC »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 757 1531 (N21E30 L=230) 629 172 0 ( 739/1461- 778/1612) -60.9 E33-E27 N16-N25
2 1212 1574 (N35E02 L=257) 242 34 1 (1189/1554-1234/1596) -14.0 E04-W00 N34-N36
3 1064 1482 (N25E09 L=250) 440 86 0 (1028/1445-1102/1522) -23.2 E12-E05 N23-N26
4 545 1475 (N12E42 L=217) 440 80 1 ( 520/1444- 566/1513) -45.0 E44-E39 N10-N14
5 625 1378 (N08E33 L=227) 371 63 0 ( 609/1338- 647/1408) -76.0 E34-E31 N06-N10
6 205 1168 (S12E62 L=197) 1090 114 1 ( 174/1115- 235/1228) 74.1 E65-E59 S15-S08
7 1310 1187 (N13W13 L=272) 250 79 0 (1267/1172-1351/1202) 31.0 W10-W15 N11-N14
8 1054 1132 (N04E01 L=259) 383 155 1 ( 990/1102-1101/1163) 51.3 E03-W01 N00-N06
9 550 1042 (S13E29 L=230) 419 114 2 ( 496/1009- 603/1072) 23.2 E32-E25 S14-S09
10 172 978 (S24E61 L=198) 1480 235 2 ( 141/ 915- 192/1042) -69.4 E64-E58 S28-S20
11 1112 950 (S05W07 L=266) 198 44 1 (1086/ 934-1143/ 968) 18.4 W05-W08 S05-S04
12 1176 761 (S14W15 L=275) 402 73 2 (1140/ 739-1209/ 789) -11.3 W12-W17 S16-S12
13 1382 719 (S12W29 L=288) 215 70 0 (1356/ 691-1398/ 754) 90.0 W28-W29 S13-S09
14 536 702 (S34E25 L=234) 647 132 1 ( 508/ 643- 574/ 745) 69.4 E27-E22 S38-S30
15 324 701 (S39E44 L=215) 705 148 0 ( 293/ 658- 363/ 741) 45.0 E47-E40 S42-S35
16 335 597 (S47E45 L=215) 706 84 0 ( 307/ 556- 368/ 643) -56.3 E47-E41 S49-S43
17 1089 551 (S29W17 L=276) 401 75 1 (1041/ 533-1131/ 574) 18.4 W13-W19 S31-S27
18 1619 480 (S19W57 L=316) 413 43 0 (1590/ 465-1645/ 498) 31.0 W54-W59 S20-S17
19 855 458 (S42W05 L=264) 288 44 1 ( 832/ 440- 882/ 484) 33.7 W03-W06 S43-S39
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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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