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| 20240814 - Filament data for 11 UTC |
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Available data for 20240814: »05 UTC »06 UTC »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 1300 1810 (N51W54 L=171) 1569 207 2 (1208/1765-1393/1851) -3.9 W39-W69 N48-N52
2 1544 1701 (N36W64 L=181) 437 57 0 (1522/1677-1573/1717) 0.0 W60-W68 N34-N36
3 1567 1362 (N16W43 L=160) 373 82 1 (1526/1339-1605/1387) -45.0 W40-W45 N13-N18
4 334 1321 (N35E49 L= 68) 432 111 0 ( 305/1272- 363/1366) 56.3 E51-E46 N31-N37
5 1690 1310 (N10W51 L=168) 533 133 1 (1637/1289-1756/1343) 0.0 W46-W58 N08-N11
6 941 1240 (N21E01 L=116) 227 119 0 ( 916/1187- 979/1283) 51.3 E03-W01 N17-N22
7 1041 1226 (N18W05 L=122) 400 201 0 ( 955/1198-1128/1251) -11.3 E01-W09 N16-N19
8 676 1087 (N16E21 L= 96) 563 201 1 ( 627/1012- 741/1165) -65.6 E23-E17 N10-N21
9 1803 973 (S12W53 L=170) 3930 432 13 (1736/ 794-1885/1106) 38.3 W46-W65 S21-S05
10 1740 1048 (S06W48 L=165) 336 44 1 (1721/1016-1756/1073) -90.0 W46-W49 S07-S04
11 1204 723 (S15W06 L=123) 758 254 3 (1172/ 592-1236/ 809) 69.0 W02-W08 S22-S09
12 867 659 (S13E16 L=101) 1312 386 5 ( 769/ 575- 943/ 784) -65.0 E19-E12 S18-S03
13 1117 739 (S12W01 L=118) 211 68 0 (1091/ 723-1157/ 761) -33.7 W00-W03 S13-S10
14 497 700 (S05E40 L= 78) 276 90 1 ( 469/ 662- 533/ 729) 33.7 E42-E36 S07-S03
15 390 545 (S14E54 L= 63) 1517 405 0 ( 335/ 400- 482/ 701) 87.4 E59-E49 S25-S03
16 950 522 (S23E14 L=103) 408 91 0 ( 928/ 476- 972/ 571) 56.3 E16-E11 S26-S19
17 1069 432 (S32E08 L=109) 725 118 1 (1012/ 405-1124/ 466) 7.1 E12-E04 S33-S29
18 654 405 (S27E39 L= 78) 861 101 2 ( 619/ 348- 692/ 443) 76.0 E42-E35 S31-S23
19 1331 280 (S52W09 L=126) 507 62 1 (1311/ 249-1358/ 305) 51.3 W07-W12 S55-S48
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Download FITS filament maps as tar archive
» All Filament Data of 20240814 ...
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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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