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| 20240628 - Latest Filament data |
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Available data for 20240628: »05 UTC »06 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
1 738 1497 (N31E23 L=355) 469 199 0 ( 665/1432- 800/1526) -22.6 E29-E17 N27-N33
2 1487 1475 (N33W33 L= 51) 416 59 1 (1464/1445-1515/1505) -45.0 W31-W35 N30-N35
3 1110 1435 (N29W04 L= 22) 398 231 1 (1062/1373-1169/1469) -50.2 W00-W08 N24-N31
4 1224 1406 (N27W12 L= 30) 227 62 2 (1206/1376-1257/1438) -90.0 W10-W14 N25-N29
5 946 1220 (N14E06 L= 12) 264 115 0 ( 896/1198-1000/1243) -15.9 E09-E02 N13-N15
6 379 1157 (N07E45 L=333) 318 64 1 ( 357/1130- 404/1184) 45.0 E46-E42 N05-N09
7 1663 1045 (N06W43 L= 61) 402 122 0 (1624/1012-1724/1066) 18.4 W39-W48 N03-N07
8 330 874 (S10E48 L=330) 1276 322 5 ( 292/ 743- 379/1015) 64.8 E53-E43 S18-S01
9 438 855 (S11E39 L=339) 242 46 2 ( 418/ 835- 458/ 877) 45.0 E40-E36 S11-S09
10 884 793 (S12E08 L= 10) 423 192 2 ( 815/ 723- 928/ 853) -48.8 E12-E04 S16-S08
11 712 757 (S15E19 L=359) 283 102 1 ( 682/ 707- 742/ 791) 78.7 E20-E16 S18-S13
12 773 728 (S17E15 L= 3) 359 63 2 ( 751/ 696- 804/ 759) 78.7 E16-E12 S19-S14
13 1869 734 (S14W72 L= 90) 707 57 1 (1837/ 716-1902/ 749) 4.4 W66-W79 S14-S12
14 699 668 (S21E20 L=358) 631 184 2 ( 638/ 597- 756/ 710) -36.9 E24-E16 S25-S18
15 289 605 (S29E59 L=319) 1117 127 2 ( 269/ 546- 315/ 675) 71.6 E64-E55 S32-S23
16 954 531 (S29E03 L= 15) 2724 616 6 ( 729/ 433-1208/ 665) 25.9 E20-W13 S38-S19
17 598 606 (S26E28 L=350) 494 126 1 ( 555/ 567- 655/ 636) 33.7 E32-E23 S29-S23
18 366 552 (S32E52 L=326) 438 83 0 ( 334/ 525- 408/ 573) 15.3 E57-E46 S34-S29
19 1396 515 (S29W30 L= 48) 576 144 0 (1332/ 488-1456/ 547) 26.6 W25-W33 S30-S26
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Download FITS filament maps as tar archive
» All Filament Data of 20240628 ...
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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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