|
|
|
|
| 20230215 - Filament data for 13 UTC |
|
Available data for 20230215: »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC »13 UTC »14 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 821 1725 (N33E31 L= 94) 863 160 2 ( 790/1651- 851/1789) -39.3 E36-E25 N28-N38
2 511 1744 (N30E59 L= 66) 1177 140 1 ( 469/1691- 555/1788) -16.3 E73-E49 N26-N33
3 1236 1615 (N34W01 L=126) 292 72 1 (1211/1593-1269/1642) -18.4 W00-W03 N32-N36
4 688 1602 (N22E34 L= 91) 295 108 1 ( 645/1569- 739/1639) 51.3 E36-E31 N19-N25
5 406 1572 (N16E56 L= 69) 598 114 1 ( 378/1542- 443/1615) -18.4 E59-E50 N14-N19
6 980 1485 (N20E12 L=113) 1348 446 7 ( 853/1346-1115/1608) -28.6 E22-W00 N13-N25
7 726 1385 (N09E25 L=100) 1363 283 3 ( 700/1219- 758/1579) -70.0 E30-E20 S01-N21
8 1498 1419 (N27W22 L=147) 498 125 0 (1478/1378-1522/1480) 82.9 W20-W24 N23-N31
9 1627 1402 (N29W33 L=158) 675 206 0 (1557/1315-1673/1472) -38.7 W26-W37 N24-N32
10 1121 1397 (N17E02 L=123) 307 56 1 (1089/1378-1155/1417) 33.7 E03-W00 N15-N17
11 1043 910 (S13W03 L=128) 637 197 1 ( 983/ 884-1143/ 949) 32.0 W00-W08 S15-S10
12 617 827 (S26E22 L=103) 301 85 1 ( 568/ 800- 651/ 851) -9.5 E25-E19 S26-S24
13 568 690 (S35E25 L=100) 336 79 1 ( 539/ 667- 607/ 718) -9.5 E27-E21 S36-S33
14 1418 501 (S28W40 L=165) 913 190 3 (1338/ 441-1484/ 572) -10.6 W31-W47 S30-S25
15 1245 523 (S31W27 L=152) 375 95 0 (1197/ 508-1296/ 537) 15.9 W23-W30 S32-S29
16 733 486 (S46E09 L=116) 808 144 3 ( 674/ 460- 819/ 518) 18.4 E14-E02 S48-S43
17 1419 370 (S36W48 L=173) 604 82 1 (1384/ 341-1464/ 399) 68.2 W45-W50 S38-S33
18 744 234 (S68E03 L=122) 916 147 0 ( 683/ 205- 813/ 264) -2.6 E13-W09 S70-S65
|
Download FITS filament maps as tar archive
» All Filament Data of 20230215 ...
|
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.
|
|
|
|