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| 20230218 - Filament data for 08 UTC |
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Available data for 20230218: »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
1 495 1683 (N24E55 L= 33) 1108 203 4 ( 417/1628- 580/1744) 41.6 E60-E50 N19-N29
2 813 1723 (N32E32 L= 56) 349 32 0 ( 788/1706- 838/1740) 33.7 E33-E30 N30-N33
3 959 1654 (N30E19 L= 69) 804 169 1 ( 901/1596-1020/1712) -22.6 E25-E13 N27-N33
4 550 1612 (N20E45 L= 43) 1350 309 9 ( 504/1507- 617/1700) -77.9 E52-E38 N13-N27
5 1302 1601 (N35W05 L= 93) 784 132 2 (1260/1541-1335/1650) -45.0 W02-W08 N30-N37
6 902 1528 (N21E18 L= 70) 245 111 0 ( 870/1487- 946/1569) 66.8 E19-E16 N17-N24
7 1563 1284 (N20W28 L=116) 956 293 2 (1457/1194-1650/1368) -17.4 W19-W35 N16-N22
8 1315 1173 (N08W14 L=102) 1083 419 4 (1277/1004-1366/1357) -58.6 W08-W20 S01-N17
9 220 1330 (S02E64 L= 24) 440 67 0 ( 197/1305- 249/1349) 21.8 E66-E61 S03-N00
10 1886 1224 (N26W61 L=149) 1215 110 3 (1857/1174-1916/1279) -63.4 W56-W65 N23-N29
11 1556 1194 (N14W29 L=117) 244 56 1 (1534/1177-1583/1210) 0.0 W27-W30 N13-N15
12 1598 1098 (N10W33 L=121) 347 81 1 (1568/1063-1619/1138) -31.0 W30-W35 N07-N11
13 1434 764 (S13W30 L=118) 242 116 1 (1384/ 715-1476/ 792) 63.4 W28-W32 S16-S10
14 1607 707 (S12W44 L=132) 860 161 1 (1544/ 664-1683/ 753) 36.9 W39-W49 S14-S07
15 1504 722 (S13W36 L=124) 241 52 3 (1481/ 702-1522/ 749) 90.0 W35-W38 S14-S11
16 1144 657 (S26W16 L=104) 435 129 2 (1097/ 606-1188/ 701) -18.4 W11-W20 S27-S23
17 1729 657 (S11W57 L=145) 506 55 2 (1707/ 633-1758/ 685) -21.8 W54-W59 S12-S09
18 1396 442 (S32W42 L=130) 801 195 0 (1323/ 389-1484/ 514) 70.0 W38-W44 S36-S25
19 1592 365 (S30W66 L=154) 839 137 1 (1532/ 349-1663/ 380) 13.2 W58-W75 S32-S27
20 898 167 (S69W29 L=117) 800 75 3 ( 864/ 131- 925/ 203) -16.7 W20-W41 S73-S65
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Download FITS filament maps as tar archive
» All Filament Data of 20230218 ...
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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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