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| 20230620 - Filament data for 07 UTC |
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Available data for 20230620: »06 UTC »07 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
1 368 1616 (N32E70 L=208) 1342 116 1 ( 341/1554- 394/1664) -29.7 E82-E65 N27-N35
2 544 1431 (N22E38 L=239) 460 100 1 ( 507/1400- 600/1464) 26.6 E40-E34 N19-N24
3 876 1242 (N14E11 L=266) 239 98 0 ( 830/1226- 930/1256) 8.1 E14-E07 N12-N14
4 1542 999 (N04W34 L=311) 713 161 1 (1506/ 927-1586/1071) 71.6 W31-W36 N00-N09
5 1010 992 (S00E01 L=277) 463 98 2 ( 964/ 969-1052/1035) 11.3 E03-W02 S01-N02
6 1473 953 (N01W29 L=307) 279 48 0 (1451/ 928-1494/ 974) -33.7 W27-W30 N00-N02
7 162 857 (S18E69 L=208) 2255 151 6 ( 142/ 774- 189/ 928) 59.0 E75-E63 S23-S13
8 1031 850 (S09W02 L=280) 481 141 0 ( 989/ 805-1088/ 875) 38.7 W00-W05 S12-S07
9 881 830 (S12E07 L=271) 375 80 0 ( 842/ 808- 923/ 849) -11.3 E09-E04 S12-S10
10 1142 798 (S11W09 L=287) 281 77 1 (1107/ 769-1173/ 827) -21.8 W06-W11 S12-S09
11 776 760 (S17E13 L=264) 301 77 1 ( 740/ 742- 802/ 786) 45.0 E15-E11 S18-S15
12 1691 710 (S12W51 L=329) 992 152 0 (1660/ 640-1730/ 778) 83.7 W49-W53 S16-S07
13 1066 722 (S17W05 L=283) 549 194 0 ( 989/ 699-1131/ 774) -18.4 W00-W09 S18-S14
14 310 716 (S25E52 L=226) 787 159 1 ( 253/ 690- 383/ 758) 14.0 E59-E43 S27-S21
15 1465 674 (S16W33 L=311) 772 235 0 (1407/ 632-1528/ 739) 49.4 W28-W36 S19-S11
16 1712 629 (S17W56 L=334) 1089 133 1 (1677/ 560-1753/ 666) 76.0 W53-W60 S22-S14
17 1048 599 (S25W06 L=284) 220 68 1 (1021/ 566-1062/ 621) -53.1 W03-W07 S27-S23
18 971 569 (S28W01 L=279) 216 79 0 ( 958/ 530- 982/ 608) 90.0 W00-W01 S30-S25
19 888 511 (S33E04 L=273) 285 86 0 ( 841/ 497- 928/ 527) 0.0 E07-E01 S33-S31
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Download FITS filament maps as tar archive
» All Filament Data of 20230620 ...
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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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