group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
113.30 | 560.63 | 70.79 | 349.59 | 7.33 | 228.82 | -37.55 | 85.49 | 0.6084 | -615.5 | -227.4 |
previous
or next observation for the same group /
back to the solar disc SDO HMI 2012-10-15 15:59:00 UT ![]() See sunspots with tool (Click here to study sunspot positions and configurations with tool using white-light and magnetogram images and polarity drawing) (It is recommended to set high resolution on your display!) |
spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
0.00 | 1.75 | 0.00 | 1.02 | 10.39 | 234.58 | -31.80 | 79.62 | 0.5290 | -840.0 | -573.5 | |
65.64 | 359.36 | 40.15 | 219.90 | 7.42 | 230.24 | -36.13 | 85.35 | 0.5889 | -1235.8 | -344.0 | |
0.00 | 1.31 | 0.00 | 0.83 | 6.96 | 227.63 | -38.75 | 86.10 | 0.6250 | -888.0 | -688.9 | |
1.92 | 9.86 | 1.22 | 6.26 | 7.40 | 227.47 | -38.91 | 85.39 | 0.6272 | -786.3 | -747.1 | |
18.16 | 47.83 | 11.52 | 30.35 | 5.01 | 227.52 | -38.86 | 89.23 | 0.6274 | -874.5 | -418.7 | |
0.00 | 3.40 | 0.00 | 2.16 | 6.77 | 227.37 | -39.00 | 86.41 | 0.6285 | -725.0 | -591.4 | |
0.00 | 0.52 | 0.00 | 0.33 | 7.75 | 227.27 | -39.10 | 84.84 | 0.6298 | -355.0 | -437.8 | |
0.00 | 1.48 | 0.00 | 0.95 | 10.04 | 226.90 | -39.47 | 81.22 | 0.6357 | -532.0 | -415.6 | |
0.00 | 1.48 | 0.00 | 0.95 | 7.59 | 227.13 | -39.24 | 85.09 | 0.6316 | -697.0 | -501.9 | |
0.00 | 2.79 | 0.00 | 1.78 | 7.34 | 227.00 | -39.37 | 85.49 | 0.6334 | -620.0 | -562.0 | |
0.00 | 1.13 | 0.00 | 0.73 | 6.43 | 226.86 | -39.52 | 86.92 | 0.6355 | -580.0 | -428.3 | |
0.00 | 1.83 | 0.00 | 1.18 | 9.53 | 226.50 | -39.87 | 82.05 | 0.6407 | -258.0 | -203.8 | |
1.83 | 22.78 | 1.18 | 14.65 | 8.22 | 226.59 | -39.78 | 84.11 | 0.6390 | 516.5 | 264.8 | |
0.00 | 1.57 | 0.00 | 1.01 | 8.75 | 226.53 | -39.85 | 83.27 | 0.6400 | 396.0 | 283.4 | |
0.00 | 0.61 | 0.00 | 0.39 | 5.17 | 226.84 | -39.53 | 88.90 | 0.6363 | -309.0 | -243.3 | |
5.06 | 54.82 | 3.25 | 35.50 | 7.23 | 226.62 | -39.75 | 85.66 | 0.6385 | -807.0 | 93.5 | |
0.00 | 4.63 | 0.00 | 2.99 | 8.82 | 226.12 | -40.25 | 83.19 | 0.6454 | 229.0 | 238.8 | |
0.96 | -16.00 | 0.62 | -16.00 | 7.27 | 226.27 | -40.11 | 85.60 | 0.6433 | -636.2 | 999999 | |
0.00 | 1.05 | 0.00 | 0.68 | 5.95 | 226.35 | -40.02 | 87.65 | 0.6425 | -505.0 | -372.3 | |
0.00 | 1.92 | 0.00 | 1.24 | 8.57 | 226.07 | -40.30 | 83.57 | 0.6459 | 799.0 | 707.2 | |
3.93 | 5.24 | 2.55 | 3.40 | 7.29 | 225.79 | -40.59 | 85.55 | 0.6496 | -564.4 | -497.1 | |
12.48 | -16.00 | 8.13 | -16.00 | 8.27 | 225.63 | -40.74 | 84.04 | 0.6517 | 799.9 | 999999 | |
0.00 | 1.75 | 0.00 | 1.14 | 9.65 | 225.45 | -40.93 | 81.94 | 0.6546 | 735.0 | 630.2 | |
0.00 | 1.05 | 0.00 | 0.69 | 9.28 | 225.34 | -41.04 | 82.51 | 0.6558 | 562.0 | 505.2 | |
0.00 | 1.40 | 0.00 | 0.91 | 8.74 | 225.37 | -41.00 | 83.33 | 0.6552 | 696.0 | 539.8 | |
1.05 | 2.53 | 0.68 | 1.65 | 6.89 | 225.51 | -40.86 | 86.17 | 0.6533 | -456.8 | -399.4 | |
2.27 | 16.67 | 1.49 | 10.98 | 7.16 | 225.08 | -41.29 | 85.75 | 0.6589 | -451.0 | 207.9 | |
0.00 | 1.31 | 0.00 | 0.87 | 8.68 | 224.49 | -41.89 | 83.45 | 0.6667 | 745.0 | 594.3 | |
0.00 | 2.01 | 0.00 | 1.33 | 8.47 | 224.48 | -41.90 | 83.77 | 0.6668 | 791.0 | 628.2 | |
0.00 | 4.89 | 0.00 | 3.24 | 8.14 | 224.48 | -41.90 | 84.26 | 0.6667 | 626.0 | 713.3 | |
0.00 | 1.40 | 0.00 | 0.93 | 7.09 | 224.52 | -41.85 | 85.84 | 0.6662 | 631.0 | 586.6 | |
0.00 | 1.13 | 0.00 | 0.77 | 5.39 | 222.85 | -43.53 | 88.28 | 0.6883 | 701.0 | 552.6 | |
0.00 | 1.13 | 0.00 | 0.78 | 5.84 | 222.35 | -44.03 | 87.61 | 0.6944 | 645.0 | 572.1 |
Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
||
Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
||
Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
B | - Heliographic latitude B; positive: North, negative: South | |
L | - Heliographic longitude L | |
LCM | - Longitudinal distance from the Sun's central meridian | |
Pos. angle | - Position angle | |
r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. |