| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 51.05 | 216.64 | 36.43 | 154.79 | -20.17 | 258.28 | -37.77 | 127.11 | 0.7233 | 200.5 | -156.2 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-08-31 06:59:08 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 | 0.45 | 0.00 | 0.31 | -22.03 | 262.48 | -33.57 | 132.44 | 0.6969 | 625.0 | 558.6 | |
| 0.00 | 0.54 | 0.00 | 0.37 | -21.87 | 262.36 | -33.69 | 132.16 | 0.6967 | 653.0 | 511.7 | |
| 0.00 | 3.40 | 0.00 | 2.32 | -20.75 | 262.31 | -33.74 | 130.81 | 0.6887 | 772.0 | 592.6 | |
| 0.00 | 0.54 | 0.00 | 0.38 | -23.04 | 261.48 | -34.57 | 132.77 | 0.7136 | -359.0 | -312.7 | |
| 0.00 | 1.08 | 0.00 | 0.75 | -21.71 | 261.70 | -34.35 | 131.44 | 0.7017 | 604.0 | 418.2 | |
| 1.43 | 15.23 | 1.00 | 10.64 | -20.47 | 260.13 | -35.92 | 128.79 | 0.7075 | 948.3 | 674.0 | |
| 3.85 | -6.00 | 2.70 | -6.00 | -20.29 | 259.86 | -36.19 | 128.37 | 0.7088 | 852.6 | 999999 | |
| 0.00 | 1.25 | 0.00 | 0.90 | -22.25 | 259.21 | -36.85 | 130.15 | 0.7284 | 619.0 | 541.8 | |
| 14.87 | 24.82 | 10.52 | 17.55 | -20.80 | 259.43 | -36.62 | 128.65 | 0.7163 | 793.7 | 483.2 | |
| 0.00 | 0.99 | 0.00 | 0.72 | -22.64 | 258.63 | -37.42 | 130.18 | 0.7363 | 580.0 | 444.5 | |
| 0.00 | 0.72 | 0.00 | 0.51 | -21.14 | 258.97 | -37.08 | 128.71 | 0.7231 | 432.0 | 349.5 | |
| 0.00 | 0.72 | 0.00 | 0.50 | -18.65 | 259.33 | -36.72 | 126.03 | 0.7029 | 333.0 | 227.0 | |
| 0.81 | 2.06 | 0.57 | 1.45 | -19.62 | 258.91 | -37.14 | 126.90 | 0.7135 | 554.2 | 521.9 | |
| 1.16 | 101.15 | 0.83 | 72.29 | -20.08 | 258.62 | -37.43 | 127.24 | 0.7193 | 626.2 | -190.8 | |
| 4.03 | -14.00 | 2.90 | -14.00 | -20.95 | 258.33 | -37.72 | 128.04 | 0.7278 | 560.0 | 999999 | |
| 14.42 | -14.00 | 10.31 | -14.00 | -20.44 | 258.44 | -37.61 | 127.52 | 0.7234 | 743.8 | 999999 | |
| 0.00 | 2.15 | 0.00 | 1.51 | -19.20 | 258.66 | -37.39 | 126.22 | 0.7132 | 670.0 | 507.5 | |
| 0.00 | 0.99 | 0.00 | 0.68 | -17.68 | 259.01 | -37.04 | 124.62 | 0.6998 | -739.0 | -636.1 | |
| 0.00 | 2.42 | 0.00 | 1.74 | -19.56 | 257.58 | -38.47 | 125.90 | 0.7260 | -285.0 | -248.2 | |
| 0.00 | 1.97 | 0.00 | 1.41 | -19.32 | 257.65 | -38.40 | 125.66 | 0.7238 | -265.0 | -252.7 | |
| 0.00 | 1.97 | 0.00 | 1.44 | -20.51 | 257.14 | -38.91 | 126.71 | 0.7362 | -797.0 | -604.1 | |
| 0.00 | 1.88 | 0.00 | 1.33 | -18.07 | 257.78 | -38.27 | 124.26 | 0.7147 | -817.0 | -711.0 | |
| 3.40 | 7.35 | 2.43 | 5.26 | -19.00 | 257.49 | -38.56 | 125.17 | 0.7233 | -653.9 | -421.0 | |
| 0.00 | 2.69 | 0.00 | 1.91 | -18.35 | 257.63 | -38.42 | 124.49 | 0.7180 | -711.0 | -736.1 | |
| 0.00 | 1.34 | 0.00 | 0.98 | -20.29 | 256.91 | -39.14 | 126.30 | 0.7369 | -275.0 | -251.7 | |
| 0.00 | 3.49 | 0.00 | 2.51 | -18.90 | 257.03 | -39.03 | 124.75 | 0.7273 | -859.0 | -633.3 | |
| 4.12 | 13.08 | 3.03 | 9.58 | -20.03 | 256.36 | -39.69 | 125.64 | 0.7406 | -809.7 | -580.8 | |
| 2.96 | 15.05 | 2.14 | 10.94 | -18.88 | 256.49 | -39.56 | 124.37 | 0.7324 | -882.2 | -605.5 | |
| 0.00 | 1.25 | 0.00 | 0.89 | -17.33 | 256.79 | -39.26 | 122.70 | 0.7202 | -237.0 | -318.7 | |
| 0.00 | 2.42 | 0.00 | 1.80 | -20.03 | 255.65 | -40.41 | 125.17 | 0.7473 | -526.0 | -472.5 | |
| 0.00 | 1.25 | 0.00 | 0.90 | -17.37 | 256.32 | -39.73 | 122.45 | 0.7252 | -621.0 | -495.9 | |
| 0.00 | 1.34 | 0.00 | 0.99 | -19.59 | 255.61 | -40.44 | 124.64 | 0.7451 | -497.0 | -362.6 | |
| 0.00 | 1.79 | 0.00 | 1.32 | -18.95 | 255.63 | -40.42 | 123.91 | 0.7412 | -658.0 | -550.2 | |
| 0.00 | 0.27 | 0.00 | 0.20 | -19.68 | 255.33 | -40.72 | 124.57 | 0.7483 | -569.0 | -534.7 | |
| 0.00 | 0.99 | 0.00 | 0.71 | -17.41 | 255.81 | -40.24 | 122.18 | 0.7305 | -551.0 | -484.7 | |
| 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. | |