SDO HMI 2011-02-19 15:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 93.52 | 394.67 | 151.39 | 673.36 | -19.28 | 35.49 | 74.10 | 251.88 | 0.9548 | -53.0 | 66.6 | |
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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 | 1.12 | 0.00 | 2.31 | -16.58 | 38.96 | 77.57 | 254.58 | 0.9720 | 339.0 | 295.2 | |
| 6.78 | 161.85 | 14.80 | 332.30 | -18.50 | 39.88 | 78.49 | 252.56 | 0.9751 | -456.6 | -5.4 | |
| 7.12 | -2.00 | 15.10 | -2.00 | -18.61 | 39.44 | 78.05 | 252.47 | 0.9734 | 298.7 | 999999 | |
| 4.38 | -2.00 | 8.64 | -2.00 | -18.49 | 38.36 | 76.97 | 252.65 | 0.9692 | -386.3 | 999999 | |
| 9.87 | -2.00 | 19.06 | -2.00 | -18.46 | 38.04 | 76.66 | 252.69 | 0.9679 | 529.9 | 999999 | |
| 4.12 | -2.00 | 7.60 | -2.00 | -17.91 | 37.16 | 75.77 | 253.30 | 0.9642 | 422.2 | 999999 | |
| 3.00 | 180.56 | 4.91 | 265.82 | -18.62 | 35.02 | 73.64 | 252.62 | 0.9541 | 545.7 | 156.0 | |
| 0.00 | 1.89 | 0.00 | 2.91 | -19.12 | 33.95 | 72.56 | 252.12 | 0.9485 | 458.0 | 327.6 | |
| 1.97 | 23.43 | 3.14 | 37.53 | -19.69 | 34.49 | 73.10 | 251.52 | 0.9513 | -369.6 | 255.6 | |
| 0.51 | -9.00 | 0.81 | -9.00 | -19.77 | 34.27 | 72.88 | 251.43 | 0.9501 | -271.7 | 999999 | |
| 2.57 | -9.00 | 4.00 | -9.00 | -19.85 | 34.14 | 72.76 | 251.35 | 0.9495 | 276.4 | 999999 | |
| 1.03 | -7.00 | 1.50 | -7.00 | -19.66 | 32.78 | 71.40 | 251.57 | 0.9423 | 113.2 | 999999 | |
| 7.98 | -7.00 | 11.40 | -7.00 | -19.34 | 32.26 | 70.87 | 251.91 | 0.9393 | -480.3 | 999999 | |
| 0.94 | -7.00 | 1.37 | -7.00 | -19.71 | 32.64 | 71.25 | 251.52 | 0.9414 | -240.5 | 999999 | |
| 0.00 | 1.80 | 0.00 | 2.47 | -18.58 | 31.32 | 69.93 | 252.74 | 0.9339 | -419.0 | -363.8 | |
| 2.15 | -7.00 | 3.14 | -7.00 | -20.79 | 32.83 | 71.44 | 250.37 | 0.9425 | -274.8 | 999999 | |
| 3.00 | -7.00 | 4.21 | -7.00 | -19.89 | 31.85 | 70.47 | 251.33 | 0.9370 | -753.9 | 999999 | |
| 0.00 | 1.03 | 0.00 | 1.40 | -19.19 | 31.15 | 69.77 | 252.08 | 0.9329 | -474.0 | -448.0 | |
| 9.70 | -7.00 | 13.64 | -7.00 | -20.19 | 31.98 | 70.59 | 251.01 | 0.9377 | -616.8 | 999999 | |
| 0.26 | -7.00 | 0.37 | -7.00 | -20.70 | 32.52 | 71.14 | 250.47 | 0.9408 | -276.7 | 999999 | |
| 9.87 | -7.00 | 14.03 | -7.00 | -20.58 | 32.19 | 70.81 | 250.60 | 0.9389 | 606.9 | 999999 | |
| 1.63 | -7.00 | 2.25 | -7.00 | -19.84 | 31.43 | 70.04 | 251.38 | 0.9345 | -671.6 | 999999 | |
| 1.29 | -7.00 | 1.84 | -7.00 | -20.94 | 32.30 | 70.92 | 250.21 | 0.9396 | 191.2 | 999999 | |
| 2.15 | -7.00 | 3.05 | -7.00 | -21.02 | 32.19 | 70.81 | 250.13 | 0.9389 | -159.9 | 999999 | |
| 1.80 | -7.00 | 2.55 | -7.00 | -21.38 | 32.02 | 70.63 | 249.73 | 0.9380 | -404.5 | 999999 | |
| 0.00 | 1.03 | 0.00 | 1.40 | -20.62 | 31.20 | 69.81 | 250.54 | 0.9332 | 393.0 | 277.0 | |
| 1.37 | 2.83 | 1.81 | 3.74 | -20.74 | 30.41 | 69.02 | 250.40 | 0.9285 | 219.0 | 167.9 | |
| 0.00 | 1.46 | 0.00 | 1.96 | -21.84 | 30.81 | 69.43 | 249.23 | 0.9310 | -331.0 | -220.2 | |
| 1.37 | 2.23 | 1.80 | 2.93 | -22.06 | 30.23 | 68.85 | 248.98 | 0.9276 | -208.1 | -213.0 | |
| 0.00 | 1.20 | 0.00 | 1.54 | -21.71 | 29.61 | 68.23 | 249.34 | 0.9237 | -124.0 | -185.9 | |
| 4.03 | 13.90 | 4.86 | 16.63 | -20.98 | 27.99 | 66.61 | 250.10 | 0.9132 | -359.0 | -395.3 | |
| 4.63 | -31.00 | 5.51 | -31.00 | -20.73 | 27.69 | 66.30 | 250.36 | 0.9111 | -671.7 | 999999 | |
| 0.00 | 0.34 | 0.00 | 0.42 | -21.80 | 28.59 | 67.20 | 249.22 | 0.9172 | -414.0 | -451.0 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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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. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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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. |
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| 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. | |