SDO HMI 2011-05-30 15:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 32.22 | 164.01 | 33.92 | 176.11 | -19.89 | 20.49 | -60.89 | 112.06 | 0.8882 | 160.0 | 79.7 | |
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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 | 0.99 | 0.00 | 0.95 | -18.99 | 24.29 | -57.09 | 111.79 | 0.8569 | -376.0 | -325.4 | |
| 4.96 | 13.90 | 4.78 | 13.40 | -17.57 | 23.71 | -57.67 | 110.05 | 0.8595 | -676.9 | -425.7 | |
| 0.00 | 1.26 | 0.00 | 1.27 | -19.64 | 22.45 | -58.92 | 112.16 | 0.8730 | -266.0 | -322.4 | |
| 0.63 | -2.00 | 0.61 | -2.00 | -17.54 | 23.43 | -57.95 | 109.96 | 0.8618 | -320.6 | 999999 | |
| 0.00 | 1.26 | 0.00 | 1.27 | -18.94 | 22.49 | -58.89 | 111.37 | 0.8716 | -629.0 | -449.8 | |
| 4.33 | 12.73 | 4.41 | 12.97 | -18.29 | 21.91 | -59.47 | 110.53 | 0.8753 | -582.0 | -399.2 | |
| 0.00 | 1.90 | 0.00 | 1.90 | -17.65 | 22.26 | -59.12 | 109.88 | 0.8716 | -372.0 | -330.9 | |
| 0.00 | 0.72 | 0.00 | 0.73 | -17.81 | 21.99 | -59.39 | 110.01 | 0.8740 | -449.0 | -364.9 | |
| 2.53 | -6.00 | 2.58 | -6.00 | -18.03 | 21.80 | -59.58 | 110.22 | 0.8758 | -394.8 | 999999 | |
| 19.77 | 127.19 | 21.54 | 139.11 | -20.32 | 19.99 | -61.39 | 112.46 | 0.8927 | 743.5 | 166.2 | |
| 0.00 | 1.90 | 0.00 | 1.98 | -18.53 | 21.13 | -60.25 | 110.67 | 0.8817 | 422.0 | 232.6 | |
| 0.00 | 1.26 | 0.00 | 1.46 | -22.30 | 18.52 | -62.86 | 114.36 | 0.9056 | -281.0 | -215.1 | |
| 0.00 | 0.90 | 0.00 | 1.07 | -19.74 | 17.49 | -63.89 | 111.41 | 0.9096 | -340.0 | -340.9 | |
| 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. | |