SDO HMI 2011-06-25 03:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.43 | 54.57 | 17.12 | 59.93 | 17.01 | 166.33 | 62.49 | 288.01 | 0.8934 | -129.2 | -163.9 | |
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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 | 1.36 | 0.00 | 1.56 | 15.92 | 167.83 | 63.99 | 286.63 | 0.9038 | -436.0 | -351.8 | |
| 0.00 | 1.27 | 0.00 | 1.42 | 14.77 | 167.12 | 63.28 | 285.43 | 0.8978 | -438.0 | -403.4 | |
| 8.17 | 10.44 | 9.36 | 11.95 | 16.59 | 167.73 | 63.88 | 287.38 | 0.9035 | -530.3 | -436.6 | |
| 0.00 | 1.63 | 0.00 | 1.84 | 16.06 | 167.34 | 63.50 | 286.83 | 0.9003 | -693.0 | -623.9 | |
| 0.00 | 1.45 | 0.00 | 1.83 | 19.97 | 169.92 | 66.07 | 290.83 | 0.9208 | 441.0 | 313.2 | |
| 0.00 | 1.09 | 0.00 | 1.21 | 16.20 | 166.92 | 63.08 | 287.03 | 0.8973 | -612.0 | -524.4 | |
| 0.00 | 4.09 | 0.00 | 4.44 | 16.16 | 166.20 | 62.36 | 287.07 | 0.8919 | -324.0 | -288.7 | |
| 1.45 | 2.45 | 1.56 | 2.64 | 15.98 | 165.89 | 62.05 | 286.90 | 0.8894 | 159.9 | 162.4 | |
| 0.00 | 1.18 | 0.00 | 1.36 | 19.24 | 167.51 | 63.67 | 290.33 | 0.9041 | -406.0 | -326.2 | |
| 0.00 | 1.91 | 0.00 | 2.03 | 16.69 | 165.47 | 61.63 | 287.75 | 0.8868 | 234.0 | 208.0 | |
| 0.00 | 1.27 | 0.00 | 1.38 | 17.85 | 165.95 | 62.11 | 288.99 | 0.8915 | 180.0 | 124.4 | |
| 4.45 | 25.06 | 4.74 | 26.94 | 17.23 | 165.51 | 61.67 | 288.35 | 0.8876 | 484.4 | -138.2 | |
| 1.36 | -12.00 | 1.46 | -12.00 | 17.48 | 165.59 | 61.75 | 288.62 | 0.8885 | 245.7 | 999999 | |
| 0.00 | 0.64 | 0.00 | 0.65 | 18.26 | 164.05 | 60.21 | 289.72 | 0.8774 | 217.0 | 184.6 | |
| 0.00 | 0.73 | 0.00 | 0.68 | 19.37 | 160.45 | 56.61 | 291.59 | 0.8492 | 263.0 | 229.9 | |
| 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. | |