SDO HMI 2014-03-06 04:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 32.36 | 133.06 | 36.23 | 151.84 | -9.91 | 359.45 | -65.05 | 97.54 | 0.9026 | 557.9 | 192.7 | |
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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 |
| 10.47 | 104.76 | 11.72 | 116.84 | -10.42 | 359.95 | -64.55 | 98.08 | 0.8989 | 867.6 | 336.4 | |
| 18.51 | -1.00 | 20.59 | -1.00 | -9.57 | 0.19 | -64.31 | 97.12 | 0.8974 | 725.7 | 999999 | |
| 1.82 | -1.00 | 2.04 | -1.00 | -10.09 | 359.93 | -64.57 | 97.71 | 0.8991 | 631.5 | 999999 | |
| 0.00 | 3.72 | 0.00 | 4.18 | -8.20 | 0.02 | -64.49 | 95.60 | 0.8994 | -459.0 | -395.9 | |
| 0.00 | 1.04 | 0.00 | 1.19 | -9.90 | 359.36 | -65.14 | 97.54 | 0.9035 | 162.0 | 130.0 | |
| 1.56 | 2.51 | 1.88 | 3.03 | -10.79 | 357.87 | -66.64 | 98.60 | 0.9138 | 202.2 | 165.5 | |
| 0.00 | 0.69 | 0.00 | 0.84 | -9.61 | 357.90 | -66.60 | 97.32 | 0.9140 | 312.0 | 251.1 | |
| 0.00 | 4.33 | 0.00 | 5.35 | -9.94 | 357.30 | -67.20 | 97.71 | 0.9180 | -279.0 | -222.6 | |
| 0.00 | 2.60 | 0.00 | 3.19 | -8.85 | 357.58 | -66.93 | 96.51 | 0.9167 | 363.0 | 302.1 | |
| 0.00 | 7.09 | 0.00 | 8.89 | -10.26 | 356.92 | -67.58 | 98.08 | 0.9205 | -484.0 | -332.3 | |
| 0.00 | 1.82 | 0.00 | 2.25 | -8.77 | 357.37 | -67.13 | 96.43 | 0.9181 | 281.0 | 281.2 | |
| 0.00 | 0.78 | 0.00 | 0.98 | -9.39 | 356.81 | -67.69 | 97.16 | 0.9216 | -120.0 | -132.0 | |
| 0.00 | 1.99 | 0.00 | 2.59 | -9.55 | 356.09 | -68.41 | 97.38 | 0.9263 | -378.0 | -332.9 | |
| 0.00 | 1.73 | 0.00 | 2.51 | -14.23 | 353.37 | -71.13 | 102.55 | 0.9412 | -383.0 | -330.9 | |
| 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. | |