SDO HMI 2014-06-30 08:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 21.45 | 50.87 | 17.17 | 41.10 | 13.05 | 277.92 | -51.65 | 75.60 | 0.7898 | -429.7 | -160.9 | |
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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 | 1.00 | 14.66 | 283.11 | -46.46 | 72.55 | 0.7374 | -521.0 | -382.5 | |
| 0.00 | 1.27 | 0.00 | 0.92 | 13.42 | 283.30 | -46.27 | 74.18 | 0.7329 | 481.0 | 311.4 | |
| 0.00 | 1.36 | 0.00 | 1.00 | 13.18 | 282.49 | -47.08 | 74.67 | 0.7417 | -631.0 | -490.7 | |
| 0.00 | 2.45 | 0.00 | 1.83 | 13.24 | 281.73 | -47.85 | 74.72 | 0.7503 | -612.0 | -515.0 | |
| 10.27 | 13.08 | 7.70 | 9.81 | 11.21 | 281.28 | -48.29 | 77.49 | 0.7524 | -795.5 | -518.2 | |
| 0.00 | 1.27 | 0.00 | 0.97 | 11.43 | 280.61 | -48.96 | 77.29 | 0.7601 | -464.0 | -374.6 | |
| 0.00 | 0.82 | 0.00 | 0.62 | 11.86 | 280.42 | -49.16 | 76.76 | 0.7628 | -344.0 | -304.3 | |
| 0.00 | 0.82 | 0.00 | 0.66 | 14.04 | 277.78 | -51.79 | 74.38 | 0.7937 | -339.0 | -300.8 | |
| 0.00 | 1.18 | 0.00 | 0.95 | 9.63 | 277.69 | -51.88 | 79.94 | 0.7900 | -476.0 | -335.4 | |
| 9.36 | 18.26 | 7.84 | 15.30 | 13.70 | 276.28 | -53.29 | 75.02 | 0.8084 | -616.0 | -405.5 | |
| 0.00 | 1.18 | 0.00 | 1.03 | 14.52 | 274.70 | -54.87 | 74.24 | 0.8248 | 563.0 | 474.8 | |
| 0.00 | 0.64 | 0.00 | 0.56 | 13.54 | 274.39 | -55.18 | 75.47 | 0.8266 | 562.0 | 518.6 | |
| 1.82 | 7.18 | 1.63 | 6.45 | 14.44 | 273.56 | -56.01 | 74.49 | 0.8354 | 651.0 | 434.1 | |
| 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. | |