SDO HMI 2014-08-07 03:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9.48 | 40.58 | 11.82 | 50.10 | -20.54 | 251.30 | 61.75 | 244.31 | 0.9168 | 137.2 | 51.2 | |
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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 |
| 3.07 | 25.67 | 3.87 | 32.89 | -19.87 | 252.16 | 62.61 | 245.27 | 0.9210 | 617.5 | 143.5 | |
| 1.36 | -1.00 | 1.74 | -1.00 | -20.40 | 252.47 | 62.92 | 244.81 | 0.9239 | 464.9 | 999999 | |
| 2.89 | -1.00 | 3.73 | -1.00 | -20.61 | 252.55 | 63.00 | 244.61 | 0.9248 | 277.4 | 999999 | |
| 0.00 | 1.36 | 0.00 | 1.70 | -20.22 | 251.98 | 62.43 | 244.86 | 0.9206 | 495.0 | 464.0 | |
| 0.00 | 1.18 | 0.00 | 1.39 | -20.51 | 250.19 | 60.64 | 244.02 | 0.9099 | -28.0 | 38.2 | |
| 0.00 | 0.45 | 0.00 | 0.52 | -20.64 | 249.55 | 60.00 | 243.67 | 0.9060 | -234.0 | -186.4 | |
| 0.00 | 1.08 | 0.00 | 1.26 | -20.82 | 249.60 | 60.05 | 243.51 | 0.9067 | -193.0 | -97.7 | |
| 1.08 | 3.07 | 1.25 | 3.54 | -20.88 | 249.25 | 59.70 | 243.33 | 0.9046 | -183.3 | -65.5 | |
| 0.00 | 2.17 | 0.00 | 2.48 | -21.12 | 248.88 | 59.34 | 242.96 | 0.9027 | -229.0 | -254.4 | |
| 0.00 | 0.63 | 0.00 | 0.71 | -20.83 | 248.70 | 59.15 | 243.21 | 0.9007 | -219.0 | -166.6 | |
| 1.08 | 2.35 | 1.23 | 2.66 | -21.28 | 248.54 | 59.00 | 242.68 | 0.9008 | -460.8 | -376.1 | |
| 0.00 | 1.72 | 0.00 | 1.94 | -21.96 | 248.23 | 58.68 | 241.86 | 0.9003 | -528.0 | -399.4 | |
| 0.00 | 0.90 | 0.00 | 1.01 | -22.05 | 247.71 | 58.17 | 241.59 | 0.8971 | 217.0 | 166.6 | |
| 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. | |