SDO HMI 2014-06-30 05:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 16.44 | 44.52 | 13.48 | 37.13 | 13.00 | 278.12 | -53.09 | 75.85 | 0.8042 | -446.4 | -154.8 | |
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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 | 1.00 | 0.00 | 0.66 | 9.77 | 290.40 | -40.81 | 78.29 | 0.6601 | -568.0 | -451.1 | |
| 0.00 | 1.09 | 0.00 | 0.82 | 13.41 | 283.24 | -47.98 | 74.51 | 0.7521 | 585.0 | 466.8 | |
| 0.00 | 1.27 | 0.00 | 0.99 | 16.83 | 282.10 | -49.12 | 70.32 | 0.7708 | -348.0 | -359.6 | |
| 0.00 | 0.64 | 0.00 | 0.48 | 13.14 | 282.50 | -48.71 | 75.01 | 0.7598 | -499.0 | -454.4 | |
| 0.36 | 2.09 | 0.28 | 1.61 | 13.17 | 281.63 | -49.58 | 75.11 | 0.7693 | -606.0 | -444.5 | |
| 8.99 | 12.90 | 6.96 | 9.99 | 11.23 | 281.30 | -49.91 | 77.67 | 0.7704 | -796.9 | -505.1 | |
| 0.00 | 1.09 | 0.00 | 0.85 | 11.43 | 280.71 | -50.50 | 77.49 | 0.7769 | -432.0 | -356.2 | |
| 0.00 | 1.00 | 0.00 | 0.84 | 9.71 | 277.63 | -53.59 | 79.98 | 0.8077 | -509.0 | -441.5 | |
| 4.54 | 14.81 | 3.98 | 12.96 | 13.90 | 276.03 | -55.19 | 75.02 | 0.8271 | -491.4 | -410.3 | |
| 1.91 | -9.00 | 1.67 | -9.00 | 13.56 | 276.09 | -55.12 | 75.43 | 0.8262 | -538.1 | 999999 | |
| 0.00 | 1.82 | 0.00 | 1.62 | 14.10 | 275.45 | -55.76 | 74.86 | 0.8328 | 268.0 | 216.4 | |
| 0.00 | 1.54 | 0.00 | 1.39 | 13.45 | 274.95 | -56.26 | 75.69 | 0.8368 | 261.0 | 218.7 | |
| 0.64 | 5.27 | 0.59 | 4.92 | 14.37 | 273.67 | -57.54 | 74.75 | 0.8492 | 648.1 | 455.9 | |
| 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. | |