SDO HMI 2014-09-27 21:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.62 | 20.47 | 0.45 | 14.44 | -14.21 | 185.49 | -40.48 | 117.82 | 0.7135 | -221.9 | -131.2 | |
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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 |
| 0.00 | 2.47 | 0.00 | 1.65 | -12.47 | 188.26 | -37.70 | 117.20 | 0.6737 | 55.0 | 115.2 | |
| 0.00 | 2.21 | 0.00 | 1.50 | -13.11 | 187.32 | -38.65 | 117.48 | 0.6879 | 625.0 | 478.4 | |
| 0.00 | 1.85 | 0.00 | 1.27 | -13.61 | 187.15 | -38.82 | 118.02 | 0.6925 | 814.0 | 610.1 | |
| 0.00 | 1.15 | 0.00 | 0.79 | -13.67 | 186.78 | -39.19 | 117.87 | 0.6969 | 587.0 | 439.4 | |
| 0.00 | 1.24 | 0.00 | 0.85 | -13.57 | 186.40 | -39.57 | 117.52 | 0.7006 | 659.0 | 485.6 | |
| 0.00 | 1.32 | 0.00 | 0.95 | -14.48 | 184.65 | -41.32 | 117.67 | 0.7242 | -618.0 | -588.5 | |
| 0.00 | 1.50 | 0.00 | 1.09 | -15.74 | 184.09 | -41.88 | 118.93 | 0.7365 | -722.0 | -538.1 | |
| 0.00 | 1.85 | 0.00 | 1.34 | -15.05 | 184.26 | -41.71 | 118.17 | 0.7312 | -728.0 | -624.9 | |
| 0.00 | 1.50 | 0.00 | 1.08 | -14.56 | 184.38 | -41.59 | 117.63 | 0.7275 | -588.0 | -520.4 | |
| 0.62 | 1.85 | 0.45 | 1.35 | -15.17 | 184.02 | -41.95 | 118.19 | 0.7342 | -677.9 | -585.1 | |
| 0.00 | 0.79 | 0.00 | 0.58 | -14.91 | 184.09 | -41.88 | 117.90 | 0.7323 | -589.0 | -553.1 | |
| 0.00 | 0.71 | 0.00 | 0.51 | -14.50 | 183.93 | -42.04 | 117.31 | 0.7319 | -617.0 | -479.4 | |
| 0.00 | 1.24 | 0.00 | 0.90 | -15.06 | 183.76 | -42.21 | 117.91 | 0.7365 | -559.0 | -397.3 | |
| 0.00 | 0.79 | 0.00 | 0.58 | -14.61 | 183.82 | -42.15 | 117.38 | 0.7335 | -542.0 | -497.7 | |
| 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. | |