SDO HMI 2014-01-15 12:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 75.43 | 422.31 | 39.30 | 220.15 | -16.32 | 12.59 | 14.04 | 228.42 | 0.3123 | 987.6 | 399.2 | |
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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 | 0.68 | 0.00 | 0.37 | -17.23 | 18.15 | 19.60 | 235.11 | 0.3922 | 860.0 | 680.5 | |
| 0.00 | 1.11 | 0.00 | 0.60 | -17.75 | 18.11 | 19.55 | 233.94 | 0.3961 | 679.0 | 493.1 | |
| 0.43 | 1.28 | 0.23 | 0.68 | -16.23 | 17.26 | 18.71 | 236.24 | 0.3721 | -744.2 | -645.3 | |
| 38.09 | 261.31 | 19.93 | 136.75 | -16.55 | 13.37 | 14.82 | 229.43 | 0.3242 | 1365.8 | 405.3 | |
| 0.00 | 0.94 | 0.00 | 0.49 | -18.58 | 13.54 | 14.99 | 225.09 | 0.3477 | 770.0 | 600.8 | |
| 4.00 | -4.00 | 2.09 | -4.00 | -16.71 | 12.72 | 14.16 | 227.81 | 0.3178 | 1187.0 | 999999 | |
| 0.00 | 1.02 | 0.00 | 0.53 | -15.10 | 11.94 | 13.39 | 230.45 | 0.2913 | 939.0 | 764.7 | |
| 32.91 | 147.62 | 17.05 | 76.50 | -15.92 | 11.59 | 13.03 | 227.53 | 0.2954 | 1350.9 | 452.6 | |
| 0.00 | 0.60 | 0.00 | 0.31 | -18.73 | 11.60 | 13.04 | 220.94 | 0.3277 | 624.0 | 415.3 | |
| 0.00 | 0.85 | 0.00 | 0.43 | -15.85 | 7.43 | 8.88 | 217.09 | 0.2473 | -830.0 | -643.3 | |
| 0.00 | 1.96 | 0.00 | 1.00 | -16.28 | 7.04 | 8.49 | 214.85 | 0.2492 | -869.0 | -578.3 | |
| 0.00 | 1.02 | 0.00 | 0.51 | -10.01 | 4.48 | 5.93 | 226.98 | 0.1398 | -918.0 | -691.0 | |
| 0.00 | 1.53 | 0.00 | 0.76 | -9.71 | 4.27 | 5.71 | 227.54 | 0.1337 | -918.0 | -644.6 | |
| 0.00 | 0.60 | 0.00 | 0.31 | -19.12 | 4.35 | 5.79 | 200.78 | 0.2701 | -690.0 | -423.0 | |
| 0.00 | 1.79 | 0.00 | 0.91 | -18.18 | 2.98 | 4.42 | 197.29 | 0.2477 | -802.0 | -499.5 | |
| 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. | |