SDO HMI 2014-01-12 01:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 76.90 | 468.73 | 44.97 | 274.58 | -16.35 | 13.67 | -30.39 | 114.36 | 0.5350 | 1050.3 | 351.6 | |
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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 | 1.70 | 0.00 | 0.95 | -14.12 | 17.44 | -26.62 | 112.41 | 0.4720 | 579.0 | 478.1 | |
| 45.38 | 460.07 | 26.41 | 269.25 | -16.42 | 14.25 | -29.81 | 114.80 | 0.5274 | 1335.1 | 367.9 | |
| 1.10 | -2.00 | 0.65 | -2.00 | -16.52 | 13.63 | -30.43 | 114.61 | 0.5362 | 854.1 | 999999 | |
| 2.63 | -2.00 | 1.54 | -2.00 | -16.33 | 13.52 | -30.54 | 114.22 | 0.5368 | 1029.5 | 999999 | |
| 0.85 | -2.00 | 0.50 | -2.00 | -16.15 | 13.52 | -30.54 | 113.89 | 0.5360 | 703.6 | 999999 | |
| 6.46 | -2.00 | 3.79 | -2.00 | -16.44 | 13.29 | -30.77 | 114.28 | 0.5405 | 1153.8 | 999999 | |
| 0.00 | 1.44 | 0.00 | 0.86 | -17.88 | 12.87 | -31.19 | 116.53 | 0.5530 | -183.0 | -121.5 | |
| 20.48 | -2.00 | 12.08 | -2.00 | -16.21 | 12.86 | -31.20 | 113.64 | 0.5452 | 1181.1 | 999999 | |
| 0.00 | 1.19 | 0.00 | 0.74 | -16.88 | 8.26 | -35.80 | 112.52 | 0.6083 | -752.0 | -638.8 | |
| 0.00 | 1.53 | 0.00 | 0.96 | -14.56 | 7.03 | -37.03 | 108.36 | 0.6165 | -671.0 | -653.6 | |
| 0.00 | 1.53 | 0.00 | 0.98 | -15.28 | 5.76 | -38.31 | 109.09 | 0.6351 | -777.0 | -586.3 | |
| 0.00 | 1.27 | 0.00 | 0.84 | -19.08 | 4.31 | -39.75 | 114.26 | 0.6652 | -710.0 | -558.9 | |
| 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. | |