SDO HMI 2014-10-02 08:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 22.12 | 0.00 | 12.66 | -5.03 | 139.30 | -27.84 | 112.10 | 0.5044 | -760.2 | -639.8 | |
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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 | 1.41 | 0.00 | 0.79 | -4.38 | 140.90 | -26.24 | 112.15 | 0.4780 | -796.0 | -669.2 | |
| 0.00 | 1.41 | 0.00 | 0.80 | -4.47 | 140.32 | -26.82 | 111.87 | 0.4867 | -963.0 | -781.7 | |
| 0.00 | 1.50 | 0.00 | 0.85 | -4.49 | 139.85 | -27.30 | 111.55 | 0.4935 | -610.0 | -564.1 | |
| 0.00 | 1.94 | 0.00 | 1.10 | -4.20 | 139.62 | -27.52 | 110.83 | 0.4950 | -900.0 | -556.4 | |
| 0.00 | 0.62 | 0.00 | 0.35 | -6.24 | 139.38 | -27.76 | 114.38 | 0.5104 | -823.0 | -657.9 | |
| 0.00 | 1.15 | 0.00 | 0.66 | -5.97 | 139.16 | -27.98 | 113.73 | 0.5118 | -809.0 | -648.8 | |
| 0.00 | 1.06 | 0.00 | 0.61 | -5.85 | 139.10 | -28.04 | 113.47 | 0.5119 | -839.0 | -700.2 | |
| 0.00 | 4.14 | 0.00 | 2.38 | -5.48 | 139.08 | -28.06 | 112.79 | 0.5099 | -870.0 | -710.6 | |
| 0.00 | 3.26 | 0.00 | 1.89 | -6.45 | 138.89 | -28.25 | 114.37 | 0.5184 | -389.0 | -570.1 | |
| 0.00 | 2.03 | 0.00 | 1.16 | -3.29 | 139.01 | -28.13 | 108.67 | 0.4989 | -794.0 | -634.6 | |
| 0.00 | 2.11 | 0.00 | 1.21 | -4.06 | 138.91 | -28.23 | 110.04 | 0.5043 | -770.0 | -635.7 | |
| 0.00 | 0.79 | 0.00 | 0.46 | -6.56 | 138.58 | -28.57 | 114.31 | 0.5233 | -643.0 | -558.2 | |
| 0.00 | 0.70 | 0.00 | 0.40 | -3.73 | 138.65 | -28.49 | 109.26 | 0.5063 | -677.0 | -597.2 | |
| 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. | |