SDO HMI 2014-03-28 11:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.89 | 28.80 | 1.54 | 15.35 | -23.52 | 116.52 | -14.15 | 142.61 | 0.3703 | 36.3 | -56.1 | |
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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 | 2.54 | 0.00 | 1.33 | -21.72 | 118.81 | -11.86 | 143.84 | 0.3249 | 699.0 | 446.1 | |
| 0.00 | 0.96 | 0.00 | 0.52 | -25.94 | 118.24 | -12.43 | 149.73 | 0.3857 | 707.0 | 585.9 | |
| 0.00 | 2.28 | 0.00 | 1.20 | -23.33 | 118.47 | -12.20 | 146.06 | 0.3491 | 831.0 | 660.3 | |
| 0.00 | 1.23 | 0.00 | 0.65 | -23.94 | 117.78 | -12.90 | 145.68 | 0.3633 | 899.0 | 778.6 | |
| 1.14 | 9.28 | 0.61 | 4.94 | -23.86 | 117.14 | -13.53 | 144.30 | 0.3682 | -776.5 | 107.3 | |
| 1.75 | -5.00 | 0.93 | -5.00 | -23.70 | 116.93 | -13.74 | 143.60 | 0.3682 | 730.3 | 999999 | |
| 0.00 | 0.70 | 0.00 | 0.37 | -21.99 | 117.07 | -13.60 | 140.70 | 0.3457 | -757.0 | -540.5 | |
| 0.00 | 1.66 | 0.00 | 0.88 | -22.90 | 116.21 | -14.46 | 140.79 | 0.3655 | -740.0 | -635.3 | |
| 0.00 | 2.45 | 0.00 | 1.30 | -22.65 | 116.20 | -14.47 | 140.31 | 0.3626 | -948.0 | -704.1 | |
| 0.00 | 0.96 | 0.00 | 0.51 | -23.17 | 115.77 | -14.90 | 140.50 | 0.3732 | -151.0 | -109.5 | |
| 0.00 | 1.31 | 0.00 | 0.71 | -24.55 | 114.99 | -15.68 | 141.61 | 0.3975 | 817.0 | 582.3 | |
| 0.00 | 1.40 | 0.00 | 0.76 | -24.12 | 114.23 | -16.44 | 139.59 | 0.4002 | -226.0 | -339.2 | |
| 0.00 | 4.03 | 0.00 | 2.18 | -24.04 | 113.83 | -16.84 | 138.81 | 0.4035 | -881.0 | -806.8 | |
| 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. | |