SDO HMI 2014-04-06 19:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.06 | 29.21 | 0.53 | 14.50 | -8.11 | 6.70 | -0.84 | 160.57 | 0.0634 | 65.1 | -237.7 | |
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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 | 1.67 | 0.00 | 0.83 | -8.30 | 12.53 | 4.99 | 246.92 | 0.0940 | 911.0 | 723.6 | |
| 0.00 | 0.79 | 0.00 | 0.39 | -10.83 | 11.18 | 3.65 | 217.79 | 0.1025 | -711.0 | -626.6 | |
| 0.00 | 1.58 | 0.00 | 0.79 | -9.24 | 10.44 | 2.90 | 223.39 | 0.0731 | 1107.0 | 841.7 | |
| 0.62 | 1.94 | 0.31 | 0.96 | -9.69 | 10.20 | 2.66 | 217.02 | 0.0764 | 1131.0 | 847.3 | |
| 0.00 | 1.76 | 0.00 | 0.87 | -5.07 | 10.08 | 2.55 | 294.14 | 0.0488 | 899.0 | 646.2 | |
| 0.00 | 0.70 | 0.00 | 0.35 | -9.12 | 9.77 | 2.23 | 217.16 | 0.0640 | 780.0 | 728.0 | |
| 0.00 | 1.06 | 0.00 | 0.52 | -7.74 | 9.46 | 1.92 | 231.27 | 0.0429 | 843.0 | 700.7 | |
| 0.00 | 0.88 | 0.00 | 0.44 | -7.84 | 9.25 | 1.71 | 226.34 | 0.0411 | 867.0 | 643.6 | |
| 0.00 | 1.50 | 0.00 | 0.74 | -7.56 | 5.83 | -1.71 | 128.51 | 0.0379 | -991.0 | -813.6 | |
| 0.44 | 5.28 | 0.22 | 2.62 | -6.90 | 5.59 | -1.94 | 109.56 | 0.0359 | -1084.8 | -762.5 | |
| 0.00 | 6.33 | 0.00 | 3.14 | -7.53 | 5.13 | -2.40 | 118.91 | 0.0477 | -1017.0 | -902.2 | |
| 0.00 | 1.23 | 0.00 | 0.61 | -7.61 | 4.62 | -2.92 | 115.91 | 0.0563 | -774.0 | -634.9 | |
| 0.00 | 1.32 | 0.00 | 0.65 | -8.30 | 4.52 | -3.01 | 125.08 | 0.0639 | -956.0 | -762.3 | |
| 0.00 | 1.85 | 0.00 | 0.92 | -7.70 | 3.68 | -3.86 | 111.35 | 0.0719 | -912.0 | -666.2 | |
| 0.00 | 1.32 | 0.00 | 0.67 | -15.56 | 358.41 | -9.12 | 136.98 | 0.2248 | 807.0 | 599.6 | |
| 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. | |