SDO HMI 2014-10-01 10:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 13.91 | 0.00 | 9.33 | -4.68 | 138.38 | -40.87 | 104.52 | 0.6758 | -596.6 | -500.3 | |
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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 | 1.85 | 0.00 | 1.22 | -4.95 | 139.55 | -39.70 | 105.39 | 0.6623 | -750.0 | -651.1 | |
| 0.00 | 1.67 | 0.00 | 1.11 | -5.03 | 139.31 | -39.94 | 105.40 | 0.6656 | -675.0 | -505.9 | |
| 0.00 | 0.35 | 0.00 | 0.23 | -4.80 | 139.13 | -40.12 | 105.00 | 0.6671 | -674.0 | -636.2 | |
| 0.00 | 2.20 | 0.00 | 1.45 | -3.46 | 139.13 | -40.11 | 103.04 | 0.6624 | -711.0 | -532.8 | |
| 0.00 | 0.88 | 0.00 | 0.58 | -4.05 | 138.94 | -40.30 | 103.83 | 0.6668 | -672.0 | -555.6 | |
| 0.00 | 1.23 | 0.00 | 0.83 | -6.00 | 138.71 | -40.53 | 106.54 | 0.6766 | -477.0 | -460.2 | |
| 0.00 | 1.06 | 0.00 | 0.70 | -3.68 | 138.60 | -40.64 | 103.17 | 0.6698 | -599.0 | -518.2 | |
| 0.00 | 0.79 | 0.00 | 0.54 | -6.40 | 138.31 | -40.93 | 106.93 | 0.6829 | -418.0 | -362.6 | |
| 0.00 | 1.06 | 0.00 | 0.71 | -3.99 | 138.51 | -40.74 | 103.58 | 0.6721 | -602.0 | -449.4 | |
| 0.00 | 1.41 | 0.00 | 0.96 | -3.95 | 137.10 | -42.14 | 103.01 | 0.6894 | -429.0 | -394.1 | |
| 0.00 | 1.41 | 0.00 | 1.00 | -5.92 | 135.07 | -44.18 | 104.99 | 0.7199 | -556.0 | -431.1 | |
| 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. | |