SDO HMI 2014-04-03 22:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 12.47 | 0.00 | 8.03 | -26.52 | 80.18 | 34.72 | 233.32 | 0.6281 | -394.7 | -244.4 | |
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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 | 1.58 | 0.00 | 1.27 | -23.08 | 96.58 | 51.12 | 245.57 | 0.7888 | 253.0 | 307.5 | |
| 0.00 | 1.23 | 0.00 | 0.88 | -27.38 | 88.48 | 43.02 | 237.59 | 0.7200 | 497.0 | 447.7 | |
| 0.00 | 1.23 | 0.00 | 0.81 | -26.27 | 83.86 | 38.40 | 237.02 | 0.6663 | -103.0 | -210.8 | |
| 0.00 | 0.88 | 0.00 | 0.57 | -25.44 | 82.71 | 37.24 | 237.60 | 0.6496 | -580.0 | -517.8 | |
| 0.00 | 1.14 | 0.00 | 0.69 | -28.04 | 75.21 | 29.75 | 228.93 | 0.5832 | -726.0 | -557.5 | |
| 0.00 | 1.14 | 0.00 | 0.70 | -28.52 | 75.28 | 29.82 | 228.29 | 0.5876 | -688.0 | -584.0 | |
| 0.00 | 0.53 | 0.00 | 0.32 | -28.79 | 75.09 | 29.63 | 227.74 | 0.5876 | -656.0 | -433.0 | |
| 0.00 | 1.23 | 0.00 | 0.72 | -26.14 | 72.32 | 26.86 | 229.32 | 0.5369 | -391.0 | -424.0 | |
| 0.00 | 1.67 | 0.00 | 0.97 | -24.79 | 71.85 | 26.39 | 231.06 | 0.5208 | -535.0 | -426.2 | |
| 0.00 | 1.05 | 0.00 | 0.62 | -27.77 | 70.59 | 25.12 | 225.16 | 0.5320 | -746.0 | -549.7 | |
| 0.00 | 0.79 | 0.00 | 0.48 | -31.62 | 71.05 | 25.59 | 220.19 | 0.5722 | -667.0 | -597.8 | |
| 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. | |