SDO HMI 2011-11-28 19:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 29.05 | 152.65 | 35.97 | 182.32 | 7.74 | 129.48 | -65.30 | 82.05 | 0.9099 | -30.1 | -162.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.31 | 0.00 | 2.54 | 8.48 | 131.62 | -63.16 | 81.12 | 0.8951 | -247.0 | -252.3 | |
| 0.00 | 1.37 | 0.00 | 1.53 | 9.19 | 131.26 | -63.52 | 80.35 | 0.8981 | 412.0 | 364.7 | |
| 11.20 | 83.50 | 12.38 | 92.33 | 7.55 | 131.48 | -63.30 | 82.17 | 0.8958 | -702.9 | -288.8 | |
| 0.00 | 2.22 | 0.00 | 2.55 | 6.49 | 130.38 | -64.40 | 83.39 | 0.9038 | -588.0 | -489.7 | |
| 0.00 | 1.97 | 0.00 | 2.27 | 7.20 | 130.20 | -64.58 | 82.61 | 0.9054 | -514.0 | -394.6 | |
| 0.51 | 2.22 | 0.58 | 2.53 | 5.45 | 130.54 | -64.24 | 84.54 | 0.9025 | -454.2 | -354.0 | |
| 0.00 | 0.94 | 0.00 | 1.09 | 6.69 | 130.12 | -64.66 | 83.18 | 0.9058 | -219.0 | -188.9 | |
| 0.00 | 0.94 | 0.00 | 1.12 | 7.45 | 129.42 | -65.36 | 82.36 | 0.9111 | -217.0 | -179.6 | |
| 1.28 | 9.57 | 1.54 | 11.60 | 7.60 | 129.16 | -65.62 | 82.22 | 0.9130 | -217.3 | 63.2 | |
| 1.79 | 3.93 | 2.16 | 4.74 | 6.94 | 129.12 | -65.65 | 82.94 | 0.9131 | -280.2 | -63.0 | |
| 0.00 | 1.03 | 0.00 | 1.27 | 8.12 | 128.47 | -66.30 | 81.67 | 0.9179 | -212.0 | -61.1 | |
| 3.42 | 6.58 | 4.38 | 8.41 | 8.71 | 127.66 | -67.12 | 81.07 | 0.9235 | 521.2 | 442.9 | |
| 7.69 | 36.07 | 10.50 | 50.34 | 8.29 | 126.12 | -68.65 | 81.58 | 0.9333 | 585.6 | 14.8 | |
| 3.16 | -13.00 | 4.43 | -13.00 | 7.86 | 125.53 | -69.25 | 82.06 | 0.9369 | 398.2 | 999999 | |
| 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. | |