SDO HMI 2014-03-06 20:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.11 | 17.30 | 2.35 | 13.37 | 17.30 | 99.94 | 44.22 | 299.84 | 0.7698 | 291.4 | 269.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.78 | 0.00 | 0.66 | 15.85 | 105.19 | 49.47 | 295.57 | 0.8127 | -453.0 | -350.0 | |
| 0.00 | 0.78 | 0.00 | 0.65 | 15.54 | 104.99 | 49.27 | 295.30 | 0.8098 | -566.0 | -515.4 | |
| 0.00 | 1.04 | 0.00 | 0.84 | 17.56 | 102.32 | 46.59 | 298.88 | 0.7933 | -614.0 | -547.9 | |
| 0.00 | 0.26 | 0.00 | 0.20 | 15.80 | 100.34 | 44.62 | 297.81 | 0.7665 | 177.0 | 205.7 | |
| 0.00 | 1.47 | 0.00 | 1.12 | 15.36 | 100.14 | 44.41 | 297.40 | 0.7624 | 463.0 | 405.5 | |
| 0.00 | 0.95 | 0.00 | 0.73 | 16.38 | 100.03 | 44.31 | 298.67 | 0.7661 | 383.0 | 324.1 | |
| 2.16 | 3.63 | 1.63 | 2.74 | 16.39 | 99.08 | 43.36 | 299.19 | 0.7568 | 666.5 | 473.1 | |
| 0.00 | 1.38 | 0.00 | 1.06 | 17.85 | 99.17 | 43.45 | 300.87 | 0.7650 | 623.0 | 463.0 | |
| 0.95 | 1.99 | 0.72 | 1.50 | 16.98 | 98.87 | 43.15 | 300.01 | 0.7577 | 648.4 | 490.3 | |
| 0.00 | 1.82 | 0.00 | 1.39 | 18.14 | 99.13 | 43.41 | 301.23 | 0.7661 | 674.0 | 530.7 | |
| 0.00 | 1.30 | 0.00 | 1.01 | 18.95 | 99.35 | 43.63 | 302.05 | 0.7722 | 501.0 | 416.0 | |
| 0.00 | 0.78 | 0.00 | 0.61 | 19.58 | 99.39 | 43.66 | 302.75 | 0.7758 | 582.0 | 481.8 | |
| 0.00 | 1.12 | 0.00 | 0.86 | 21.08 | 97.31 | 41.59 | 305.69 | 0.7649 | 567.0 | 483.8 | |
| 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. | |