SDO HMI 2014-03-07 23:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 36.69 | 203.26 | 50.08 | 260.04 | -13.18 | 108.96 | 68.07 | 258.73 | 0.9208 | 316.6 | 196.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.82 | 0.00 | 3.59 | -14.96 | 117.73 | 76.84 | 256.36 | 0.9692 | -24.0 | -18.4 | |
| 0.00 | 0.61 | 0.00 | 1.21 | -15.15 | 117.96 | 77.06 | 256.15 | 0.9700 | -239.0 | -232.6 | |
| 0.00 | 1.73 | 0.00 | 3.47 | -15.33 | 118.03 | 77.13 | 255.96 | 0.9703 | -350.0 | -346.3 | |
| 6.66 | 14.36 | 12.81 | 27.63 | -15.39 | 117.27 | 76.38 | 255.95 | 0.9671 | 295.8 | 188.9 | |
| 2.25 | 3.63 | 3.35 | 5.41 | -11.16 | 112.43 | 71.53 | 260.68 | 0.9445 | 322.3 | 266.1 | |
| 0.00 | 0.87 | 0.00 | 1.10 | -12.39 | 108.93 | 68.04 | 259.57 | 0.9227 | 196.0 | 189.2 | |
| 0.00 | 0.61 | 0.00 | 0.94 | -18.59 | 113.70 | 72.81 | 252.77 | 0.9494 | 59.0 | 79.4 | |
| 1.47 | 167.00 | 1.85 | 198.47 | -12.90 | 108.72 | 67.83 | 259.02 | 0.9212 | -121.8 | 252.6 | |
| 3.03 | 6.66 | 4.63 | 10.18 | -18.94 | 113.34 | 72.45 | 252.40 | 0.9475 | -215.5 | -158.1 | |
| 0.00 | 0.78 | 0.00 | 1.16 | -18.69 | 112.86 | 71.96 | 252.69 | 0.9449 | -361.0 | -318.4 | |
| 0.00 | 2.68 | 0.00 | 3.87 | -18.47 | 112.03 | 71.14 | 252.93 | 0.9404 | -466.0 | -407.8 | |
| 23.28 | -8.00 | 27.44 | -8.00 | -12.32 | 106.92 | 66.03 | 259.75 | 0.9090 | 612.2 | 999999 | |
| 0.00 | 1.21 | 0.00 | 1.44 | -14.87 | 107.33 | 66.43 | 256.93 | 0.9112 | -266.0 | -202.0 | |
| 0.00 | 1.30 | 0.00 | 1.57 | -16.07 | 107.86 | 66.97 | 255.60 | 0.9148 | -287.0 | -292.9 | |
| 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. | |