SDO HMI 2014-03-05 19:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.61 | 64.72 | 6.95 | 35.72 | -17.06 | 44.59 | -24.86 | 114.39 | 0.4428 | 144.2 | -108.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.32 | 13.31 | 2.35 | 7.22 | -17.09 | 46.83 | -22.62 | 116.12 | 0.4112 | 916.6 | 911.5 | |
| 0.00 | 2.07 | 0.00 | 1.13 | -16.73 | 46.74 | -22.71 | 115.21 | 0.4104 | 872.0 | 885.7 | |
| 1.38 | 4.58 | 0.75 | 2.49 | -16.33 | 46.62 | -22.83 | 114.20 | 0.4099 | 1050.0 | 740.2 | |
| 0.00 | 2.85 | 0.00 | 1.55 | -17.02 | 46.50 | -22.95 | 115.68 | 0.4154 | 695.0 | 589.1 | |
| 0.00 | 1.21 | 0.00 | 0.66 | -16.69 | 46.54 | -22.90 | 114.96 | 0.4130 | 678.0 | 565.1 | |
| 0.00 | 1.47 | 0.00 | 0.80 | -16.51 | 46.06 | -23.39 | 114.18 | 0.4190 | 885.0 | 757.5 | |
| 0.00 | 1.21 | 0.00 | 0.66 | -17.55 | 45.72 | -23.73 | 116.23 | 0.4296 | 772.0 | 600.9 | |
| 2.33 | 3.72 | 1.28 | 2.05 | -17.43 | 45.08 | -24.36 | 115.47 | 0.4378 | 842.2 | 539.6 | |
| 0.00 | 2.25 | 0.00 | 1.24 | -16.36 | 44.31 | -25.14 | 112.62 | 0.4434 | -816.0 | -485.5 | |
| 0.00 | 0.95 | 0.00 | 0.52 | -15.63 | 44.10 | -25.35 | 110.90 | 0.4431 | -719.0 | -533.1 | |
| 0.00 | 1.64 | 0.00 | 0.91 | -16.19 | 43.92 | -25.53 | 112.01 | 0.4482 | -823.0 | -716.5 | |
| 0.00 | 4.49 | 0.00 | 2.52 | -17.80 | 42.92 | -26.53 | 114.72 | 0.4701 | -246.0 | -396.8 | |
| 0.00 | 1.21 | 0.00 | 0.67 | -16.18 | 43.10 | -26.35 | 111.48 | 0.4600 | -793.0 | -616.8 | |
| 4.58 | 23.76 | 2.57 | 13.30 | -17.28 | 42.76 | -26.69 | 113.55 | 0.4698 | -809.5 | -893.8 | |
| 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. | |