SDO HMI 2013-09-20 04:59:04 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 60.91 | 345.60 | 48.99 | 278.01 | -17.64 | 58.59 | -46.13 | 119.12 | 0.7886 | 760.4 | 218.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 57.36 | 329.72 | 45.77 | 263.97 | -17.68 | 58.85 | -45.87 | 119.28 | 0.7864 | 1071.5 | 245.9 | |
| 0.00 | 1.60 | 0.00 | 1.26 | -16.38 | 58.86 | -45.86 | 117.76 | 0.7804 | 281.0 | 250.1 | |
| 0.00 | 0.89 | 0.00 | 0.74 | -18.34 | 57.14 | -47.59 | 119.19 | 0.8050 | 0.0 | 39.3 | |
| 0.00 | 1.60 | 0.00 | 1.35 | -18.76 | 56.55 | -48.17 | 119.38 | 0.8119 | -416.0 | -427.1 | |
| 0.00 | 0.71 | 0.00 | 0.61 | -16.69 | 54.85 | -49.88 | 116.27 | 0.8189 | -475.0 | -415.0 | |
| 0.00 | 0.80 | 0.00 | 0.73 | -18.26 | 52.62 | -52.11 | 117.07 | 0.8438 | -530.0 | -422.6 | |
| 0.00 | 1.68 | 0.00 | 1.52 | -16.94 | 52.75 | -51.98 | 115.66 | 0.8381 | -777.0 | -629.1 | |
| 0.00 | 0.80 | 0.00 | 0.72 | -16.56 | 52.64 | -52.08 | 115.19 | 0.8378 | -521.0 | -538.9 | |
| 0.00 | 1.15 | 0.00 | 1.05 | -17.17 | 52.34 | -52.38 | 115.76 | 0.8424 | -503.0 | -475.2 | |
| 0.71 | 1.68 | 0.65 | 1.54 | -16.66 | 52.24 | -52.49 | 115.15 | 0.8416 | -333.8 | -242.0 | |
| 2.84 | 3.99 | 2.57 | 3.62 | -16.33 | 52.32 | -52.41 | 114.81 | 0.8398 | -543.2 | -453.8 | |
| 0.00 | 0.98 | 0.00 | 0.90 | -15.64 | 51.43 | -53.29 | 113.70 | 0.8452 | -393.0 | -331.9 | |
| 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. | |