SDO HMI 2014-09-08 17:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 33.96 | 159.63 | 32.10 | 152.69 | -16.40 | 64.61 | -54.39 | 114.24 | 0.8563 | 324.4 | 29.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.53 | 0.00 | 0.47 | -17.75 | 68.16 | -50.84 | 117.12 | 0.8319 | 387.0 | 323.5 | |
| 26.12 | 108.47 | 23.76 | 98.69 | -16.32 | 66.52 | -52.48 | 114.84 | 0.8409 | 731.5 | 186.4 | |
| 0.00 | 1.16 | 0.00 | 1.09 | -16.48 | 65.30 | -53.70 | 114.55 | 0.8517 | 513.0 | 333.3 | |
| 0.00 | 1.25 | 0.00 | 1.19 | -16.73 | 64.76 | -54.24 | 114.62 | 0.8569 | 406.0 | 323.8 | |
| 0.00 | 2.32 | 0.00 | 2.20 | -16.18 | 64.77 | -54.23 | 114.01 | 0.8551 | 444.0 | 358.3 | |
| 0.71 | 1.60 | 0.69 | 1.55 | -16.63 | 64.20 | -54.80 | 114.30 | 0.8611 | 192.6 | 117.6 | |
| 0.00 | 1.07 | 0.00 | 1.07 | -16.75 | 63.03 | -55.97 | 114.01 | 0.8707 | -279.0 | -295.9 | |
| 0.00 | 0.45 | 0.00 | 0.47 | -16.52 | 61.28 | -57.72 | 113.16 | 0.8835 | -672.0 | -650.0 | |
| 0.00 | 0.98 | 0.00 | 1.04 | -16.61 | 61.06 | -57.94 | 113.18 | 0.8854 | -443.0 | -505.1 | |
| 3.03 | 40.20 | 3.25 | 43.15 | -16.66 | 60.61 | -58.39 | 113.08 | 0.8888 | -609.1 | -291.1 | |
| 2.85 | -10.00 | 3.04 | -10.00 | -16.30 | 60.67 | -58.33 | 112.71 | 0.8875 | -659.8 | 999999 | |
| 0.00 | 1.60 | 0.00 | 1.77 | -17.38 | 60.00 | -59.00 | 113.65 | 0.8949 | -520.0 | -393.9 | |
| 1.25 | -10.00 | 1.36 | -10.00 | -16.65 | 60.13 | -58.87 | 112.91 | 0.8922 | -259.7 | 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. | |