SDO HMI 2014-07-06 16:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.00 | 27.59 | 2.11 | 14.60 | -14.14 | 256.34 | 10.59 | 210.28 | 0.3539 | 430.6 | 434.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.27 | 0.00 | 1.21 | -13.80 | 259.68 | 13.93 | 218.41 | 0.3778 | 734.0 | 644.3 | |
| 0.00 | 1.09 | 0.00 | 0.58 | -13.92 | 259.52 | 13.77 | 217.90 | 0.3778 | 700.0 | 588.6 | |
| 0.00 | 1.45 | 0.00 | 0.77 | -12.87 | 259.37 | 13.62 | 219.41 | 0.3630 | 878.0 | 607.6 | |
| 0.00 | 5.90 | 0.00 | 3.15 | -14.10 | 258.60 | 12.85 | 215.71 | 0.3711 | 465.0 | 693.2 | |
| 0.00 | 1.09 | 0.00 | 0.58 | -13.81 | 258.58 | 12.83 | 216.14 | 0.3672 | 825.0 | 657.1 | |
| 0.00 | 1.18 | 0.00 | 0.63 | -14.29 | 258.35 | 12.60 | 214.88 | 0.3712 | 627.0 | 496.0 | |
| 4.00 | 6.63 | 2.11 | 3.50 | -14.57 | 255.44 | 9.69 | 207.85 | 0.3504 | 991.7 | 797.2 | |
| 0.00 | 1.00 | 0.00 | 0.53 | -14.68 | 254.24 | 8.49 | 204.69 | 0.3433 | 874.0 | 806.1 | |
| 0.00 | 1.54 | 0.00 | 0.80 | -11.79 | 254.04 | 8.29 | 208.31 | 0.2991 | 850.0 | 691.6 | |
| 0.00 | 1.45 | 0.00 | 0.76 | -14.83 | 253.32 | 7.57 | 202.12 | 0.3396 | 739.0 | 486.8 | |
| 0.00 | 1.09 | 0.00 | 0.57 | -15.11 | 252.09 | 6.34 | 198.53 | 0.3368 | -743.0 | -596.7 | |
| 0.00 | 1.36 | 0.00 | 0.71 | -14.47 | 251.98 | 6.23 | 198.86 | 0.3262 | -989.0 | -721.4 | |
| 0.00 | 1.54 | 0.00 | 0.81 | -14.82 | 251.48 | 5.73 | 197.12 | 0.3291 | -977.0 | -785.0 | |
| 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. | |