SDO HMI 2014-03-01 06:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.52 | 53.74 | 0.27 | 28.67 | 10.27 | 119.88 | -9.40 | 23.31 | 0.3592 | -411.9 | -339.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.29 | 0.00 | 0.66 | 7.01 | 128.73 | -0.55 | 2.21 | 0.2472 | -1000.0 | -816.9 | |
| 0.00 | 1.47 | 0.00 | 0.74 | 4.57 | 128.73 | -0.55 | 2.67 | 0.2056 | -531.0 | -512.8 | |
| 0.52 | 2.33 | 0.27 | 1.20 | 9.42 | 128.58 | -0.70 | 2.40 | 0.2879 | -958.8 | -763.6 | |
| 0.00 | 1.81 | 0.00 | 0.92 | 4.69 | 128.55 | -0.73 | 3.50 | 0.2078 | -1057.0 | -829.5 | |
| 0.00 | 1.29 | 0.00 | 0.67 | 9.45 | 128.37 | -0.91 | 3.12 | 0.2886 | -1026.0 | -909.1 | |
| 0.00 | 0.78 | 0.00 | 0.40 | 7.17 | 128.31 | -0.97 | 3.85 | 0.2502 | -843.0 | -627.7 | |
| 0.00 | 3.71 | 0.00 | 1.92 | 9.88 | 128.28 | -1.00 | 3.35 | 0.2960 | -1004.0 | -786.6 | |
| 0.00 | 1.55 | 0.00 | 0.81 | 9.98 | 128.06 | -1.21 | 4.03 | 0.2978 | -909.0 | -779.3 | |
| 0.00 | 1.29 | 0.00 | 0.66 | 7.84 | 128.04 | -1.24 | 4.70 | 0.2620 | -711.0 | -514.3 | |
| 0.00 | 2.33 | 0.00 | 1.19 | 7.54 | 127.98 | -1.30 | 5.03 | 0.2569 | -853.0 | -706.3 | |
| 0.00 | 1.12 | 0.00 | 0.58 | 10.66 | 127.85 | -1.42 | 4.55 | 0.3095 | -815.0 | -583.8 | |
| 0.00 | 1.38 | 0.00 | 0.71 | 6.86 | 127.77 | -1.50 | 6.12 | 0.2458 | -894.0 | -748.2 | |
| 0.00 | 1.90 | 0.00 | 0.99 | 10.48 | 127.34 | -1.94 | 6.24 | 0.3072 | -570.0 | -614.1 | |
| 0.00 | 1.29 | 0.00 | 0.67 | 10.79 | 127.03 | -2.24 | 7.09 | 0.3130 | -760.0 | -601.4 | |
| 0.00 | 1.64 | 0.00 | 0.83 | 5.77 | 126.97 | -2.31 | 10.12 | 0.2293 | -886.0 | -604.2 | |
| 0.00 | 0.69 | 0.00 | 0.36 | 11.06 | 121.07 | -8.20 | 24.14 | 0.3439 | -779.0 | -655.2 | |
| 0.00 | 1.99 | 0.00 | 1.06 | 12.33 | 120.36 | -8.92 | 24.44 | 0.3676 | -827.0 | -664.5 | |
| 0.00 | 0.60 | 0.00 | 0.32 | 12.87 | 120.19 | -9.09 | 24.24 | 0.3768 | -714.0 | -595.7 | |
| 0.00 | 2.59 | 0.00 | 1.41 | 15.36 | 119.99 | -9.28 | 22.13 | 0.4147 | -794.0 | -543.3 | |
| 0.00 | 0.95 | 0.00 | 0.50 | 11.03 | 119.60 | -9.67 | 27.90 | 0.3540 | -861.0 | -748.3 | |
| 0.00 | 1.29 | 0.00 | 0.70 | 14.39 | 119.07 | -10.21 | 25.10 | 0.4064 | -451.0 | -483.9 | |
| 0.00 | 0.86 | 0.00 | 0.47 | 14.11 | 118.71 | -10.57 | 26.18 | 0.4049 | -859.0 | -711.3 | |
| 0.00 | 0.86 | 0.00 | 0.46 | 12.63 | 118.40 | -10.87 | 28.62 | 0.3860 | -624.0 | -539.4 | |
| 0.00 | 0.60 | 0.00 | 0.33 | 14.45 | 118.04 | -11.24 | 27.22 | 0.4145 | -723.0 | -645.0 | |
| 0.00 | 1.99 | 0.00 | 1.07 | 12.12 | 117.27 | -12.00 | 31.74 | 0.3881 | -1038.0 | -796.1 | |
| 0.00 | 1.38 | 0.00 | 0.74 | 12.23 | 117.05 | -12.22 | 32.07 | 0.3914 | -847.0 | -709.3 | |
| 0.00 | 0.86 | 0.00 | 0.47 | 12.21 | 116.37 | -12.91 | 33.51 | 0.3971 | -774.0 | -739.8 | |
| 0.00 | 2.50 | 0.00 | 1.36 | 9.15 | 110.68 | -18.60 | 48.83 | 0.4201 | 715.0 | 568.0 | |
| 0.00 | 1.29 | 0.00 | 0.70 | 7.30 | 110.64 | -18.63 | 52.38 | 0.4019 | 850.0 | 580.4 | |
| 0.00 | 1.04 | 0.00 | 0.57 | 11.35 | 110.07 | -19.21 | 45.98 | 0.4505 | 848.0 | 631.1 | |
| 0.00 | 2.16 | 0.00 | 1.18 | 8.58 | 109.53 | -19.74 | 51.57 | 0.4282 | 697.0 | 568.2 | |
| 0.00 | 1.38 | 0.00 | 0.80 | 15.34 | 108.26 | -21.02 | 42.65 | 0.5127 | 297.0 | 328.9 | |
| 0.00 | 1.04 | 0.00 | 0.60 | 15.42 | 107.78 | -21.49 | 43.16 | 0.5184 | 632.0 | 477.8 | |
| 0.00 | 1.47 | 0.00 | 0.85 | 13.82 | 106.06 | -23.22 | 47.63 | 0.5202 | 752.0 | 636.8 | |
| 0.00 | 0.95 | 0.00 | 0.55 | 10.31 | 103.59 | -25.68 | 55.87 | 0.5172 | 712.0 | 599.5 | |
| 0.00 | 0.69 | 0.00 | 0.40 | 10.16 | 102.42 | -26.85 | 57.30 | 0.5305 | 773.0 | 720.5 | |
| 0.00 | 1.38 | 0.00 | 0.82 | 7.72 | 99.10 | -30.18 | 64.19 | 0.5555 | 741.0 | 619.9 | |
| 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. | |