SDO HMI 2014-03-29 01:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 69.88 | 331.66 | 39.66 | 187.72 | 10.10 | 146.50 | 23.55 | 305.58 | 0.4851 | -433.7 | -277.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.14 | 0.00 | 0.67 | 9.32 | 151.85 | 28.90 | 298.77 | 0.5461 | -535.0 | -396.6 | |
| 0.00 | 1.49 | 0.00 | 0.84 | 4.91 | 149.58 | 26.62 | 292.97 | 0.4868 | -822.0 | -670.1 | |
| 5.25 | 13.49 | 3.04 | 7.80 | 10.50 | 148.98 | 26.02 | 303.39 | 0.5187 | -757.3 | -717.0 | |
| 0.00 | 1.58 | 0.00 | 0.91 | 10.84 | 148.95 | 25.99 | 303.98 | 0.5211 | -517.0 | -391.8 | |
| 0.79 | 3.42 | 0.45 | 1.97 | 10.57 | 148.55 | 25.59 | 303.96 | 0.5139 | -752.3 | -609.8 | |
| 0.00 | 2.01 | 0.00 | 1.16 | 10.93 | 148.14 | 25.18 | 304.97 | 0.5119 | 272.0 | 369.3 | |
| 1.66 | 244.60 | 0.95 | 138.77 | 9.98 | 148.02 | 25.07 | 303.53 | 0.5026 | -594.3 | -359.7 | |
| 0.00 | 0.96 | 0.00 | 0.55 | 10.67 | 148.08 | 25.13 | 304.61 | 0.5091 | -677.0 | -559.7 | |
| 0.00 | 0.96 | 0.00 | 0.55 | 10.72 | 147.85 | 24.90 | 304.95 | 0.5066 | -448.0 | -409.5 | |
| 0.00 | 0.61 | 0.00 | 0.35 | 11.04 | 147.88 | 24.92 | 305.43 | 0.5097 | -464.0 | -374.3 | |
| 1.05 | -7.00 | 0.60 | -7.00 | 9.90 | 147.58 | 24.62 | 303.87 | 0.4963 | -728.2 | 999999 | |
| 1.49 | 8.41 | 0.85 | 4.82 | 11.05 | 147.51 | 24.56 | 305.86 | 0.5053 | -587.1 | -359.1 | |
| 6.22 | -7.00 | 3.54 | -7.00 | 10.14 | 147.33 | 24.38 | 304.54 | 0.4952 | -782.9 | 999999 | |
| 29.25 | -7.00 | 16.59 | -7.00 | 9.66 | 147.16 | 24.20 | 303.92 | 0.4891 | -1066.4 | 999999 | |
| 0.00 | 1.05 | 0.00 | 0.60 | 11.12 | 147.05 | 24.09 | 306.50 | 0.5003 | -258.0 | -220.3 | |
| 0.00 | 2.10 | 0.00 | 1.20 | 10.90 | 146.86 | 23.91 | 306.34 | 0.4960 | -125.0 | -6.1 | |
| 4.64 | 10.07 | 2.64 | 5.74 | 11.23 | 146.63 | 23.67 | 307.16 | 0.4961 | 775.3 | 423.6 | |
| 13.49 | -7.00 | 7.64 | -7.00 | 10.28 | 146.51 | 23.56 | 305.72 | 0.4863 | -929.1 | 999999 | |
| 1.66 | -7.00 | 0.94 | -7.00 | 10.53 | 146.50 | 23.54 | 306.16 | 0.4884 | 345.2 | 999999 | |
| 0.00 | 3.42 | 0.00 | 1.94 | 11.43 | 146.31 | 23.35 | 307.87 | 0.4942 | 586.0 | 668.0 | |
| 1.40 | -7.00 | 0.79 | -7.00 | 10.58 | 146.21 | 23.25 | 306.59 | 0.4852 | 240.7 | 999999 | |
| 0.00 | 1.05 | 0.00 | 0.59 | 10.75 | 145.72 | 22.76 | 307.45 | 0.4808 | 706.0 | 598.9 | |
| 0.00 | 3.42 | 0.00 | 1.90 | 10.02 | 144.12 | 21.17 | 308.24 | 0.4546 | -1006.0 | -841.8 | |
| 0.00 | 1.05 | 0.00 | 0.58 | 7.68 | 143.88 | 20.92 | 304.25 | 0.4300 | -716.0 | -606.4 | |
| 1.93 | 6.48 | 1.06 | 3.56 | 10.80 | 141.88 | 18.92 | 312.79 | 0.4359 | -892.0 | -655.4 | |
| 0.00 | 2.98 | 0.00 | 1.63 | 10.67 | 141.51 | 18.56 | 313.11 | 0.4302 | -818.0 | -664.5 | |
| 0.00 | 1.23 | 0.00 | 0.67 | 10.29 | 140.79 | 17.83 | 313.62 | 0.4179 | 521.0 | 416.8 | |
| 0.00 | 2.10 | 0.00 | 1.14 | 10.00 | 140.51 | 17.56 | 313.55 | 0.4116 | 743.0 | 667.2 | |
| 0.00 | 0.96 | 0.00 | 0.53 | 10.66 | 140.55 | 17.59 | 314.64 | 0.4192 | 519.0 | 456.1 | |
| 0.00 | 2.10 | 0.00 | 1.14 | 9.78 | 140.47 | 17.51 | 313.22 | 0.4087 | 762.0 | 646.1 | |
| 0.00 | 3.07 | 0.00 | 1.66 | 9.58 | 140.08 | 17.12 | 313.51 | 0.4019 | 867.0 | 650.7 | |
| 0.00 | 1.84 | 0.00 | 0.99 | 9.39 | 139.97 | 17.01 | 313.34 | 0.3986 | 861.0 | 674.8 | |
| 0.00 | 1.31 | 0.00 | 0.71 | 9.60 | 139.70 | 16.74 | 314.19 | 0.3978 | 808.0 | 668.3 | |
| 0.00 | 0.88 | 0.00 | 0.47 | 9.07 | 139.54 | 16.58 | 313.47 | 0.3901 | 572.0 | 470.7 | |
| 0.00 | 1.05 | 0.00 | 0.57 | 10.40 | 139.20 | 16.24 | 316.48 | 0.4012 | 833.0 | 679.8 | |
| 1.05 | 5.78 | 0.57 | 3.14 | 11.85 | 138.43 | 15.47 | 320.28 | 0.4103 | 916.1 | 625.2 | |
| 0.00 | 1.05 | 0.00 | 0.57 | 11.53 | 137.40 | 14.44 | 321.72 | 0.3960 | 609.0 | 509.4 | |
| 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. | |