SDO HMI 2014-11-30 15:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 47.76 | 285.31 | 49.04 | 291.21 | -13.62 | 165.13 | 59.84 | 253.82 | 0.8767 | 406.1 | 213.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.51 | 0.00 | 0.67 | -15.30 | 171.98 | 66.68 | 253.03 | 0.9277 | 432.0 | 424.3 | |
| 4.61 | 43.24 | 5.08 | 47.64 | -12.11 | 167.69 | 62.39 | 255.91 | 0.8952 | 494.1 | 80.4 | |
| 2.05 | -2.00 | 2.23 | -2.00 | -12.05 | 167.33 | 62.04 | 255.94 | 0.8924 | 670.7 | 999999 | |
| 1.28 | -2.00 | 1.40 | -2.00 | -12.41 | 167.42 | 62.12 | 255.54 | 0.8934 | 497.1 | 999999 | |
| 0.00 | 3.50 | 0.00 | 3.86 | -12.72 | 167.55 | 62.25 | 255.22 | 0.8947 | 451.0 | 299.3 | |
| 0.00 | 1.28 | 0.00 | 1.34 | -10.54 | 166.21 | 60.91 | 257.46 | 0.8820 | -433.0 | -339.3 | |
| 0.00 | 1.03 | 0.00 | 1.10 | -12.98 | 166.88 | 61.58 | 254.83 | 0.8899 | 327.0 | 381.1 | |
| 0.00 | 0.68 | 0.00 | 0.72 | -12.03 | 166.24 | 60.94 | 255.80 | 0.8838 | 425.0 | 373.0 | |
| 0.00 | 2.48 | 0.00 | 2.55 | -11.47 | 165.66 | 60.36 | 256.34 | 0.8786 | 348.0 | 318.0 | |
| 0.00 | 0.26 | 0.00 | 0.26 | -11.20 | 165.32 | 60.02 | 256.60 | 0.8755 | 395.0 | 379.3 | |
| 0.00 | 0.26 | 0.00 | 0.28 | -15.03 | 166.79 | 61.50 | 252.54 | 0.8917 | -493.0 | -391.0 | |
| 0.00 | 2.48 | 0.00 | 2.52 | -11.62 | 165.16 | 59.86 | 256.10 | 0.8747 | 508.0 | 484.4 | |
| 0.77 | 2.05 | 0.78 | 2.07 | -11.89 | 165.01 | 59.72 | 255.77 | 0.8738 | 503.7 | 453.7 | |
| 1.11 | 8.54 | 1.10 | 8.53 | -11.06 | 164.55 | 59.25 | 256.64 | 0.8690 | -556.7 | -300.7 | |
| 4.02 | 194.48 | 4.11 | 196.98 | -13.62 | 165.15 | 59.85 | 253.83 | 0.8770 | 473.0 | 305.7 | |
| 0.00 | 1.11 | 0.00 | 1.10 | -11.82 | 164.39 | 59.10 | 255.76 | 0.8685 | 323.0 | 246.8 | |
| 0.00 | 1.71 | 0.00 | 1.70 | -12.52 | 164.47 | 59.17 | 254.97 | 0.8700 | 411.0 | 296.3 | |
| 0.00 | 1.11 | 0.00 | 1.11 | -12.79 | 164.33 | 59.03 | 254.64 | 0.8692 | 418.0 | 400.8 | |
| 32.47 | -15.00 | 33.03 | -15.00 | -14.23 | 164.86 | 59.56 | 253.09 | 0.8755 | 801.5 | 999999 | |
| 0.00 | 1.11 | 0.00 | 1.14 | -15.40 | 165.08 | 59.79 | 251.81 | 0.8789 | 467.0 | 373.1 | |
| 0.00 | 4.10 | 0.00 | 3.86 | -13.42 | 162.26 | 56.96 | 253.53 | 0.8524 | 413.0 | 247.5 | |
| 0.00 | 0.94 | 0.00 | 0.87 | -13.14 | 161.54 | 56.25 | 253.73 | 0.8456 | -150.0 | -101.2 | |
| 0.00 | 0.94 | 0.00 | 0.87 | -13.78 | 161.44 | 56.15 | 252.96 | 0.8457 | -93.0 | -48.9 | |
| 0.00 | 1.37 | 0.00 | 1.25 | -13.84 | 161.19 | 55.89 | 252.84 | 0.8436 | -248.0 | -243.8 | |
| 0.00 | 0.77 | 0.00 | 0.70 | -13.10 | 160.88 | 55.58 | 253.64 | 0.8395 | -648.0 | -604.6 | |
| 0.00 | 0.94 | 0.00 | 0.86 | -13.92 | 160.95 | 55.65 | 252.69 | 0.8416 | -439.0 | -387.5 | |
| 0.00 | 0.60 | 0.00 | 0.54 | -13.58 | 160.72 | 55.42 | 253.04 | 0.8389 | -423.0 | -314.4 | |
| 0.00 | 0.60 | 0.00 | 0.55 | -14.32 | 160.93 | 55.64 | 252.22 | 0.8421 | -376.0 | -319.9 | |
| 0.60 | 1.79 | 0.54 | 1.61 | -14.68 | 160.15 | 54.85 | 251.63 | 0.8356 | -611.7 | -513.1 | |
| 0.00 | 0.26 | 0.00 | 0.22 | -12.80 | 159.24 | 53.95 | 253.66 | 0.8238 | -445.0 | -449.3 | |
| 0.85 | 3.33 | 0.77 | 2.99 | -15.44 | 160.12 | 54.83 | 250.72 | 0.8369 | -674.0 | -561.2 | |
| 0.00 | 0.26 | 0.00 | 0.22 | -12.98 | 159.25 | 53.95 | 253.44 | 0.8242 | -295.0 | -353.0 | |
| 0.00 | 0.85 | 0.00 | 0.76 | -15.23 | 159.88 | 54.58 | 250.92 | 0.8342 | -625.0 | -542.5 | |
| 0.00 | 0.60 | 0.00 | 0.52 | -13.56 | 158.86 | 53.57 | 252.67 | 0.8216 | -420.0 | -383.7 | |
| 0.00 | 0.85 | 0.00 | 0.73 | -13.67 | 158.34 | 53.04 | 252.41 | 0.8167 | -576.0 | -553.8 | |
| 0.00 | 1.28 | 0.00 | 1.09 | -15.35 | 157.89 | 52.60 | 250.29 | 0.8160 | -429.0 | -330.8 | |
| 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. | |