SDO HMI 2011-11-18 12:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 65.99 | 290.09 | 78.20 | 343.76 | -15.76 | 267.03 | -63.41 | 108.66 | 0.9093 | 53.6 | -29.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.54 | 116.47 | 16.66 | 125.47 | -16.61 | 270.12 | -60.32 | 110.19 | 0.8890 | 720.5 | 195.1 | |
| 3.09 | -1.00 | 3.42 | -1.00 | -17.08 | 269.29 | -61.15 | 110.52 | 0.8959 | 271.4 | 999999 | |
| 1.97 | -1.00 | 2.17 | -1.00 | -16.83 | 269.43 | -61.01 | 110.27 | 0.8944 | 258.5 | 999999 | |
| 5.75 | 24.72 | 6.63 | 28.85 | -17.29 | 268.04 | -62.40 | 110.48 | 0.9051 | 429.6 | -366.7 | |
| 0.86 | -4.00 | 1.02 | -4.00 | -16.91 | 267.24 | -63.20 | 109.91 | 0.9100 | -626.4 | 999999 | |
| 10.81 | 15.71 | 13.23 | 19.17 | -16.83 | 266.31 | -64.13 | 109.63 | 0.9162 | -493.6 | -487.5 | |
| 0.51 | 6.78 | 0.63 | 8.28 | -16.39 | 266.22 | -64.22 | 109.15 | 0.9162 | -692.0 | -525.0 | |
| 0.00 | 1.72 | 0.00 | 2.15 | -16.30 | 265.55 | -64.89 | 108.92 | 0.9204 | -566.0 | -470.8 | |
| 7.12 | 52.10 | 8.41 | 61.60 | -13.89 | 266.77 | -63.67 | 106.55 | 0.9094 | 542.2 | 203.5 | |
| 1.54 | -9.00 | 1.85 | -9.00 | -14.56 | 266.43 | -64.01 | 107.21 | 0.9126 | 157.2 | 999999 | |
| 0.00 | 0.77 | 0.00 | 0.98 | -16.56 | 265.24 | -65.20 | 109.15 | 0.9228 | -264.0 | -241.2 | |
| 4.38 | -9.00 | 5.14 | -9.00 | -13.46 | 266.85 | -63.59 | 106.09 | 0.9084 | 629.4 | 999999 | |
| 0.00 | 1.54 | 0.00 | 1.96 | -16.28 | 265.27 | -65.17 | 108.85 | 0.9222 | -472.0 | -403.2 | |
| 0.00 | 3.86 | 0.00 | 5.09 | -17.06 | 264.45 | -65.99 | 109.54 | 0.9283 | 385.0 | 271.6 | |
| 2.23 | 9.78 | 2.86 | 12.51 | -16.10 | 264.93 | -65.51 | 108.61 | 0.9242 | -570.2 | -366.6 | |
| 0.00 | 1.20 | 0.00 | 1.44 | -13.61 | 266.29 | -64.15 | 106.15 | 0.9124 | 33.0 | -39.4 | |
| 1.63 | -15.00 | 2.09 | -15.00 | -15.92 | 264.98 | -65.46 | 108.41 | 0.9237 | -201.6 | 999999 | |
| 1.46 | -15.00 | 1.87 | -15.00 | -15.79 | 264.98 | -65.46 | 108.28 | 0.9235 | 81.9 | 999999 | |
| 0.00 | 1.03 | 0.00 | 1.34 | -16.33 | 264.63 | -65.81 | 108.80 | 0.9263 | -417.0 | -478.6 | |
| 0.00 | 0.94 | 0.00 | 1.13 | -13.30 | 266.30 | -64.14 | 105.82 | 0.9120 | -183.0 | -154.3 | |
| 0.00 | 1.12 | 0.00 | 1.46 | -16.09 | 264.41 | -66.03 | 108.50 | 0.9275 | -41.0 | -83.5 | |
| 0.00 | 0.94 | 0.00 | 1.33 | -17.93 | 263.00 | -67.44 | 110.21 | 0.9378 | 189.0 | 149.4 | |
| 0.00 | 0.51 | 0.00 | 0.73 | -17.72 | 262.84 | -67.60 | 109.96 | 0.9385 | -73.0 | -134.2 | |
| 0.00 | 0.86 | 0.00 | 1.15 | -15.99 | 263.93 | -66.51 | 108.31 | 0.9303 | -393.0 | -374.9 | |
| 2.32 | 4.55 | 2.89 | 5.67 | -13.34 | 265.27 | -65.17 | 105.70 | 0.9190 | 215.6 | 164.5 | |
| 0.00 | 6.01 | 0.00 | 8.73 | -17.62 | 262.25 | -68.19 | 109.75 | 0.9417 | -720.0 | -466.6 | |
| 0.00 | 2.32 | 0.00 | 2.93 | -13.63 | 264.89 | -65.55 | 105.95 | 0.9218 | -6.0 | -140.6 | |
| 0.00 | 0.86 | 0.00 | 1.18 | -15.92 | 263.26 | -67.18 | 108.13 | 0.9342 | -530.0 | -559.1 | |
| 0.00 | 1.03 | 0.00 | 1.44 | -16.22 | 262.90 | -67.54 | 108.38 | 0.9367 | -155.0 | -209.1 | |
| 0.00 | 1.54 | 0.00 | 2.04 | -14.11 | 263.87 | -66.57 | 106.29 | 0.9288 | -663.0 | -557.8 | |
| 6.78 | 26.01 | 9.33 | 35.80 | -13.96 | 262.92 | -67.52 | 105.99 | 0.9344 | -563.2 | -349.5 | |
| 0.00 | 1.12 | 0.00 | 1.57 | -14.47 | 262.44 | -68.00 | 106.47 | 0.9377 | -439.0 | -409.2 | |
| 0.00 | 2.40 | 0.00 | 3.51 | -15.06 | 261.71 | -68.73 | 106.97 | 0.9424 | -483.0 | -478.0 | |
| 0.00 | 0.77 | 0.00 | 1.10 | -14.08 | 262.28 | -68.16 | 106.03 | 0.9383 | -97.0 | -73.4 | |
| 0.00 | 3.43 | 0.00 | 5.15 | -15.20 | 261.17 | -69.27 | 107.05 | 0.9455 | -128.0 | -152.8 | |
| 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. | |