| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 112.52 | 398.99 | 85.29 | 302.01 | -15.43 | 266.55 | -46.30 | 112.84 | 0.7580 | 95.1 | 16.0 | |
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back to the solar disc SDO HMI 2011-11-19 20:58:57 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.06 | 103.09 | 3.62 | 74.40 | -16.62 | 270.12 | -42.73 | 115.81 | 0.7246 | 974.4 | 339.3 | |
| 2.06 | 2.40 | 1.49 | 1.74 | -17.20 | 269.53 | -43.32 | 116.29 | 0.7334 | 581.1 | 448.5 | |
| 25.04 | -1.00 | 18.10 | -1.00 | -16.61 | 269.53 | -43.32 | 115.53 | 0.7309 | 807.1 | 999999 | |
| 0.00 | 0.94 | 0.00 | 0.69 | -17.37 | 269.22 | -43.63 | 116.37 | 0.7373 | 373.0 | 298.4 | |
| 0.00 | 0.69 | 0.00 | 0.51 | -17.32 | 267.66 | -45.18 | 115.63 | 0.7534 | 430.0 | 405.0 | |
| 1.89 | 2.49 | 1.44 | 1.90 | -17.13 | 266.74 | -46.10 | 115.01 | 0.7622 | 373.2 | 329.7 | |
| 2.57 | 99.49 | 1.88 | 72.95 | -12.83 | 267.58 | -45.27 | 109.83 | 0.7387 | 882.5 | 337.2 | |
| 18.27 | -7.00 | 13.42 | -7.00 | -13.17 | 267.50 | -45.35 | 110.25 | 0.7407 | 878.3 | 999999 | |
| 1.37 | -7.00 | 1.01 | -7.00 | -12.68 | 267.44 | -45.41 | 109.59 | 0.7398 | 549.1 | 999999 | |
| 0.00 | 1.46 | 0.00 | 1.12 | -16.96 | 266.17 | -46.68 | 114.57 | 0.7675 | -368.0 | -317.2 | |
| 13.89 | 107.81 | 10.71 | 83.44 | -16.40 | 265.89 | -46.96 | 113.78 | 0.7684 | -957.1 | -373.1 | |
| 2.66 | -11.00 | 2.05 | -11.00 | -16.10 | 265.72 | -47.13 | 113.33 | 0.7692 | -791.0 | 999999 | |
| 1.29 | 3.52 | 0.97 | 2.66 | -14.22 | 266.22 | -46.63 | 111.15 | 0.7579 | 451.3 | 395.5 | |
| 3.77 | -11.00 | 2.93 | -11.00 | -16.01 | 265.42 | -47.42 | 113.12 | 0.7719 | -715.9 | 999999 | |
| 1.37 | -11.00 | 1.07 | -11.00 | -16.49 | 265.27 | -47.58 | 113.65 | 0.7750 | -451.2 | 999999 | |
| 0.00 | 1.54 | 0.00 | 1.16 | -13.12 | 266.19 | -46.66 | 109.73 | 0.7548 | 602.0 | 468.6 | |
| 1.20 | -11.00 | 0.94 | -11.00 | -16.93 | 265.03 | -47.82 | 114.11 | 0.7789 | -504.9 | 999999 | |
| 5.23 | 6.18 | 3.93 | 4.64 | -12.72 | 266.11 | -46.74 | 109.19 | 0.7545 | 612.8 | 307.6 | |
| 0.43 | -11.00 | 0.33 | -11.00 | -15.93 | 265.22 | -47.63 | 112.94 | 0.7737 | 437.2 | 999999 | |
| 3.09 | -11.00 | 2.44 | -11.00 | -16.85 | 264.73 | -48.11 | 113.89 | 0.7816 | 425.4 | 999999 | |
| 0.86 | -11.00 | 0.67 | -11.00 | -16.44 | 264.87 | -47.98 | 113.44 | 0.7789 | 538.6 | 999999 | |
| 0.00 | 1.29 | 0.00 | 0.99 | -13.97 | 265.48 | -47.37 | 110.57 | 0.7650 | 442.0 | 411.5 | |
| 0.00 | 1.80 | 0.00 | 1.40 | -14.24 | 264.76 | -48.08 | 110.67 | 0.7732 | 493.0 | 487.8 | |
| 3.43 | 5.15 | 2.77 | 4.16 | -17.16 | 263.78 | -49.07 | 113.93 | 0.7920 | 494.1 | 270.0 | |
| 0.00 | 1.11 | 0.00 | 0.87 | -14.77 | 264.52 | -48.33 | 111.25 | 0.7773 | 473.0 | 406.2 | |
| 0.00 | 0.86 | 0.00 | 0.67 | -14.46 | 264.56 | -48.29 | 110.88 | 0.7760 | 424.0 | 431.0 | |
| 0.00 | 2.06 | 0.00 | 1.58 | -12.66 | 265.00 | -47.85 | 108.76 | 0.7662 | 654.0 | 466.0 | |
| 0.00 | 0.86 | 0.00 | 0.69 | -16.70 | 263.46 | -49.38 | 113.26 | 0.7937 | -647.0 | -604.8 | |
| 0.00 | 0.86 | 0.00 | 0.69 | -16.26 | 263.52 | -49.33 | 112.75 | 0.7918 | -670.0 | -557.8 | |
| 0.00 | 3.86 | 0.00 | 3.15 | -16.80 | 263.19 | -49.66 | 113.29 | 0.7967 | -720.0 | -582.2 | |
| 0.00 | 2.66 | 0.00 | 2.17 | -16.62 | 263.06 | -49.79 | 113.03 | 0.7973 | -533.0 | -455.8 | |
| 0.00 | 1.72 | 0.00 | 1.41 | -17.16 | 262.87 | -49.98 | 113.61 | 0.8008 | 350.0 | 265.3 | |
| 0.00 | 0.94 | 0.00 | 0.77 | -16.97 | 262.94 | -49.91 | 113.40 | 0.7996 | -572.0 | -562.5 | |
| 0.00 | 0.86 | 0.00 | 0.72 | -17.74 | 262.40 | -50.44 | 114.14 | 0.8070 | 358.0 | 232.8 | |
| 1.20 | 2.14 | 1.01 | 1.80 | -17.43 | 262.08 | -50.77 | 113.67 | 0.8092 | -716.4 | -558.9 | |
| 13.98 | 23.84 | 11.26 | 19.18 | -14.05 | 262.99 | -49.85 | 109.87 | 0.7908 | -779.5 | -555.3 | |
| 0.00 | 3.95 | 0.00 | 3.39 | -18.62 | 261.34 | -51.50 | 114.83 | 0.8194 | -690.0 | -649.6 | |
| 0.00 | 2.06 | 0.00 | 1.78 | -18.20 | 260.92 | -51.93 | 114.19 | 0.8221 | -582.0 | -459.9 | |
| 0.00 | 1.37 | 0.00 | 1.17 | -16.99 | 261.15 | -51.70 | 112.85 | 0.8166 | -742.0 | -591.1 | |
| 1.11 | 1.97 | 0.94 | 1.66 | -15.86 | 261.53 | -51.32 | 111.62 | 0.8100 | -584.4 | -594.7 | |
| 0.00 | 1.29 | 0.00 | 1.12 | -18.14 | 260.63 | -52.21 | 114.03 | 0.8245 | -386.0 | -298.7 | |
| 0.00 | 0.94 | 0.00 | 0.81 | -16.84 | 261.11 | -51.74 | 112.65 | 0.8165 | -509.0 | -484.0 | |
| 1.29 | 2.74 | 1.08 | 2.32 | -15.50 | 261.26 | -51.59 | 111.10 | 0.8116 | -666.3 | -448.9 | |
| 0.00 | 0.77 | 0.00 | 0.67 | -17.11 | 260.65 | -52.19 | 112.82 | 0.8215 | -355.0 | -291.6 | |
| 1.46 | 1.80 | 1.23 | 1.51 | -15.15 | 261.28 | -51.57 | 110.70 | 0.8105 | -484.4 | -637.5 | |
| 0.00 | 1.97 | 0.00 | 1.67 | -15.38 | 261.05 | -51.80 | 110.90 | 0.8133 | -366.0 | -314.5 | |
| 0.00 | 0.51 | 0.00 | 0.45 | -15.75 | 259.28 | -53.57 | 110.82 | 0.8306 | -416.0 | -398.2 | |
| 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. | |