SOHO MDI 2000-07-10 04:47:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 235 | 1814 | 205 | 1600 | 18.01 | 309.36 | -55.13 | 70.71 | 0.8263 | -406.4 | -382.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12 | 88 | 8 | 60 | 18.94 | 323.11 | -41.38 | 66.25 | 0.6855 | 1309.4 | 561.8 | |
| 6 | -1 | 4 | -1 | 18.92 | 322.67 | -41.82 | 66.43 | 0.6905 | 762.2 | 999999 | |
| 0 | 6 | 0 | 4 | 19.15 | 320.53 | -43.97 | 66.82 | 0.7157 | 451.0 | 390.8 | |
| 0 | 6 | 0 | 4 | 18.45 | 320.52 | -43.97 | 67.78 | 0.7137 | 429.0 | 331.5 | |
| 0 | 5 | 0 | 3 | 16.59 | 321.03 | -43.46 | 70.21 | 0.7029 | 742.0 | 639.7 | |
| 0 | 10 | 0 | 7 | 18.05 | 319.84 | -44.66 | 68.53 | 0.7204 | 486.0 | 481.6 | |
| 0 | 6 | 0 | 4 | 17.40 | 319.22 | -45.28 | 69.58 | 0.7257 | 201.0 | 216.6 | |
| 0 | 14 | 0 | 10 | 18.40 | 318.59 | -45.91 | 68.41 | 0.7352 | -951.0 | -464.8 | |
| 10 | 82 | 7 | 61 | 19.21 | 317.32 | -47.17 | 67.69 | 0.7509 | -1168.6 | -495.1 | |
| 0 | 5 | 0 | 4 | 18.34 | 317.33 | -47.16 | 68.82 | 0.7488 | -700.0 | -546.0 | |
| 0 | 7 | 0 | 5 | 17.53 | 317.55 | -46.94 | 69.83 | 0.7445 | -746.0 | -753.4 | |
| 7 | 79 | 5 | 61 | 19.08 | 316.31 | -48.19 | 68.12 | 0.7614 | -939.6 | -422.5 | |
| 0 | 5 | 0 | 4 | 17.44 | 316.53 | -47.96 | 70.19 | 0.7554 | -748.0 | -704.0 | |
| 8 | -12 | 6 | -12 | 19.14 | 315.84 | -48.65 | 68.16 | 0.7664 | -880.0 | 999999 | |
| 0 | 8 | 0 | 6 | 17.74 | 315.99 | -48.50 | 69.92 | 0.7618 | -619.0 | -534.0 | |
| 10 | -12 | 8 | -12 | 18.75 | 315.54 | -48.95 | 68.73 | 0.7686 | -727.0 | 999999 | |
| 0 | 5 | 0 | 4 | 19.91 | 313.88 | -50.61 | 67.64 | 0.7879 | -477.0 | -476.9 | |
| 0 | 3 | 0 | 2 | 19.20 | 312.92 | -51.57 | 68.74 | 0.7961 | 499.0 | 373.0 | |
| 0 | 5 | 0 | 4 | 18.39 | 312.52 | -51.97 | 69.82 | 0.7985 | 508.0 | 502.1 | |
| 0 | 3 | 0 | 3 | 19.39 | 311.17 | -53.32 | 68.85 | 0.8134 | 550.0 | 406.3 | |
| 0 | 3 | 0 | 3 | 17.57 | 311.91 | -52.58 | 70.95 | 0.8033 | -444.0 | -370.2 | |
| 0 | 2 | 0 | 2 | 19.79 | 310.76 | -53.73 | 68.45 | 0.8178 | 660.0 | 568.0 | |
| 0 | 4 | 0 | 3 | 19.98 | 310.52 | -53.97 | 68.26 | 0.8204 | 471.0 | 551.6 | |
| 12 | 1409 | 10 | 1287 | 18.46 | 309.89 | -54.60 | 70.21 | 0.8239 | -1588.4 | -457.1 | |
| 42 | -24 | 37 | -24 | 19.18 | 309.54 | -54.95 | 69.40 | 0.8282 | 553.5 | 999999 | |
| -25 | -24 | -25 | -24 | 18.66 | 309.14 | -55.36 | 70.09 | 0.8312 | 999999 | 999999 | |
| 6 | -24 | 6 | -24 | 18.05 | 309.35 | -55.14 | 70.78 | 0.8283 | -1746.7 | 999999 | |
| 19 | -24 | 17 | -24 | 15.77 | 309.63 | -54.87 | 73.50 | 0.8230 | -1437.7 | 999999 | |
| 21 | -24 | 18 | -24 | 17.05 | 309.01 | -55.48 | 72.04 | 0.8302 | -1376.8 | 999999 | |
| 6 | -24 | 5 | -24 | 19.01 | 307.90 | -56.59 | 69.87 | 0.8427 | 441.1 | 999999 | |
| 19 | -24 | 17 | -24 | 16.62 | 308.76 | -55.74 | 72.59 | 0.8321 | -869.0 | 999999 | |
| 21 | -24 | 20 | -24 | 19.47 | 306.48 | -58.01 | 69.54 | 0.8556 | 844.0 | 999999 | |
| 0 | 2 | 0 | 2 | 15.93 | 307.41 | -57.08 | 73.57 | 0.8437 | 258.0 | 200.5 | |
| 0 | 20 | 0 | 19 | 15.01 | 307.04 | -57.45 | 74.69 | 0.8462 | 140.0 | 103.2 | |
| 0 | 5 | 0 | 5 | 16.14 | 305.99 | -58.50 | 73.48 | 0.8564 | -437.0 | -404.6 | |
| 0 | 6 | 0 | 6 | 14.54 | 306.62 | -57.87 | 75.29 | 0.8496 | 614.0 | 474.9 | |
| 2 | 9 | 2 | 10 | 19.42 | 303.50 | -60.99 | 69.99 | 0.8797 | 120.7 | 108.7 | |
| 0 | 4 | 0 | 4 | 15.38 | 305.63 | -58.87 | 74.40 | 0.8589 | 222.0 | 251.3 | |
| 8 | -24 | 8 | -24 | 18.57 | 303.78 | -60.72 | 70.93 | 0.8768 | 164.9 | 999999 | |
| 26 | -24 | 27 | -24 | 17.64 | 304.15 | -60.35 | 71.95 | 0.8730 | -954.7 | 999999 | |
| 0 | 13 | 0 | 13 | 16.11 | 304.79 | -59.70 | 73.63 | 0.8666 | 253.0 | -171.4 | |
| 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. | |