SOHO MDI 2000-09-29 11:11:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 178 | 894 | 97 | 488 | -11.27 | 352.31 | -17.76 | 136.20 | 0.4303 | 23.6 | 2.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 12 | 0 | 6 | -10.88 | 358.12 | -11.96 | 145.90 | 0.3644 | -816.0 | -587.2 | |
| 0 | 4 | 0 | 2 | -10.47 | 357.97 | -12.10 | 144.93 | 0.3604 | -493.0 | -469.1 | |
| 0 | 5 | 0 | 3 | -13.58 | 357.13 | -12.94 | 147.72 | 0.4094 | -743.0 | -517.7 | |
| 17 | 350 | 9 | 187 | -10.38 | 356.92 | -13.15 | 142.50 | 0.3692 | -2285.0 | -703.6 | |
| 12 | -4 | 6 | -4 | -10.83 | 356.82 | -13.25 | 143.03 | 0.3760 | -1604.1 | 999999 | |
| 0 | 4 | 0 | 2 | -9.00 | 356.81 | -13.26 | 139.85 | 0.3529 | -599.0 | -441.4 | |
| 36 | -4 | 19 | -4 | -11.05 | 356.16 | -13.92 | 142.04 | 0.3854 | -1454.2 | 999999 | |
| 3 | 15 | 2 | 8 | -12.41 | 356.00 | -14.07 | 143.85 | 0.4041 | -753.9 | -664.6 | |
| 0 | 5 | 0 | 3 | -13.07 | 355.92 | -14.15 | 144.66 | 0.4134 | -508.0 | -453.2 | |
| 4 | -4 | 2 | -4 | -11.52 | 355.52 | -14.55 | 141.54 | 0.3976 | -636.5 | 999999 | |
| 0 | 4 | 0 | 2 | -12.47 | 355.30 | -14.77 | 142.60 | 0.4116 | -761.0 | -658.3 | |
| 0 | 4 | 0 | 2 | -13.74 | 354.64 | -15.43 | 143.24 | 0.4337 | -649.0 | -544.9 | |
| 0 | 5 | 0 | 3 | -13.12 | 354.47 | -15.60 | 142.05 | 0.4276 | -728.0 | -540.2 | |
| 0 | 7 | 0 | 4 | -10.42 | 354.34 | -15.73 | 137.50 | 0.3963 | -698.0 | -577.1 | |
| 0 | 6 | 0 | 3 | -12.23 | 353.87 | -16.20 | 139.64 | 0.4229 | 685.0 | 643.9 | |
| 0 | 4 | 0 | 2 | -10.92 | 353.82 | -16.25 | 137.43 | 0.4079 | 484.0 | 400.8 | |
| 0 | 2 | 0 | 1 | -10.07 | 353.83 | -16.24 | 135.97 | 0.3979 | -900.0 | -830.5 | |
| 0 | 6 | 0 | 3 | -10.52 | 353.64 | -16.43 | 136.43 | 0.4052 | 273.0 | 315.9 | |
| 0 | 4 | 0 | 2 | -11.72 | 353.24 | -16.84 | 137.74 | 0.4234 | -205.0 | -245.4 | |
| 0 | 5 | 0 | 3 | -12.10 | 353.13 | -16.94 | 138.15 | 0.4289 | -475.0 | -364.9 | |
| 0 | 3 | 0 | 2 | -14.59 | 352.78 | -17.29 | 141.29 | 0.4619 | -528.0 | -476.7 | |
| 3 | 14 | 2 | 8 | -11.66 | 352.74 | -17.33 | 136.80 | 0.4280 | -284.1 | 114.9 | |
| 0 | 6 | 0 | 3 | -11.55 | 352.25 | -17.82 | 135.83 | 0.4322 | 267.0 | 272.5 | |
| 11 | 161 | 6 | 89 | -11.30 | 351.35 | -18.73 | 133.99 | 0.4394 | 1809.8 | 512.4 | |
| 8 | -24 | 5 | -24 | -11.92 | 351.13 | -18.94 | 134.69 | 0.4485 | 1095.9 | 999999 | |
| 13 | -24 | 7 | -24 | -11.48 | 351.00 | -19.07 | 133.75 | 0.4453 | 1076.2 | 999999 | |
| 10 | -24 | 5 | -24 | -12.07 | 350.70 | -19.37 | 134.27 | 0.4548 | 740.0 | 999999 | |
| 6 | -24 | 4 | -24 | -11.70 | 350.52 | -19.55 | 133.41 | 0.4530 | -918.5 | 999999 | |
| 0 | 2 | 0 | 1 | -11.30 | 350.46 | -19.61 | 132.66 | 0.4494 | -803.0 | -676.8 | |
| 8 | -24 | 4 | -24 | -12.08 | 350.28 | -19.79 | 133.67 | 0.4597 | 831.6 | 999999 | |
| 0 | 6 | 0 | 3 | -13.21 | 348.99 | -21.08 | 133.63 | 0.4858 | 1039.0 | 798.0 | |
| 0 | 10 | 0 | 6 | -11.38 | 348.55 | -21.52 | 130.13 | 0.4724 | 1195.0 | 946.1 | |
| 0 | 4 | 0 | 2 | -12.79 | 348.13 | -21.95 | 131.84 | 0.4912 | 915.0 | 765.1 | |
| 0 | 4 | 0 | 2 | -11.81 | 348.17 | -21.90 | 130.34 | 0.4810 | 802.0 | 607.4 | |
| 0 | 13 | 0 | 7 | -10.28 | 347.69 | -22.38 | 127.19 | 0.4722 | 962.0 | 771.7 | |
| 6 | 13 | 3 | 7 | -12.00 | 347.51 | -22.56 | 129.81 | 0.4906 | 1004.6 | 902.0 | |
| 0 | 4 | 0 | 2 | -15.04 | 347.20 | -22.87 | 133.99 | 0.5238 | 708.0 | 473.4 | |
| 0 | 7 | 0 | 4 | -12.52 | 347.03 | -23.04 | 130.03 | 0.5010 | 592.0 | 547.7 | |
| 26 | 205 | 15 | 116 | -11.38 | 346.79 | -23.29 | 127.92 | 0.4933 | 1544.3 | 688.0 | |
| 15 | -39 | 8 | -39 | -10.58 | 346.51 | -23.56 | 126.27 | 0.4894 | 1296.5 | 999999 | |
| 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. | |