SDO HMI 2011-11-03 08:58:59 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 97.46 | 483.82 | 79.81 | 393.64 | -13.84 | 120.80 | -49.59 | 111.14 | 0.7941 | 389.6 | 184.6 | |
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See sunspots with tool (Click here to study sunspot positions and configurations with tool using white-light and magnetogram images and polarity drawing) (It is recommended to set high resolution on your display!) |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.73 | 0.00 | 1.29 | -18.74 | 127.10 | -43.30 | 119.71 | 0.7500 | 696.0 | 539.0 | |
| 5.36 | 277.12 | 4.12 | 214.84 | -14.91 | 123.94 | -46.45 | 113.54 | 0.7663 | 997.3 | 281.4 | |
| 4.07 | -2.00 | 3.11 | -2.00 | -14.57 | 123.94 | -46.45 | 113.11 | 0.7650 | 1052.7 | 999999 | |
| 9.25 | -2.00 | 7.19 | -2.00 | -15.53 | 123.53 | -46.86 | 114.13 | 0.7727 | 707.6 | 999999 | |
| 20.93 | -2.00 | 16.24 | -2.00 | -14.97 | 123.42 | -46.97 | 113.40 | 0.7717 | 784.5 | 999999 | |
| 0.86 | -2.00 | 0.68 | -2.00 | -15.39 | 123.16 | -47.23 | 113.81 | 0.7759 | 412.3 | 999999 | |
| 5.88 | -2.00 | 4.56 | -2.00 | -14.48 | 123.25 | -47.14 | 112.73 | 0.7718 | 748.7 | 999999 | |
| 3.55 | -2.00 | 2.77 | -2.00 | -14.59 | 122.90 | -47.50 | 112.73 | 0.7758 | 465.7 | 999999 | |
| 0.00 | 1.30 | 0.00 | 1.04 | -14.90 | 121.88 | -48.51 | 112.71 | 0.7870 | 340.0 | 298.5 | |
| 0.00 | 3.11 | 0.00 | 2.49 | -14.29 | 121.69 | -48.70 | 111.90 | 0.7869 | 343.0 | 318.3 | |
| 1.12 | 2.16 | 0.90 | 1.73 | -14.11 | 121.41 | -48.98 | 111.59 | 0.7892 | 349.2 | 367.1 | |
| 0.00 | 1.21 | 0.00 | 0.98 | -14.82 | 121.06 | -49.33 | 112.31 | 0.7949 | 293.0 | 178.8 | |
| 1.99 | 3.55 | 1.60 | 2.85 | -13.72 | 121.15 | -49.24 | 111.02 | 0.7906 | 475.7 | 459.4 | |
| 0.00 | 3.03 | 0.00 | 2.52 | -13.42 | 119.46 | -50.93 | 110.08 | 0.8063 | -745.0 | -643.2 | |
| 0.00 | 1.04 | 0.00 | 0.87 | -13.31 | 119.25 | -51.14 | 109.88 | 0.8080 | -526.0 | -521.7 | |
| 5.45 | 6.83 | 4.67 | 5.85 | -14.62 | 118.54 | -51.85 | 111.21 | 0.8184 | -749.7 | -671.3 | |
| 1.12 | 4.93 | 0.99 | 4.35 | -14.78 | 117.42 | -52.97 | 111.04 | 0.8292 | -647.8 | -640.7 | |
| 1.82 | 15.91 | 1.61 | 14.17 | -15.11 | 117.20 | -53.19 | 111.35 | 0.8321 | -790.2 | -581.0 | |
| 3.81 | -18.00 | 3.41 | -18.00 | -15.19 | 116.86 | -53.53 | 111.33 | 0.8354 | -366.5 | 999999 | |
| 9.25 | 116.33 | 7.83 | 99.22 | -11.00 | 118.11 | -52.28 | 106.77 | 0.8132 | 909.2 | 225.8 | |
| 3.89 | 5.19 | 3.44 | 4.58 | -13.81 | 117.03 | -53.36 | 109.78 | 0.8302 | -583.5 | -453.4 | |
| 2.25 | 19.46 | 2.04 | 17.70 | -15.44 | 116.40 | -54.00 | 111.48 | 0.8401 | -289.3 | -250.0 | |
| 1.12 | -22.00 | 1.02 | -22.00 | -15.19 | 116.49 | -53.90 | 111.21 | 0.8386 | -381.3 | 999999 | |
| 12.97 | -20.00 | 11.13 | -20.00 | -10.97 | 117.51 | -52.88 | 106.57 | 0.8189 | 539.0 | 999999 | |
| 0.95 | 10.29 | 0.86 | 9.32 | -14.67 | 116.21 | -54.18 | 110.53 | 0.8398 | -259.4 | -115.9 | |
| 1.82 | -25.00 | 1.64 | -25.00 | -14.42 | 116.25 | -54.14 | 110.25 | 0.8388 | -345.1 | 999999 | |
| 0.00 | 1.56 | 0.00 | 1.49 | -15.60 | 114.38 | -56.01 | 111.05 | 0.8578 | -288.0 | -267.8 | |
| 0.00 | 0.86 | 0.00 | 0.76 | -10.11 | 116.09 | -54.30 | 105.17 | 0.8305 | 634.0 | 462.9 | |
| 0.00 | 0.95 | 0.00 | 0.92 | -14.23 | 113.76 | -56.63 | 109.33 | 0.8599 | -277.0 | -279.2 | |
| 0.00 | 5.10 | 0.00 | 4.64 | -10.23 | 115.00 | -55.39 | 105.06 | 0.8409 | 658.0 | 507.6 | |
| 0.00 | 0.86 | 0.00 | 0.81 | -10.67 | 113.85 | -56.54 | 105.29 | 0.8521 | 301.0 | 260.6 | |
| 0.00 | 1.30 | 0.00 | 1.22 | -9.78 | 113.48 | -56.91 | 104.17 | 0.8536 | 396.0 | 362.3 | |
| 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. | |