SDO HMI 2014-11-01 02:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.14 | 27.03 | 5.14 | 17.65 | -16.79 | 99.81 | -34.90 | 122.62 | 0.6498 | 227.5 | 196.0 | |
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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 | 1.13 | 0.00 | 0.70 | -16.91 | 104.11 | -30.60 | 125.94 | 0.6039 | -749.0 | -623.1 | |
| 0.00 | 1.04 | 0.00 | 0.65 | -16.37 | 102.42 | -32.29 | 123.81 | 0.6191 | 668.0 | 549.8 | |
| 0.52 | 2.60 | 0.33 | 1.63 | -15.87 | 102.37 | -32.34 | 123.06 | 0.6163 | 982.3 | 827.1 | |
| 2.86 | 4.42 | 1.80 | 2.78 | -16.15 | 102.28 | -32.43 | 123.40 | 0.6193 | 984.0 | 823.5 | |
| 0.00 | 1.21 | 0.00 | 0.77 | -16.47 | 102.22 | -32.49 | 123.80 | 0.6222 | 589.0 | 564.5 | |
| 4.76 | 9.35 | 3.01 | 5.91 | -16.04 | 101.93 | -32.78 | 122.97 | 0.6225 | 834.6 | 588.5 | |
| 0.00 | 1.04 | 0.00 | 0.66 | -16.12 | 101.66 | -33.05 | 122.87 | 0.6261 | 548.0 | 442.2 | |
| 0.00 | 0.95 | 0.00 | 0.64 | -15.63 | 97.00 | -37.71 | 119.05 | 0.6761 | -638.0 | -537.6 | |
| 0.00 | 0.78 | 0.00 | 0.55 | -18.52 | 94.63 | -40.08 | 121.38 | 0.7175 | -584.0 | -433.2 | |
| 0.00 | 0.87 | 0.00 | 0.62 | -18.26 | 93.54 | -41.16 | 120.43 | 0.7273 | -487.0 | -395.9 | |
| 0.00 | 1.13 | 0.00 | 0.84 | -19.54 | 91.78 | -42.93 | 121.05 | 0.7515 | -546.0 | -473.8 | |
| 0.00 | 0.78 | 0.00 | 0.59 | -19.72 | 91.55 | -43.16 | 121.14 | 0.7547 | -521.0 | -475.3 | |
| 0.00 | 1.73 | 0.00 | 1.31 | -19.47 | 91.24 | -43.47 | 120.69 | 0.7565 | -198.0 | -216.1 | |
| 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. | |