SDO HMI 2011-02-19 09:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 108.11 | 479.72 | 150.07 | 694.07 | -19.25 | 35.53 | 70.85 | 251.96 | 0.9379 | -34.5 | 74.4 | |
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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 | 0.86 | 0.00 | 1.42 | -16.65 | 38.46 | 73.78 | 254.68 | 0.9551 | 200.0 | 185.0 | |
| 0.60 | 2.06 | 1.00 | 3.44 | -17.31 | 38.71 | 74.02 | 253.99 | 0.9562 | 485.0 | 375.3 | |
| 5.32 | 185.90 | 9.48 | 314.73 | -18.53 | 39.94 | 75.25 | 252.67 | 0.9618 | -402.7 | 32.4 | |
| 11.25 | -3.00 | 19.60 | -3.00 | -18.52 | 39.54 | 74.86 | 252.70 | 0.9600 | 409.9 | 999999 | |
| 4.38 | -3.00 | 7.18 | -3.00 | -18.46 | 38.42 | 73.73 | 252.79 | 0.9546 | -368.5 | 999999 | |
| 13.22 | -3.00 | 21.26 | -3.00 | -18.44 | 38.06 | 73.37 | 252.82 | 0.9528 | 662.9 | 999999 | |
| 3.61 | 8.07 | 5.53 | 12.33 | -17.98 | 37.13 | 72.45 | 253.33 | 0.9481 | 466.4 | 508.2 | |
| 0.00 | 1.37 | 0.00 | 2.08 | -19.32 | 36.89 | 72.21 | 251.92 | 0.9467 | 379.0 | 313.8 | |
| 0.00 | 0.52 | 0.00 | 0.86 | -21.04 | 38.67 | 73.98 | 250.08 | 0.9555 | 308.0 | 259.3 | |
| 0.00 | 1.37 | 0.00 | 1.85 | -17.60 | 34.24 | 69.56 | 253.79 | 0.9318 | -270.0 | -178.5 | |
| 3.35 | 241.97 | 4.66 | 314.76 | -18.55 | 34.91 | 70.23 | 252.77 | 0.9357 | 640.6 | 138.6 | |
| 1.55 | -11.00 | 2.11 | -11.00 | -19.74 | 34.58 | 69.89 | 251.49 | 0.9337 | -185.4 | 999999 | |
| 1.03 | -11.00 | 1.41 | -11.00 | -19.96 | 34.61 | 69.92 | 251.26 | 0.9339 | -332.4 | 999999 | |
| 2.92 | -11.00 | 3.91 | -11.00 | -19.89 | 34.08 | 69.40 | 251.33 | 0.9307 | 358.0 | 999999 | |
| 9.10 | -11.00 | 11.48 | -11.00 | -19.28 | 32.56 | 67.87 | 251.98 | 0.9212 | -531.8 | 999999 | |
| 2.92 | -11.00 | 3.71 | -11.00 | -19.69 | 32.75 | 68.07 | 251.53 | 0.9225 | -398.7 | 999999 | |
| 2.15 | -11.00 | 2.77 | -11.00 | -20.52 | 33.18 | 68.50 | 250.63 | 0.9253 | 285.1 | 999999 | |
| 2.40 | -11.00 | 3.09 | -11.00 | -20.44 | 33.10 | 68.41 | 250.73 | 0.9247 | -273.6 | 999999 | |
| 2.32 | 3.26 | 2.80 | 3.95 | -18.62 | 31.44 | 66.75 | 252.68 | 0.9138 | -420.8 | -359.4 | |
| 13.91 | -11.00 | 17.33 | -11.00 | -20.03 | 32.21 | 67.53 | 251.15 | 0.9191 | -686.8 | 999999 | |
| 1.89 | -11.00 | 2.29 | -11.00 | -19.39 | 31.50 | 66.82 | 251.84 | 0.9143 | -593.0 | 999999 | |
| 0.00 | 0.86 | 0.00 | 1.10 | -21.02 | 32.96 | 68.28 | 250.09 | 0.9240 | -135.0 | -108.8 | |
| 6.70 | -11.00 | 8.39 | -11.00 | -20.49 | 32.37 | 67.69 | 250.66 | 0.9202 | 623.2 | 999999 | |
| 1.46 | -11.00 | 1.82 | -11.00 | -20.91 | 32.26 | 67.57 | 250.20 | 0.9195 | 223.8 | 999999 | |
| 0.00 | 1.03 | 0.00 | 1.25 | -20.64 | 31.59 | 66.91 | 250.48 | 0.9151 | -102.0 | -16.0 | |
| 2.40 | 3.43 | 2.99 | 4.26 | -21.43 | 32.08 | 67.40 | 249.62 | 0.9184 | -478.2 | -485.5 | |
| 0.00 | 0.77 | 0.00 | 0.96 | -22.13 | 32.08 | 67.40 | 248.86 | 0.9186 | -383.0 | -326.1 | |
| 1.72 | 1.97 | 2.04 | 2.34 | -21.95 | 30.84 | 66.16 | 249.02 | 0.9104 | -206.7 | -147.0 | |
| 0.00 | 0.69 | 0.00 | 0.77 | -20.56 | 29.12 | 64.44 | 250.48 | 0.8980 | -456.0 | -396.4 | |
| 2.40 | 4.98 | 2.80 | 5.78 | -22.07 | 30.32 | 65.64 | 248.86 | 0.9069 | -396.3 | -317.1 | |
| 9.62 | 16.49 | 10.34 | 17.69 | -20.90 | 27.94 | 63.25 | 250.04 | 0.8895 | -622.7 | -532.5 | |
| 1.89 | 2.23 | 2.08 | 2.46 | -21.99 | 28.66 | 63.98 | 248.86 | 0.8953 | -427.0 | -458.8 | |
| 0.00 | 1.89 | 0.00 | 2.04 | -21.96 | 28.05 | 63.37 | 248.85 | 0.8908 | -558.0 | -519.2 | |
| 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. | |