SDO HMI 2014-03-03 20:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 19.94 | 131.20 | 19.21 | 123.95 | -1.68 | 153.51 | 58.27 | 272.50 | 0.8524 | -454.4 | -180.6 | |
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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 | 1.04 | 0.00 | 1.01 | 1.13 | 154.32 | 59.07 | 275.62 | 0.8639 | -151.0 | -220.9 | |
| 19.94 | 111.53 | 19.21 | 107.59 | -1.66 | 154.27 | 59.03 | 272.41 | 0.8599 | -825.2 | -214.6 | |
| 0.00 | 0.60 | 0.00 | 0.57 | -0.18 | 153.55 | 58.30 | 274.24 | 0.8552 | -508.0 | -467.3 | |
| 0.00 | 0.69 | 0.00 | 0.63 | -2.58 | 152.67 | 57.43 | 271.57 | 0.8443 | 89.0 | 140.9 | |
| 0.00 | 0.60 | 0.00 | 0.55 | -1.30 | 152.00 | 56.76 | 273.18 | 0.8396 | -308.0 | -406.0 | |
| 0.00 | 0.26 | 0.00 | 0.23 | -0.75 | 151.83 | 56.58 | 273.87 | 0.8387 | -552.0 | -547.7 | |
| 0.00 | 1.64 | 0.00 | 1.47 | -2.43 | 151.78 | 56.54 | 271.88 | 0.8361 | -421.0 | -423.2 | |
| 0.00 | 3.80 | 0.00 | 3.31 | -1.55 | 150.51 | 55.27 | 273.13 | 0.8250 | -498.0 | -554.4 | |
| 0.00 | 0.35 | 0.00 | 0.30 | -2.99 | 150.22 | 54.98 | 271.44 | 0.8203 | -356.0 | -422.2 | |
| 0.00 | 1.38 | 0.00 | 1.16 | -2.07 | 149.19 | 53.95 | 272.71 | 0.8111 | 415.0 | 382.0 | |
| 0.00 | 1.55 | 0.00 | 1.24 | 2.58 | 145.95 | 50.71 | 279.15 | 0.7854 | 236.0 | 332.8 | |
| 0.00 | 1.81 | 0.00 | 1.40 | -2.82 | 145.29 | 50.05 | 272.40 | 0.7687 | 425.0 | 342.7 | |
| 0.00 | 1.55 | 0.00 | 1.19 | -2.98 | 145.16 | 49.92 | 272.21 | 0.7670 | 365.0 | 407.4 | |
| 0.00 | 2.42 | 0.00 | 1.85 | -2.82 | 144.97 | 49.72 | 272.45 | 0.7650 | 655.0 | 518.7 | |
| 0.00 | 1.29 | 0.00 | 0.98 | -3.16 | 144.53 | 49.28 | 272.07 | 0.7596 | 589.0 | 484.2 | |
| 0.00 | 0.69 | 0.00 | 0.47 | -6.92 | 138.70 | 43.45 | 267.60 | 0.6857 | 326.0 | 282.6 | |
| 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. | |