| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 10.93 | 0.00 | 6.92 | -19.99 | 69.87 | -34.03 | 120.27 | 0.5955 | 220.2 | 179.8 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-01-07 12:00:24 UT
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 | 1.10 | 0.00 | 0.61 | -19.26 | 83.33 | -20.57 | 129.30 | 0.4304 | 809.0 | 611.8 | |
| 0.00 | 1.10 | 0.00 | 0.61 | -19.29 | 83.16 | -20.74 | 129.14 | 0.4327 | 719.0 | 605.9 | |
| 0.00 | 0.85 | 0.00 | 0.46 | -13.53 | 82.80 | -21.10 | 116.46 | 0.3927 | -738.0 | -584.7 | |
| 0.00 | 0.76 | 0.00 | 0.45 | -20.78 | 74.58 | -29.32 | 123.30 | 0.5500 | 709.0 | 558.0 | |
| 0.00 | 0.51 | 0.00 | 0.31 | -20.33 | 73.26 | -30.64 | 121.60 | 0.5633 | 788.0 | 608.2 | |
| 0.00 | 2.29 | 0.00 | 1.38 | -21.09 | 72.90 | -31.00 | 122.56 | 0.5724 | 658.0 | 588.8 | |
| 0.00 | 1.27 | 0.00 | 0.78 | -20.89 | 71.57 | -32.33 | 121.35 | 0.5872 | 562.0 | 464.8 | |
| 0.00 | 1.10 | 0.00 | 0.70 | -13.91 | 65.84 | -38.06 | 107.61 | 0.6301 | -572.0 | -394.5 | |
| 0.00 | 1.10 | 0.00 | 0.91 | -23.47 | 52.63 | -51.27 | 116.71 | 0.8033 | -237.0 | -283.2 | |
| 0.00 | 0.85 | 0.00 | 0.71 | -23.18 | 52.38 | -51.52 | 116.28 | 0.8049 | -496.0 | -434.4 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
|
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. |
||
| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
|
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. |
||
| 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. | |