| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 109.31 | 578.79 | 109.59 | 586.11 | -19.96 | 258.72 | -57.06 | 114.98 | 0.8717 | 317.2 | 3.1 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-07-01 09:00:40 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 | 1.54 | 0.00 | 1.32 | -23.66 | 266.76 | -49.03 | 121.94 | 0.8171 | 266.0 | 289.6 | |
| 0.00 | 1.09 | 0.00 | 0.97 | -21.94 | 264.36 | -51.43 | 119.02 | 0.8315 | 491.0 | 447.9 | |
| 2.82 | 200.80 | 2.54 | 190.28 | -21.28 | 263.30 | -52.48 | 117.89 | 0.8383 | 758.0 | -238.9 | |
| 10.36 | -3.00 | 9.39 | -3.00 | -21.06 | 263.09 | -52.69 | 117.56 | 0.8394 | 753.7 | 999999 | |
| 1.91 | -3.00 | 1.76 | -3.00 | -21.25 | 262.50 | -53.28 | 117.57 | 0.8449 | 484.6 | 999999 | |
| 0.00 | 1.73 | 0.00 | 1.66 | -22.67 | 261.32 | -54.47 | 118.75 | 0.8586 | -580.0 | -505.9 | |
| 10.18 | -3.00 | 9.49 | -3.00 | -21.27 | 261.99 | -53.79 | 117.42 | 0.8492 | 475.4 | 999999 | |
| 0.55 | 1.64 | 0.54 | 1.62 | -23.31 | 260.34 | -55.45 | 119.14 | 0.8679 | -522.8 | -451.8 | |
| 0.00 | 1.18 | 0.00 | 1.20 | -23.85 | 259.69 | -56.09 | 119.51 | 0.8742 | -409.0 | -323.6 | |
| 0.00 | 0.27 | 0.00 | 0.27 | -23.37 | 259.77 | -56.02 | 119.01 | 0.8724 | -513.0 | -488.0 | |
| 0.00 | 0.55 | 0.00 | 0.53 | -21.93 | 260.54 | -55.25 | 117.67 | 0.8626 | -509.0 | -470.8 | |
| 1.54 | -3.00 | 1.49 | -3.00 | -21.03 | 260.59 | -55.19 | 116.69 | 0.8598 | -836.4 | 999999 | |
| 0.00 | 0.82 | 0.00 | 0.81 | -22.16 | 259.88 | -55.91 | 117.71 | 0.8684 | -283.0 | -347.7 | |
| 0.00 | 1.36 | 0.00 | 1.34 | -21.68 | 260.04 | -55.74 | 117.24 | 0.8659 | -617.0 | -497.8 | |
| 7.00 | 12.90 | 6.64 | 12.25 | -20.02 | 260.91 | -54.88 | 115.67 | 0.8546 | -296.3 | -272.8 | |
| 12.90 | -3.00 | 12.59 | -3.00 | -21.25 | 260.18 | -55.61 | 116.80 | 0.8636 | -687.9 | 999999 | |
| 0.00 | 1.09 | 0.00 | 1.08 | -21.60 | 259.74 | -56.05 | 117.05 | 0.8680 | -279.0 | -295.9 | |
| 2.63 | 5.63 | 2.63 | 5.64 | -21.84 | 259.54 | -56.25 | 117.26 | 0.8702 | -309.3 | -120.5 | |
| 0.00 | 0.55 | 0.00 | 0.53 | -20.34 | 259.76 | -56.03 | 115.66 | 0.8647 | -322.0 | -333.8 | |
| 0.82 | 4.18 | 0.83 | 4.23 | -21.54 | 258.82 | -56.97 | 116.70 | 0.8749 | 315.1 | 61.4 | |
| 0.00 | 1.73 | 0.00 | 1.70 | -20.28 | 259.56 | -56.23 | 115.54 | 0.8661 | -460.0 | -354.7 | |
| 0.00 | 1.27 | 0.00 | 1.26 | -20.52 | 259.30 | -56.48 | 115.73 | 0.8687 | -496.0 | -291.3 | |
| 0.64 | 2.00 | 0.67 | 2.10 | -22.15 | 257.82 | -57.97 | 117.07 | 0.8837 | 519.7 | 453.9 | |
| 0.00 | 0.73 | 0.00 | 0.82 | -23.25 | 255.82 | -59.97 | 117.69 | 0.9001 | -428.0 | -379.9 | |
| 0.00 | 0.91 | 0.00 | 1.03 | -23.05 | 255.63 | -60.16 | 117.43 | 0.9010 | -261.0 | -221.0 | |
| 0.00 | 0.82 | 0.00 | 0.87 | -21.02 | 257.04 | -58.75 | 115.62 | 0.8869 | 320.0 | 282.2 | |
| 55.33 | 329.18 | 58.00 | 346.73 | -19.08 | 257.02 | -58.76 | 113.49 | 0.8830 | 720.3 | 149.1 | |
| 0.00 | 0.82 | 0.00 | 0.96 | -22.41 | 254.20 | -61.59 | 116.36 | 0.9093 | -295.0 | -245.9 | |
| 0.00 | 0.91 | 0.00 | 1.04 | -21.23 | 254.66 | -61.12 | 115.21 | 0.9040 | 307.0 | 294.8 | |
| 2.63 | 4.18 | 3.02 | 4.79 | -20.83 | 254.60 | -61.19 | 114.77 | 0.9037 | 365.8 | 183.1 | |
| 0.00 | 0.91 | 0.00 | 1.08 | -19.86 | 253.40 | -62.38 | 113.44 | 0.9101 | -351.0 | -373.0 | |
| 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. | |