SDO HMI 2011-06-15 15:59:11 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!)
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 96.41 | 525.86 | 110.91 | 604.35 | 16.50 | 166.22 | -63.40 | 72.08 | 0.9007 | -118.1 | -2.4 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-06-15 15:59:11 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 |
| 27.01 | 275.52 | 26.94 | 276.65 | 17.14 | 170.55 | -59.06 | 70.78 | 0.8700 | -919.9 | -163.3 | |
| 20.75 | -1.00 | 20.84 | -1.00 | 16.50 | 170.25 | -59.36 | 71.55 | 0.8716 | -706.1 | 999999 | |
| 1.18 | -1.00 | 1.20 | -1.00 | 16.85 | 169.82 | -59.79 | 71.23 | 0.8755 | 130.8 | 999999 | |
| 0.00 | 0.54 | 0.00 | 0.58 | 16.48 | 168.33 | -61.29 | 71.88 | 0.8868 | -334.0 | -253.3 | |
| 0.00 | 1.00 | 0.00 | 1.04 | 14.81 | 168.85 | -60.77 | 73.68 | 0.8810 | -417.0 | -456.5 | |
| 0.00 | 1.09 | 0.00 | 1.14 | 14.93 | 168.59 | -61.02 | 73.58 | 0.8831 | -242.0 | -354.8 | |
| 0.00 | 6.62 | 0.00 | 8.49 | 18.67 | 163.32 | -66.30 | 70.15 | 0.9239 | 284.0 | 252.7 | |
| 1.63 | 3.53 | 1.90 | 4.12 | 15.29 | 165.50 | -64.12 | 73.56 | 0.9066 | -478.4 | -435.0 | |
| 1.54 | 1.72 | 1.79 | 2.00 | 14.35 | 165.44 | -64.18 | 74.61 | 0.9063 | -527.5 | -503.5 | |
| 1.63 | 2.08 | 1.95 | 2.49 | 15.19 | 164.75 | -64.87 | 73.76 | 0.9118 | -308.7 | -438.2 | |
| 7.34 | 68.43 | 9.73 | 91.42 | 18.21 | 162.45 | -67.17 | 70.75 | 0.9289 | 558.3 | 329.6 | |
| 0.00 | 7.98 | 0.00 | 10.21 | 16.78 | 163.10 | -66.51 | 72.21 | 0.9238 | 681.0 | 555.9 | |
| 6.34 | 57.64 | 7.79 | 71.53 | 14.80 | 163.99 | -65.63 | 74.27 | 0.9167 | -508.5 | -49.7 | |
| 0.00 | 0.82 | 0.00 | 1.04 | 16.05 | 163.20 | -66.42 | 72.99 | 0.9227 | 648.0 | 627.3 | |
| 0.00 | 3.90 | 0.00 | 5.00 | 16.27 | 162.97 | -66.65 | 72.78 | 0.9243 | 645.0 | 587.8 | |
| 3.26 | -11.00 | 4.38 | -11.00 | 17.40 | 162.07 | -67.55 | 71.66 | 0.9307 | 706.4 | 999999 | |
| 1.72 | -11.00 | 2.29 | -11.00 | 17.12 | 162.28 | -67.33 | 71.94 | 0.9292 | 668.4 | 999999 | |
| 0.00 | 1.81 | 0.00 | 2.48 | 17.97 | 161.62 | -68.00 | 71.10 | 0.9337 | 299.0 | 207.3 | |
| 0.00 | 4.35 | 0.00 | 6.05 | 18.22 | 161.24 | -68.38 | 70.87 | 0.9361 | -325.0 | -210.7 | |
| 0.00 | 1.63 | 0.00 | 2.11 | 15.98 | 162.76 | -66.86 | 73.11 | 0.9254 | 630.0 | 600.1 | |
| 1.54 | 2.72 | 1.97 | 3.48 | 15.48 | 163.01 | -66.60 | 73.63 | 0.9235 | 560.0 | 567.1 | |
| 3.35 | -11.00 | 4.57 | -11.00 | 17.20 | 161.63 | -67.99 | 71.92 | 0.9332 | 357.9 | 999999 | |
| 0.00 | 1.36 | 0.00 | 1.77 | 15.66 | 162.65 | -66.97 | 73.47 | 0.9260 | 529.0 | 487.7 | |
| 0.00 | 4.62 | 0.00 | 6.23 | 16.66 | 161.86 | -67.76 | 72.47 | 0.9315 | 525.0 | 366.8 | |
| 8.52 | 12.69 | 11.35 | 16.91 | 16.03 | 162.06 | -67.55 | 73.12 | 0.9298 | 530.7 | 279.4 | |
| 0.00 | 1.54 | 0.00 | 1.98 | 14.87 | 162.83 | -66.78 | 74.30 | 0.9243 | 532.0 | 442.9 | |
| 10.60 | 62.63 | 14.21 | 85.51 | 15.49 | 161.85 | -67.77 | 73.73 | 0.9308 | 552.3 | -10.0 | |
| 0.00 | 0.91 | 0.00 | 1.18 | 14.08 | 162.51 | -67.11 | 75.18 | 0.9259 | 398.0 | 295.2 | |
| 0.00 | 0.73 | 0.00 | 0.94 | 13.99 | 162.48 | -67.14 | 75.28 | 0.9260 | 368.0 | 317.8 | |
| 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. | |