IVM Magnetograms
Each magnetogram is a 168 kbyte GIF image. Celestial north is at the top;
east is at the left. The magnetogram is displayed as four panels:
- Continuum brightness
- This is in arbitrary units, but on a linear scale.
- Line-of-sight component of magnetic field
- Projection of magnetic field vector onto the line between the solar feature
and the observer. The units are Gauss. The color changes linearly with the cube
root of the field strength, to better show both strong and weak features. Thus if
the top of the scale is 1000 = 10^3, the midpoint is 5^3 or 125.
- Transverse component of magnetic field
- Magnitude of the projection of the field vector onto the plane perpendicular to
the line of sight. The units are Gauss; cube-root scaling is used here too.
- Direction of transverse component
- The orientation of the transverse component is indicated by the pixel color,
as in the key wheel at the lower left. Note that there is a 180-degree ambiguity in
the direction: the polarization data does not tell us whether the field vector points
to the right or to the left.
AR9591_20010904.1724_ivm
AR9591_20010904.1724_ivm
AR9596_20010904.1702_ivm
AR9596_20010904.1702_ivm
AR9599_20010904.1719_ivm
AR9599_20010904.1719_ivm
AR9601_20010904.1657_ivm
AR9601_20010904.1657_ivm
AR9602_20010904.1713_ivm
AR9602_20010904.1713_ivm
AR9603_20010904.1708_ivm
AR9603_20010904.1708_ivm
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