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Coronal Prediction for the August 21, 2017 Total Solar Eclipse

Final Prediction: Updated with Energized Magnetic Fields

Polarized Brightness (Newkirk Filter)
Log Polarized Brightness (Unsharp Masked)
Click on the images to see slideshow of larger versions

This is our final prediction of the solar corona for the August 21, 2017 total solar eclipse. Our XT S Red RED nt8271Ay
was posted on July 31, 2017. The above images show two versions of the predicted brightness of polarized white light in the corona. The left image shows an image processed to simulate what would be seen when using a "Newkirk" radially graded filter. The image on the right is the polarized brightness on a log scale, sharpened using an "Unsharp Mask" filter. These are two different attempts to approximate what the human eye might see during the solar eclipse.

The image below on the left shows a digital processing of the polarized brightness using a "Wavelet" filter to bring out the details in the image. The image on the right shows traces of selected magnetic field lines from the model. Additional details about the eclipse and our prediction model are given below.

Polarized Brightness (Wavelet Filtered)
Magnetic Field Lines
Click on the images to see slideshow of larger versions

These images are aligned so that terrestrial (geocentric) north is up. This is the view of the Sun that would be seen by an observer on Earth with a camera aligned so that vertical is toward the Earth's north pole. In the magnetic field line image, the Sun's surface shows the intensity of the radial component of the photospheric magnetic field. The brightest colors show the location of active regions (strong magnetic fields). Vans Unisex Adults hxkr1j0wU
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Volume-rendered Magnetic Squashing Factor Q
(Eclipse Day View)
Volume-rendered Magnetic Squashing Factor Q
(Movie with Rotating Q)
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The last set of images show a special visualization of the three-dimensional (3D) magnetic field. By tracing magnetic field lines at extremely high resolution, we can calculate a 3D map of the so-called magnetic squashing factor - a scientific measure designed to indicate the presence of complex structuring in the magnetic field. We then integrate the map along the line-of-sight, with special weightings to create a composite that resembles solar eclipse images. This is intended to highlight the inherent complexity of the Sun's magnetic field and its intimate connection to visible emission from the solar corona.

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