Weekly Report 18Feb2011 25Feb2011

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(MESSENGER Data Analysis Project)
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Time series analysis was done on the 31Dec2007 flare using MESSENGER XRS data. Abundances were measured for various elements over the course of the flare.
Time series analysis was done on the 31Dec2007 flare using MESSENGER XRS data. Abundances were measured for various elements over the course of the flare.
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[[File:Fe ni abundance.jpg|center|thumb|600px|]]
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[[File:Fe ni abundance.jpg|center|thumb|400px|]]
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[[File:Ca abundance.jpg|center|thumb|600px|]]
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[[File:Ca abundance.jpg|center|thumb|400px|]]
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[[File:Su abundance.jpg |center|thumb|600px|]]
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[[File:Su abundance.jpg |center|thumb|400px|]]
===RHESSI Pixon Albedo Imaging Test===
===RHESSI Pixon Albedo Imaging Test===
Calibrated eventlist files were created from maps consisting of a compact Gaussian source and an extended cosine cubed source. The total flux of the cosine cubed source was adjusted to different percentages of the total flux of the compact Gaussian source. Pixon and Clean images were made from each eventlist file. Using these images, plots were made of the flux as a function of the radial distance from the peak of the Gaussian source.
Calibrated eventlist files were created from maps consisting of a compact Gaussian source and an extended cosine cubed source. The total flux of the cosine cubed source was adjusted to different percentages of the total flux of the compact Gaussian source. Pixon and Clean images were made from each eventlist file. Using these images, plots were made of the flux as a function of the radial distance from the peak of the Gaussian source.
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[[File:Gaussian source cosine cubed.jpg|center|thumb|400px|]]

Revision as of 19:38, 1 March 2011

RHESSI Website Migration

The RHESSI Website Migration Project continued.

MESSENGER Data Analysis Project

Time series analysis was done on the 31Dec2007 flare using MESSENGER XRS data. Abundances were measured for various elements over the course of the flare.

Fe ni abundance.jpg
Ca abundance.jpg
Su abundance.jpg

RHESSI Pixon Albedo Imaging Test

Calibrated eventlist files were created from maps consisting of a compact Gaussian source and an extended cosine cubed source. The total flux of the cosine cubed source was adjusted to different percentages of the total flux of the compact Gaussian source. Pixon and Clean images were made from each eventlist file. Using these images, plots were made of the flux as a function of the radial distance from the peak of the Gaussian source.

Gaussian source cosine cubed.jpg
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