Skip to content Skip to navigation

Connexions

You are here: Home » Content » More Details on the Third Stage of the LF Algorithm

Navigation

Recently Viewed

This feature requires Javascript to be enabled.

More Details on the Third Stage of the LF Algorithm

Module by: C. Sidney Burrus. E-mail the author

User rating (How does the rating system work?)
Ratings

Ratings allow you to judge the quality of modules. If other users have ranked the module then its average rating is displayed below. Ratings are calculated on a scale from one star (Poor) to five stars (Excellent).

How to rate a module

Hover over the star that corresponds to the rating you wish to assign. Click on the star to add your rating. Your rating should be based on the quality of the content. You must have an account and be logged in to rate content.

:
(0 ratings)

Summary: The third stage of the Lindsey-Fox algorithm multiplies the factors back together to check with the original polynomial coefficients.

Note: Your browser may not currently support MathML. See our browser support page for additional details. You can always view the correct math in the PDF version.

Addendum: More details of the third (unfactor and deflation) stage

The deflation stage of the Lindsey-Fox program first separates the unique, polished candidate roots that were found by the grid search and polish stages into two sets, one, a set very, very near the unit circle and the other, a set containing the rest of them. Both groups are unfactored in the frequency domain by the rootSpectrum program. It takes each zero or root, rr size 12{r} {}, forms the associated first degree factor, (zr)(zr) size 12{ \( z - r \) } {}, and pads with zeros to a length which is a an appropriate power of 2; i.e. [1,-r,0,0,0,...]. The DFT's of these terms are computed and multiplied together to get the DFT of the coefficients of the candidate polynomial. Exception: if the degree is less than 500, Matlab's command “poly” is used to combine them. This is the second most time consuming part of the total program. The coefficients are calculated from the candidate zeros with the “ifft” command and compared to the original coefficients. If they are the same number, then the search and polish possibly found them all. If the polishing process says the roots are close and a comparison in the unfactoring process says the coefficients are close, then these are the two criteria for success.

If the grid search and polish stages did not find all of the zeros, the original polynomial is deflated by removing those zeros found from it. That is done by dividing the DFT of the coefficients of the original polynomial, point-by-point, by the DFT associated with the zeros away from the unit circle which are found by the rootSpectrum program (deflation in the frequency domain). This quotient polynomial is further deflated (this time in the coefficient domain) by deconvolving it with the inverse FFT of the DFT associated with the zeros very near the unit circle. The resulting new quotient polynomial is now the original polynomial with all of the zeros found by the grid search and polish stages removed from it. This, hopefully low degree, polynomial is factored with the Matlab “roots” function and polished, first against the quotient polynomial, then the original polynomial. These new candidate zeros are added to the set found by grid search and polish, their associated spectra multiplied by that found in the “unfactoring” function, then checked to see if there are enough and if their associated coefficients are close to the original coefficients. If the answer is yes to both, the factoring is finished. If there are too few zeros, deflation will be performed again. This is repeated until all of the zeros are found or until no new ones are found. If there are still too few, a new search grid is designed with a smaller cell size and started again in stage one.

The basic mathematics behind this program can be found here.

Content actions

Give Feedback:

E-mail the module author | Rate module ( How does the rating system work?)

Rating system

Ratings

Ratings allow you to judge the quality of modules. If other users have ranked the module then its average rating is displayed below. Ratings are calculated on a scale from one star (Poor) to five stars (Excellent).

How to rate a module

Hover over the star that corresponds to the rating you wish to assign. Click on the star to add your rating. Your rating should be based on the quality of the content. You must have an account and be logged in to rate content.

(0 ratings)

Download:

Add module to:

My Favorites (?)

'My Favorites' is a special kind of lens which you can use to bookmark modules and collections directly in Connexions. 'My Favorites' can only be seen by you, and collections saved in 'My Favorites' can remember the last module you were on. You need a Connexions account to use 'My Favorites'.

| A lens (?)

Definition of a lens

Lenses

A lens is a custom view of Connexions content. You can think of it as a fancy kind of list that will let you see Connexions through the eyes of organizations and people you trust.

What is in a lens?

Lens makers point to Connexions materials (modules and collections), creating a guide that includes their own comments and descriptive tags about the content.

Who can create a lens?

Any individual Connexions member, a community, or a respected organization.

What are tags? tag icon

Tags are descriptors added by lens makers to help label content, attaching a vocabulary that is meaningful in the context of the lens.

| External bookmarks