Selecting Background for RHESSI Spectra

Options for choosing Background when fitting RHESSI Spectra

Introduction

Before a fit is done for a selected time interval using a RHESSI Spectrum file background must be selected. There are two types of background that need to be subtracted from RHESSI spectra. The preflare solar background and the non-solar background. The preflare background is the solar activity measured by RHESSI before a flare be gins or after it ends. The non-solar background is primarily due to cosmic-ray interactions with the spacecraft, the spacecraft passing through the South Atlantic Anomaly, or electron precipitation events from the outer radiation belt.

Methods for selecting Background

Using the same background for all fit intervals at all energy bands

This is the simplest method for selecting background. The basics are described in OSPEX Documentation. Background is selected by choosing a single time interval and using the spectrum as a function of energy during this interval as the background, The interval selected is usually during nighttime at the start or end of the RHESSI orbit. During these times RHESSI is measuring the non-solar background. The background defined by this time interval is subtracted from all intervals before fitting. Note that this background is constant. It does not change as a function of time. It is assumed that the background remains the same regardless of what happens during the flare.

The next step in complexity when selecting background is to select multiple background intervals. The intervals are selected in the same manner as above. The advantage of selecting multiple intervals is it gives a better idea of how the background changes over the course of the flare if the background intervals are far enough apart in time. For example background intervals can be selected during nighttime at the start of the orbit and nighttime at the end of the orbit. The OSPEX background selection GUI allows the user to select the order of the polynomial used to model background. In cases were a single interval is selected this should be left at the 0Poly option. This means that a zeroth order polynomial is used to fit the background spectrum then subtracted from all intervals fit, otherwise small timescale variations in the background time interval can cause large errors in the background. When selecting more than one time interval a zeroth order polynomial can still be used. In this case the background from each interval is fit with a zeroth order polynomial then the two are averaged to get the overall background. However when the intervals selected are far enough apart in time a first order polynomial (1Poly) can be used to fit the background as well. This fit gives a better idea of how the background changes as a function of time. Examples of both types of background selections are shown below.

A zero order polynomial fit to the background. The two nighttime intervals at the start and end of orbit were selected (top panel). A first order polynomial fit to the background. The same time intervals were selected as in the above panel (lower panel).

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