GOES Flux vs STIX counts - Revision history

Hualin at 10:29, 21 January 2022

2022-01-21T10:29:42Z

2022-01-21T09:18:55Z

2022-01-21T08:22:43Z

2022-01-21T08:22:21Z

2022-01-21T08:19:48Z

2022-01-21T08:00:18Z

2022-01-20T20:22:51Z

2022-01-20T16:11:31Z

2022-01-20T14:19:04Z

2022-01-20T14:18:39Z

← Older revision		Revision as of 10:29, 21 January 2022
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−	[[File:~~Goes bkg~~.png \|600px\|thumb\|none\| An example of estimated GOES flux background. ]]	+	[[File:Goes_background.png \|600px\|thumb\|none\| An example of estimated GOES flux background. ]]

@@ Line 1: / Line 1: @@
-[[File:Goes stix scatter polynomial 1oder v2.png|800px|thumb|none|  Scatter plot of STIX counts (4 - 10 keV) versus GOES background subtracted flux and   as well as a linear fit and a polynomial fit to the data.   ]]
+[[File:Goes stix flux fit lms.png|800px|thumb|none|  Scatter plot of STIX counts (4 - 10 keV) versus GOES and   as well as a linear fit and a polynomial fit to the data.   ]]
 The GOES flux of a solar flare is estimated using<br>
 flux=10^(p0+p1*x), <br>

← Older revision		Revision as of 08:22, 21 January 2022
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−	[[File:Goes bkg.png \|~~400px~~\|thumb\|none\| An example of estimated GOES flux background. ]]	+	[[File:Goes bkg.png \|600px\|thumb\|none\| An example of estimated GOES flux background. ]]

@@ Line 1: / Line 1: @@
-[[File:Goes stix scatter polynomial 1oder v2.png|800px|thumb|none|  Scatter plot of STIX counts (4 - 10 keV) versus GOES flux and   as well as a linear fit and a polynomial fit to the data.   ]]
+[[File:Goes stix scatter polynomial 1oder v2.png|800px|thumb|none|  Scatter plot of STIX counts (4 - 10 keV) versus GOES background subtracted flux and   as well as a linear fit and a polynomial fit to the data.   ]]
 The GOES flux of a solar flare is estimated using<br>
 flux=10^(p0+p1*x), <br>
@@ Line 7: / Line 7: @@
+[[File:Goes bkg.png |400px|thumb|none|  An example of estimated GOES flux background. ]]

@@ Line 1: / Line 1: @@
-[[File:Goes_stix_scatter_polynomial_2oder.png|800px|thumb|none|  Scatter plot of STIX counts (4 - 10 keV) versus GOES flux and   as well as a linear fit and a polynomial fit to the data.   ]]
+[[File:Goes stix scatter polynomial 1oder v2.png|800px|thumb|none|  Scatter plot of STIX counts (4 - 10 keV) versus GOES flux and   as well as a linear fit and a polynomial fit to the data.   ]]
 The GOES flux of a solar flare is estimated using<br>
 flux=10^(p0+p1*x), <br>

← Older revision		Revision as of 20:22, 20 January 2022
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	-->		-->
	[[File:Goes stix flux polynomial.png \|400px\|thumb\|none\| A polynomial fit to the data. Occulted flares were excluded. ]]		[[File:Goes stix flux polynomial.png \|400px\|thumb\|none\| A polynomial fit to the data. Occulted flares were excluded. ]]
		+
		+
		+	[[File:Goes bkg.png \|400px\|thumb\|none\| GOES flux background estimation using algorithm described <a href="https://root.cern.ch/doc/v608/classTSpectrum.html#a56e15d1c36c7557b17d5f6d68fa315a7">here</a> ]]

← Older revision		Revision as of 16:11, 20 January 2022
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		+	<!--
		+	The scatter plot can be also fitted with a polynomial function.
		+	-->
	[[File:Goes stix flux polynomial.png \|400px\|thumb\|none\| A polynomial fit to the data. Occulted flares were excluded. ]]		[[File:Goes stix flux polynomial.png \|400px\|thumb\|none\| A polynomial fit to the data. Occulted flares were excluded. ]]

← Older revision		Revision as of 14:19, 20 January 2022
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−	[[File:Goes stix flux polynomial.png \|~~800px~~\|thumb\|none\| A polynomial fit to the data. Occulted flares were excluded. ]]	+	[[File:Goes stix flux polynomial.png \|400px\|thumb\|none\| A polynomial fit to the data. Occulted flares were excluded. ]]

← Older revision		Revision as of 14:18, 20 January 2022
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−	[[File: Goes stix flux polynomial.png \|800px\|thumb\|none\| A polynomial fit to the data. Occulted flares were excluded. ]]	+	[[File:Goes stix flux polynomial.png \|800px\|thumb\|none\| A polynomial fit to the data. Occulted flares were excluded. ]]