Relative and (maybe) Absolute RHESSI Detector Efficiency: 2002-2008

From RHESSI Wiki

(Difference between revisions)
Jump to: navigation, search
(New page: {{Infobox Nugget |name = Nugget |title = Nugget Details |number = 117 |first_author = Jim McTiernan |publish_date = 21 December 2009 |next_nugget = TBD |previous_nugget = [[A tiny whit...)
Line 10: Line 10:
== Introduction ==
== Introduction ==
-
 
+
[[Image:97_jmm_Spd2006_fig1.png|400px|thumb|left|'''Figure 1''':This is the RHESSI 3 to 6 keV count rate for one orbit. The black dashed lines show an interval which was chosen for a temperature measurement. The red line is the expected background level.]]
[[Category:Nugget]]
[[Category:Nugget]]

Revision as of 22:38, 21 December 2009


Nugget
Number: 117
1st Author: Jim McTiernan
2nd Author:
Published: 21 December 2009
Next Nugget: TBD
Previous Nugget: A tiny white-light flare
List all



Introduction

Figure 1:This is the RHESSI 3 to 6 keV count rate for one orbit. The black dashed lines show an interval which was chosen for a temperature measurement. The red line is the expected background level.
Personal tools
Namespaces
Variants
Actions
Navigation
Toolbox