
READ ME File for: Dataset for "Numerical Study of a Novel Monolithic Heat Exchanger for Electrothermal Space Propulsion"

Dataset DOI: 10.5258/SOTON/D0633

ReadMe Author: Federico Romei, University of Southampton

This dataset supports the publication:
AUTHORS			Federico Romei and Angelo Grubisic
TITLE			Numerical Study of a Novel Monolithic Heat Exchanger for Electrothermal Space Propulsion
JOURNAL			submitted to Acta Astronautica
PAPER DOI 		-


This dataset contains:

Data supporting the figures as follows:

Fig.4-i			Electrical resistivity of selected materials for the STAR resistojet heater. The materials in analysis are highlighted in orange.
				i = 1 (Inconel 718); i = 2 (AISI 316); i = 3 (Re); i = 4 (Ta); i = 5 (W)		
Fig.7-i			Specific impulse efficiency optimisation for the three cases in analysis, as function of the diverging angle of the nozzle.
				i = 1 (Inconel 718); i = 2 (Ta); i = 3 (Re);	
Fig.11-Ii*		Ignition of STAR-Inc from cold gas stationary solution. Maximum structural temperature (solid line) and Xe stagnation temperature at the inlet of the nozzle (dashed line) are shown at four current levels. The MOT of Inconel 718 is represented with a horizontal dashed line.
				i = 1 (I=17.6A); i = 2 (I=24.4A); i = 3 (I=29.7A); i = 4 (I=34.2A)		
Fig.12-top-Ii*		Ignition of STAR-Ta (top) and of STAR-Re (bottom) from cold gas stationary solution. Maximum structural temperature (solid line) and Xe stagnation temperature at the inlet of the nozzle (dashed line) are shown at four current levels. The MOT of the two materials are represented with a horizontal dashed line.
Fig.12-bottom-Ii*	Ignition of STAR-Ta (top) and of STAR-Re (bottom) from cold gas stationary solution. Maximum structural temperature (solid line) and Xe stagnation temperature at the inlet of the nozzle (dashed line) are shown at four current levels. The MOT of the two materials are represented with a horizontal dashed line.
Fig.13-i*		Bang-bang heating cycle of STAR-Inc with two current levels corresponding to about 25 W and 50 W of electrical power.
				i = 1 (top subfigure); i = 2 (bottom subfigure)

*Data at actual time steps taken by the solver.

Information about geographic location of data collection: University of Southampton, U.K.

Federico Romei
Astronautics Research Group
University of Southampton
f.romei@soton.ac.uk

Date that the file was created: May 2018