Published October 2008 | Version v1
Journal article

Mass spectrometric study of various coated targets utilizing the PUPR Mirror/Cusp plasma machine for the NASA Solar Probe space mission

  • 1. Plasma Engineering Laboratory, Polytechnic University of Puerto Rico, San Juan, PR 00918 (Puerto Rico)

Description

The NASA Solar Probe space mission will be a historic operation, flying for the first time into one of the last unexplored regions of the solar system, the Sun's atmosphere or corona; hopefully revolutionizing our knowledge of the physics of the origin and evolution of the solar wind phenomenon. The spacecraft's most prominent feature is the thermal protection system (TPS), composed of a large carbon-carbon conical shield, designed to withstand the Sun's violent temperatures. Thermal testing will be conducted on various coatings on the carbon-carbon targets in order to study mass loss components using mass spectrometry. Mass spectrometry is an analytical technique used to measure the mass-to-charge ratio of ions. It is more generally used to find the composition of a physical sample by generating a mass spectrum representing the masses of sample components. By using a quadrupole mass spectrometer, the effects of plasma on various coated targets were analyzed and the effects of various gases on the plasma were studied on the PUPR Mirror/Cusp (M/C) plasma machine. A series of five tests was performed for this experiment; the first four tests consist of creating plasma with four different gases, and studying the effects of each gas on the plasma using mass spectrometry, in order to decide which plasma resembles the Sun's atmosphere or corona. The fifth test consists of introducing various coated targets, which represent the spacecraft's shield, inside the PUPR M/C plasma machine, to study how the different coatings react with the plasma that best bears a resemblance to the Sun's atmosphere, for approximately 12 h of exposure. After studying the results for the first four tests, it is evident that each gas has a distinctive effect on the plasma. For the fifth test following the study of the mass spectrometry results, it is clear that the quadrupole mass spectrometer was able to detect mass loss components for the introduced targets, and the presence of the coatings were successfully identified inside the PUPR M/C plasma machine, therefore assisting in the shield coating selection for the solar probe aircraft.

Availability note (English)

Available from http://dx.doi.org/10.1088/0031-8949/2008/T131/014049

Additional details

Publishing Information

Journal Title
Physica Scripta (Online)
Journal Volume
2008
Journal Issue
T131
Journal Page Range
[4 p.]
ISSN
1402-4896

Conference

Title
12. Latin American workshop on plasma physics
Dates
17-21 Sep 2007
Place
Caracas (Venezuela, Bolivarian Republic of)

INIS

Country of Publication
United Kingdom
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
41041680
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Resource subtype / Literary indicator
Conference
Descriptors DEI
CARBON; CUSPED GEOMETRIES; MASS SPECTRA; MASS SPECTROMETERS; MASS SPECTROSCOPY; PLASMA; SOLAR SYSTEM; SOLAR WIND; SUN; THERMAL TESTING
Descriptors DEC
ELEMENTS; MAGNETIC FIELD CONFIGURATIONS; MAIN SEQUENCE STARS; MATERIALS TESTING; MEASURING INSTRUMENTS; NONDESTRUCTIVE TESTING; NONMETALS; OPEN CONFIGURATIONS; SOLAR ACTIVITY; SPECTRA; SPECTROMETERS; SPECTROSCOPY; STARS; STELLAR ACTIVITY; STELLAR WINDS; TESTING