Beaming up on the way to space

(麻豆淫院) -- Space may be the final frontier. But often a few trips to PML are necessary before things can get off the ground. One recent case in point is the test of an instrument called the Extreme Ultraviolet Monitor, which will soon be heading for Mars to help answer a vexing question in planetary science: Where did the Red Planet鈥檚 once-dense atmosphere go?
The obvious answer is: off into space. But why? And how? NASA鈥檚 Mars Atmosphere and Volatile Evolution mission (MAVEN for short), scheduled for launch in late 2013, will investigate possible causes for the depletion. To model that process, researchers need a detailed understanding of multiple dynamic factors, including what reactions result when sunlight and solar wind hit the Martian atmosphere; how the atmosphere was and is structured; which chemical species are relatively stable; and which are ejected into space at what rate. A data set of that scope will presumably allow planetary scientists to extrapolate backward to a time when Mars was a wetter world.
鈥淲e鈥檙e trying to understand what happens when sunlight and solar wind hit the atmosphere, as well as energetic particles from solar storms and solar flares,鈥 says MAVEN PI Bruce Jakosky of the University of Colorado鈥檚 Laboratory for Atmospheric and Space 麻豆淫院ics (LASP). 鈥淲e want to know what the upper atmospheric response is.鈥 An essential part of that research involves measuring the extreme ultraviolet flux. So the MAVEN researchers brought their EUV filter radiometer to NIST鈥檚 Synchrotron Ultraviolet Radiation Facility (SURF), under the auspices of the Ultraviolet Radiation Group in PML鈥檚 Sensor Science Division.
They spent a week characterizing the instrument鈥檚 performance at different wavelengths (1 nm to 7 nm, 17 nm to 22 nm, and the Lyman alpha spectral line at 121 nm), temperatures (5掳C to 25 掳C), radiation intensities, and orientations, all within a vacuum chamber at the end of a SURF beam line. Although other MAVEN sensors will examine other aspects of the Martian atmosphere, readings from the EUV filter radiometer 鈥 which sits in a housing the size of a beer can 鈥 will provide particularly significant input.
鈥淯V drives a lot of the key photochemical processes that result in ejection of volatiles into space,鈥 says Frank Eparvier, a LASP senior scientist who came to SURF for the testing. 鈥淏ut on the time scales of solar flares, for example, UV at the shortest wavelengths in our part of the solar system can change by a factor of 1000 over a few minutes. For Mars, we need to know how the UV input varies with time, exactly which wavelengths get absorbed by the atmosphere, how molecules break apart and recombine, and the role UV plays in the atmospheric temperature structure.鈥
Judging from its first week of tests, the instrument is up to the task. 鈥淲e鈥檝e been able to calibrate it within about 5 percent, which is very good for UV,鈥 Eparvier says. The unit will return to SURF one more time before launch for a second round of tests and calibrations. Then after mission launch and a 10-month trip to Mars, the arriving spacecraft will orbit the planet and begin collecting data that will help create an historical portrait painted in gases.
SURF offers exceptional capabilities for this and other space missions. 鈥淭he SURF spectrometer calibration beamline is unique in the sense that we combine a calculable ultraviolet source, operated in a clean and oil-free ultrahigh vacuum with a large vacuum chamber that can accommodate space instrumentation,鈥 says Uwe Arp, a physicist in PML鈥檚 Ultraviolet Radiation Group.
鈥淥f course, NASA maintains many very large vacuum chambers that can house whole spacecraft, but they don't have them combined with a calculable ultraviolet light source. In addition, SURF is optimized for the spectral range interesting to solar missions, namely the ultraviolet spectral region, whereas most other synchrotron light sources are optimized for x-ray operations. Furthermore, to effectively operate SURF as an absolute source, the storage ring has to be characterized very carefully and many operational parameters have to be monitored during operation, which is not routinely done at other synchrotron light sources.鈥
Meanwhile, in another part of PML, a very different kind of space testing is underway. In this case, a solar-panel manufacturer brings samples of solar cells intended for long-term deployment on various sorts of spacecraft in order to see if the cells can withstand the punishing torrent of charged particles that stream throughout the solar system.
鈥淲hat we do for them,鈥 says Fred Bateman of PML鈥檚 Radiation and Biomolecular 麻豆淫院ics Division, 鈥渋s we space-qualify their solar cells. They鈥檙e mainly concerned with electrons and heavy ions. That鈥檚 where they can incur the most damage. In a half an hour we can provide the electron fluence that they might encounter in Earth orbit in the course of decades.鈥
That鈥檚 a lot of electrons. But Bateman, who manages the small facility, has an ample supply 鈥 provided by a powerful Van de Graaff generator that sits directly above the test area. Electrons from the generator are accelerated downward and focused onto a waist-high platform about the size of a small serving tray. Arranged on the platform are several prototype high-efficiency solar cells about 4 cm2 in size, although larger wafer-type cells are also processed.
A motor moves the platform back and forth, and the beam sweeps across the samples. Mounted underneath the platform is a Faraday cup, centered on a small hole, which monitors the electron fluence incident on the samples. 鈥淭he direct current electron beam typically has an energy of 1 MeV,鈥 Bateman says, 鈥渁lthough customers sometimes request other energies.鈥 In general, the process entails exposing the samples to a range of electron fluences and then making a degradation curve from the data.
Beside radiation-hardness testing, the facility also conducts electron dosimetry studies and materials modification studies using the platform apparatus Bateman says he built for 鈥渁 couple thousand dollars鈥 using a stepper motor to move the platform and customized software that automates adjustments in the exposure regimen. 鈥淚n addition,鈥 Bateman says, 鈥渨e look at other applications. For example, I鈥檓 assisting groups at Penn State to develop transducer films from electroactive copolymers. In this case, the radiation can actually enhance the electromechanical response. They鈥檙e trying to find the right combination of materials.鈥 Transducers of this sort convert energy of motion into electrical signals, such as in sonar operations.
Ultraviolet sensors and solar cells are only two of the myriad devices that pass through PML on their way to space. Many more will be featured in future editions of PML at Work.
Provided by National Institute of Standards and Technology