The first NASA mission comprised of five different coordinated spacecraft, all five THEMIS spacecraft were launched from Cape Canaveral together aboard a single rocket on February 17, 2007. Eventually the five will study the mysterious eruptions in Earth's Northern and Southern Lights known as "substorms," but first they must achieve widely separated orbits, a process that will take several months.
An acronym for Time History of Events and Macroscopic Interactions during Substorms, THEMIS will obtain the evidence needed to solve what principal investigator Angelopoulos calls "a nagging question that the field has to resolve" — namely, competing theories about where auroral substorms originate in the magnetosphere.
As one of several instrument systems carried aboard the five THEMIS spacecraft, the solid-state telescopes will gather some of the most important evidence. The SSTs' job is to measure the energy distribution of electrons and ions (charged atoms and atomic nuclei) arriving at each spacecraft from different parts of the sky. To do this, the SSTs use custom-built silicon diode detectors made in Berkeley Lab's Microsystems Laboratory by Craig Tindall, Steve Holland, and Nick Palaio of the Engineering Division.
These large-area detectors have very thin contacts, only a few hundred angstroms thick. This allows them to detect electrons and ions with energies much lower than those that can be detected with standard silicon detectors, giving the SSTs the ability to cover a wide energy range, from high to low. But because the contacts are so thin, making a sufficient quantity of the large detectors posed a significant challenge.
Says Tindall, "Berkeley Lab's Microsystems Laboratory provided advanced equipment and processes in an ultraclean environment, enabling the fabrication of these detectors with high yield."
Tindall and Palaio made detectors for the IMPACT instrument suite aboard STEREO using the same process as the THEMIS detectors; these are currently returning data on energetic solar particles.
THEMIS is managed by NASA's Goddard Spaceflight Center Explorers office. For more information about auroras, the magnetosphere, and the scientific and technical aspects of THEMIS, visit SSL's site at http://themis.ssl.berkeley.edu/ and NASA's site at http://www.nasa.gov/mission_pages/themis/main/index.html.
Berkeley Lab is a U.S. Department of Energy national laboratory located in Berkeley, California. It conducts unclassified scientific research and is managed by the University of California. Visit our website at http://www.lbl.gov.
Paul Preuss | EurekAlert!
SF State astronomer searches for signs of life on Wolf 1061 exoplanet
20.01.2017 | San Francisco State University
Molecule flash mob
19.01.2017 | Technische Universität Wien
An important step towards a completely new experimental access to quantum physics has been made at University of Konstanz. The team of scientists headed by...
Yersiniae cause severe intestinal infections. Studies using Yersinia pseudotuberculosis as a model organism aim to elucidate the infection mechanisms of these...
Researchers from the University of Hamburg in Germany, in collaboration with colleagues from the University of Aarhus in Denmark, have synthesized a new superconducting material by growing a few layers of an antiferromagnetic transition-metal chalcogenide on a bismuth-based topological insulator, both being non-superconducting materials.
While superconductivity and magnetism are generally believed to be mutually exclusive, surprisingly, in this new material, superconducting correlations...
Laser-driving of semimetals allows creating novel quasiparticle states within condensed matter systems and switching between different states on ultrafast time scales
Studying properties of fundamental particles in condensed matter systems is a promising approach to quantum field theory. Quasiparticles offer the opportunity...
Among the general public, solar thermal energy is currently associated with dark blue, rectangular collectors on building roofs. Technologies are needed for aesthetically high quality architecture which offer the architect more room for manoeuvre when it comes to low- and plus-energy buildings. With the “ArKol” project, researchers at Fraunhofer ISE together with partners are currently developing two façade collectors for solar thermal energy generation, which permit a high degree of design flexibility: a strip collector for opaque façade sections and a solar thermal blind for transparent sections. The current state of the two developments will be presented at the BAU 2017 trade fair.
As part of the “ArKol – development of architecturally highly integrated façade collectors with heat pipes” project, Fraunhofer ISE together with its partners...
19.01.2017 | Event News
10.01.2017 | Event News
09.01.2017 | Event News
20.01.2017 | Awards Funding
20.01.2017 | Materials Sciences
20.01.2017 | Life Sciences