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The LMSAL team is part of Lockheed Martin Space Systems and has close affiliations with NASA and the solar physics group at Stanford University. Located in Palo Alto, California , LMSAL is involved in many ground- and space-based missions that study the Sun , with a sharp focus on basic research into understanding and predicting space weather ...
Multi-slit Solar Explorer. The Multi-slit Solar Explorer (MUSE) is a future NASA mission to study the heating of the solar corona and the impact of solar eruptions and flares that are at the foundation of space weather. MUSE will have two instruments, a multi-slit extreme ultraviolet (EUV) spectrograph and an EUV context imager. The satellite ...
Interface Region Imaging Spectrograph (IRIS), [1] also called Explorer 94 and SMEX-12, [2] is a NASA solar observation satellite. The mission was funded through the Small Explorer program to investigate the physical conditions of the solar limb, particularly the interface region made up of the chromosphere and transition region.
Lockheed Martin Space Systems is now headquartered in Denver, but still does considerable operations from Sunnyvale. Also located near Sunnyvale is the main office of Lockheed Martin's space research and development group, the Advanced Technology Center (ATC), formerly the Lockheed Palo Alto Research Laboratory (LPARL).
At the SOT focal plane, the Focal Plane Package (FPP) built by the Lockheed Martin Solar and Astrophysics Laboratory in Palo Alto, California consists of three optical instruments: the Broadband Filter Imager (BFI) which produces images of the solar photosphere and chromosphere in six wide-band interference filters; the Narrowband Filter Imager ...
The Atmospheric Imaging Assembly (AIA), led from the Lockheed Martin Solar and Astrophysics Laboratory (LMSAL), provides continuous full-disk observations of the solar chromosphere and corona in seven extreme ultraviolet (EUV) channels, spanning a temperature range from approximately 20,000 Kelvin to in excess of 20 million Kelvin. The 12 ...
The Interface Region Imaging Spectrograph mission is a partnership with the Lockheed Martin Solar and Astrophysics Laboratory to understand the processes at the boundary between the Sun's chromosphere and corona. This mission is sponsored by the NASA Small Explorer program. [16]
Bart De Pontieu is a solar physicist who works at Lockheed Martin's Solar & Astrophysics Laboratory. He is known for his work on the dynamics and heating of the solar chromosphere, transition region and corona, [1] via both wave mechanisms [2] and nanoflares.