Physics
Optics
Scientist
Bristol, University, Bristol, England
Rutherford Appleton Laboratory, Chilton, Didcot, Oxon, OX110QX United Kingdom Science Department, Rutherford Appleton Laboratory, Oxfordshire, UK
Rutherford Appleton Laboratory, Oxfordshire OX11 0QX, England
Institute of Mathematical and Physical Sciences, University of Wales, Aberystwyth, UK
Rutherford Appleton Laboratory, Chilton, Didcot, Oxfordshire OX11 0QX, UK.
Rutherford Appleton Lab., Didcot
Rutherford Appleton Lab., Oxfordshire, UK
IMAPS, Aberystwyth University, Aberystwyth, United Kingdom; University, Institute of Mathematics and Physics, Aberystwyth, United Kingdom
Rutherford Appleton National Laboratory, Chilton Didcot, Oxfordshire, UK
University of Wales Aberystwyth, UK
Institute of Mathematical and Physical Sciences, University of Wales Aberystwyth
Rutherford Appleton Laboratory, England
Institute of Mathematical and Physical Sciences, University of Wales, Aberystwyth, Ceredigion, Wales, UK
Rutherford Appleton Laboratory, Chilton, UK
Rutherford Appleton Laboratory, Chilton, Didcot, Oxon, UK
Planets and Space Plasma Group, Rutherford Appleton Laboratory, Chilton, Oxon OX11 0QX, Didcot, UK
Aerospace Corp., Los Angeles, California 90009M.GrandeRutherford Appleton Laboratories, Chilton-Didcot, Great BritainB.WilkenMax-Planck-Institute for Aeronomy, Katelenburg-Lindau, Germany
Institute of Mathematics and Physics, Aberystwyth University
Institute of Mathematical and Physical Sciences, University of Wales Aberystwyth, Penglais, Aberystwyth, SY23 3BZ, Wales, UK
University of Wales, Aberystwyth, Ceredigion SY23 3BZ, Wales, UK
Rutherford Appleton Laboratory, Chilton, Didcot, OXO OX11 0QX United Kingdom Appleton, Laboratory, Chilton, didcot, OX OX11, OQX United Kingdom Appleton Laboratory, Ded
A comparison between ion characteristics observed by the POLAR and DMSP spacecraft in the high-latitude magnetosphere
A new view of solar wind structures: Combined interplanetary scintillation and STEREO HI studies of the inner solar wind
A Preliminary Comparison of the Frequency of Transient Lunar Phenomena with Routine Observations
A Quantitative Analysis of Lunar and Planetary Fluorescence Modelling
A solar storm observed from the Sun to Venus using the STEREO, Venus Express, and MESSENGER spacecraft
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