FRANK McDONALD is a pioneer and world-renowned leader in space physics and cosmicray astrophysics. His career of more than 50 years began with James Van Allen at the University of Iowa. He has devoted much of this time to studies of galactic cosmic radiation, solar energetic particles, and planetary magnetospheres. With their experiments on Pioneer 10 and 11, McDonald and Van Allen gave us the first comprehensive close-up look of energetic particles trapped in the magnetospheres of Jupiter and Saturn. With his many space-borne instruments, McDonald explored vast regions of our solar system, from the orbit of Mercury with the twin Helios spacecraft to distances of over 100 astronomical units with the Voyager 1 and 2 spacecraft that have now entered a new frontier, the heliosheath beyond the solar wind termination shock. McDonald’s pioneering work began in the mid 1950s when he led two Rockoon (sounding rockets launched from balloons—a system invented by Van Allen) expeditions in 1954 and 1955 to study cosmic rays and what was then known as “soft radiation.” McDonald opened up the new area of cosmic ray astrophysics—being first to use a multi-parameter electronic detector system to determine both the atomic number and kinetic energy of individual nuclei of the primary cosmic rays.

Over the years, he has made definitive observational and interpretive studies of the energy spectra and elemental as well as isotopic composition of galactic cosmic radiation, the dependence of the intensity of this radiation on solar activity and on distance from the Sun, and of the composition, energy spectra, and propagation of energetic nuclei accelerated at the Sun and by shock waves in the heliosphere. He discovered co-rotating streams of energetic nuclei in the heliosphere beyond a few AU. He discovered quiet time fluxes of 3 to 12 MeV electrons. In the early 1970s he co-discovered a new component of low-energy cosmic rays with a highly unusual elemental composition, which he named “anomalous cosmic rays.” His subsequent discovery of anomalous cosmic ray N and Ne paved the way to our current understanding of the role of interstellar neutrals in the heliosphere. He discovered the important role of radially propagating merged interaction regions in modulating cosmic rays.

Still very active in his research, McDonald is focused on understanding the basic acceleration and transport processes of solar, anomalous and galactic cosmic rays. Using data from the two Voyager spacecraft, he is studying the dynamics of one of the last unexplored regions of our solar system, the regions close to the termination shock and the heliosheath.

Dr. McDonald served as chief of the Laboratory for High Energy Astrophysics at the NASA Goddard Space Flight Center, as NASA chief scientist, and as associate director/chief scientist at Goddard. Dr. McDonald made numerous important contributions to national and international activities in high-energy astrophysics, both by his own work and by his effective advocacy. He served as project scientist on nine NASA missions and was principal investigator on fifteen space experiments. Dr. McDonald is the author of more than 300 scientific publications and has written articles on space policy and space related subjects in Science and Physics Today. He served as chair or member on almost 35 committees and panels. He is a member of the National Academy of Sciences as well as the recipient of numerous honors and awards, among them the Lindsay Award and the Presidential Rank of Meritorious Excellence Award.



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FRANK McDONALD is a pioneer and world-renowned leader in space physics and cos- micray astrophysics. His career of more than 50 years began with James Van Allen at the University of Iowa. He has devoted much of this time to studies of galactic cosmic radia- tion, solar energetic particles, and planetary magnetospheres. With their experiments on Pioneer 10 and 11, McDonald and Van Allen gave us the first comprehensive close-up look of energetic particles trapped in the magnetospheres of Jupiter and Saturn. With his many space-borne instruments, McDonald explored vast regions of our solar system, from the orbit of Mercury with the twin Helios spacecraft to distances of over 100 astronomical units with the Voyager 1 and 2 spacecraft that have now entered a new frontier, the heliosheath beyond the solar wind termination shock. McDonald’s pioneering work began in the mid 1950s when he led two Rockoon (sounding rockets launched from balloons—a system invented by Van Allen) expeditions in 1954 and 1955 to study cosmic rays and what was then known as “soft radiation.” McDonald opened up the new area of cosmic ray astrophysics—being first to use a multi-parameter electronic detector system to determine both the atomic number and kinetic energy of individual nuclei of the primary cosmic rays. Over the years, he has made definitive observational and interpretive studies of the energy spectra and elemental as well as isotopic composition of galactic cosmic radiation, the dependence of the intensity of this radiation on solar activity and on distance from the Sun, and of the composition, energy spectra, and propagation of energetic nuclei accelerated at the Sun and by shock waves in the heliosphere. He discovered co-rotating streams of energetic nuclei in the heliosphere beyond a few AU. He discovered quiet time fluxes of 3 to 12 MeV electrons. In the early 1970s he co-discovered a new component of low-energy cosmic rays with a highly unusual elemental composition, which he named “anomalous cosmic rays.” His subsequent discovery of anomalous cosmic ray N and Ne paved the way to our current understanding of the role of interstellar neutrals in the heliosphere. He discovered the important role of radially propagating merged interaction regions in modulating cosmic rays. Still very active in his research, McDonald is focused on understanding the basic acceleration and transport processes of solar, anomalous and galactic cosmic rays. Using data from the two Voyager spacecraft, he is studying the dynamics of one of the last un- explored regions of our solar system, the regions close to the termination shock and the heliosheath. Dr. McDonald served as chief of the Laboratory for High Energy Astrophysics at the NASA Goddard Space Flight Center, as NASA chief scientist, and as associate direc- tor/chief scientist at Goddard. Dr. McDonald made numerous important contributions to national and international activities in high-energy astrophysics, both by his own work and by his effective advocacy. He served as project scientist on nine NASA missions and was principal investigator on fifteen space experiments. Dr. McDonald is the author of more than 300 scientific publications and has written articles on space policy and space related subjects in Science and Physics Today. He served as chair or member on almost 35 committees and panels. He is a member of the National Academy of Sciences as well as the recipient of numerous honors and awards, among them the Lindsay Award and the Presidential Rank of Meritorious Excellence Award.