His primary areas of investigation include Astrophysics, Solar flare, Astronomy, Flare and Line. His Astrophysics study frequently involves adjacent topics like Spectral line. His Solar flare research incorporates elements of Corona, Particle acceleration, Gamma ray, Chromosphere and Magnetic reconnection.
His work on Solar physics, Submillimeter Array and Spectroscopy as part of general Astronomy research is often related to Context, thus linking different fields of science. His Flare study integrates concerns from other disciplines, such as Plasma oscillation, Wavelength, Optics and Magnetic loop. His study in Line is interdisciplinary in nature, drawing from both Excited state and Far infrared.
Arnold O. Benz spends much of his time researching Astrophysics, Astronomy, Solar flare, Flare and Line. His Astrophysics study often links to related topics such as Spectral line. His work deals with themes such as Coronal mass ejection and Coronal loop, which intersect with Astronomy.
His research on Solar flare also deals with topics like
Arnold O. Benz focuses on Astrophysics, Astronomy, Line, Protostar and Submillimeter Array. The Astrophysics study which covers Spectral line that intersects with Spectroscopy. His work investigates the relationship between Astronomy and topics such as Spectrometer that intersect with problems in Gamma ray.
His Line research incorporates themes from Stars, Excitation temperature, Interstellar medium, Radiative transfer and Far infrared. His work carried out in the field of Protostar brings together such families of science as Radius, Luminosity, Low Mass and Outflow. His Flare study integrates concerns from other disciplines, such as Solar flare, Particle acceleration and Current sheet.
The scientist’s investigation covers issues in Astrophysics, Line, Astronomy, Spectral line and Protostar. Arnold O. Benz merges Astrophysics with Context in his research. His Line research includes themes of Radiative transfer, Far infrared and Molecular cloud.
His work on Submillimeter Array, Solar physics, Galaxy and Corona as part of general Astronomy research is frequently linked to Coronal plane, thereby connecting diverse disciplines of science. Arnold O. Benz studied Spectral line and Luminosity that intersect with Envelope. His Protostar research is multidisciplinary, incorporating elements of Excitation temperature, Low Mass, Outflow and Young stellar object.
This overview was generated by a machine learning system which analysed the scientist’s body of work. If you have any feedback, you can contact us here.
The Reuven Ramaty High-Energy Solar Spectroscopic Imager (Rhessi)
R. P. Lin;B. R. Dennis;G. J. Hurford;D. M. Smith.
Solar Physics (2003)
The Herschel-Heterodyne Instrument for the Far-Infrared (HIFI)
Th. de Graauw;Th. de Graauw;F. P. Helmich;T. G. Phillips;J. Stutzki.
Astronomy and Astrophysics (2010)
On coronal oscillations
B. Roberts;P. M. Edwin;A. O. Benz.
The Astrophysical Journal (1984)
RADIO EMISSION FROM SOLAR FLARES
T. S. Bastian;A. O. Benz;Dale Gary.
Annual Review of Astronomy and Astrophysics (1998)
Plasma Astrophysics: Kinetic Processes in Solar and Stellar Coronae
Arnold O. Benz.
Arnold O. Benz.
Water in Star-Forming Regions with the Herschel Space Observatory (WISH): Overview of key program and first results
E. F. van Dishoeck;L. E. Kristensen;A. O. Benz;E. A. Bergin.
arXiv: Astrophysics of Galaxies (2010)
Energy Distribution of Heating Processes in the Quiet Solar Corona
Säm Krucker;Säm Krucker;Arnold O. Benz.
The Astrophysical Journal (1998)
Millisecond Radio Spikes
A. O. Benz.
Solar Physics (1986)
X-ray/microwave relation of different types of active stars
Manuel Guedel;Arnold O. Benz.
The Astrophysical Journal (1993)
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