A SURVEY OF MAGNETIC WAVES EXCITED BY NEWBORN INTERSTELLAR He+ OBSERVED BY THE ACE SPACECRAFT AT 1 au

• Published in: The Astrophysical journal Vol. 830; no. 1; pp. 47 - 60
• Main Authors: Fisher, Meghan K., Argall, Matthew R., Joyce, Colin J., Smith, Charles W., Isenberg, Philip A., Vasquez, Bernard J., Schwadron, Nathan A., Skoug, Ruth M., Sokó, Justyna M., Bzowski, Maciej, Zurbuchen, Thomas H., Gilbert, Jason A.
• Format: Journal Article
• Language: English
• Published: Philadelphia The American Astronomical Society 10.10.2016; IOP Publishing; Institute of Physics (IOP)
• Subjects: Advanced Composition Explorer; ASTRONOMY AND ASTROPHYSICS; Astrophysics; Cyclotron frequency; Cyclotrons; heliospheric and magnetospheric physics; instabilities; Interstellar; Magnetic fields; magnetic fields; solar wind; Spacecraft; Sun: heliosphere; Turbulence; Variation; Wave energy; Wave power; waves
• ISSN: 0004-637X; 1538-4357; 1538-4357
• DOI: 10.3847/0004-637X/830/1/47

ABSTRACT We report observations of low-frequency waves at 1 au by the magnetic field instrument on the Advanced Composition Explorer (ACE/MAG) and show evidence that they arise due to newborn interstellar pickup He+. Twenty-five events are studied. They possess the generally predicted attributes: spacecraft-frame frequencies slightly greater than the He+ cyclotron frequency, left-hand polarization in the spacecraft frame, and transverse fluctuations with minimum variance directions that are quasi-parallel to the mean magnetic field. Their occurrence spans the first 18 years of ACE operations, with no more than 3 such observations in any given year. Thus, the events are relatively rare. As with past observations by the Ulysses and Voyager spacecraft, we argue that the waves are seen only when the background turbulence is sufficiently weak as to allow for the slow accumulation of wave energy over many hours.