Determining the Mode, Frequency, and Azimuthal Wave Number of ULF Waves During a HSS and Moderate Geomagnetic Storm

Author:

Murphy Kyle R.1ORCID,Inglis Andrew R.2,Sibeck David G.3ORCID,Rae I. Jonathan4ORCID,Watt Clare E. J.5ORCID,Silveira Marcos6ORCID,Plaschke Ferdinand7ORCID,Claudepierre Seth G.8,Nakamura Rumi7ORCID

Affiliation:

1. Department of Astronomy; University of Maryland; College Park MD USA

2. Physics Department; Catholic University of America; Washington DC USA

3. NASA Goddard Space Flight Center, Space Weather Laboratory (674); Greenbelt MD USA

4. Department of Space and Climate Physics, Mullard Space Science Laboratory; University College London; London UK

5. Department of Meteorology; University of Reading; Reading UK

6. Universities Space Research Association; Columbia MD USA

7. Space Research Institute; Austrian Academy of Sciences; Graz Austria

8. Space Sciences Department; The Aerospace Corporation; El Segundo CA USA

Funder

National Aeronautics and Space Administration

Natural Environment Research Council

Science and Technology Facilities Council

NASA's Prime

JHU/APL

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Reference86 articles.

1. Electric and magnetic radial diffusion coefficients using the Van Allen Probes data;Ali;Journal of Geophysical Research: Space Physics,2016

2. A statistical study of PC 3-5 pulsations observed by the AMPTEICCE magnetic fields experiment 1. Occurrence distributions;Anderson;Journal of Geophysical Research,1990

3. Observation of chorus waves by the Van Allen Probes: Dependence on solar wind parameters and scale size;Aryan;Journal of Geophysical Research: Space Physics,2016

4. Neutral line model of substorms: Past results and present view;Baker;Journal of Geophysical Research,1996

5. The Magnetic Electron Ion Spectrometer (MagEIS) instruments aboard the Radiation Belt Storm Probes (RBSP) spacecraft;Blake;Space Science Reviews,2013

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