An Observation Linking the Origin of Plasmaspheric Hiss to Discrete Chorus Emissions

Author:

Bortnik J.1,Li W.1,Thorne R. M.1,Angelopoulos V.2,Cully C.3,Bonnell J.4,Le Contel O.5,Roux A.5

Affiliation:

1. Department of Atmospheric and Oceanic Sciences, University of California, Los Angeles, CA 90095, USA.

2. Institute of Geophysics and Planetary Physics/Earth and Space Sciences, University of California, Los Angeles, CA 90095, USA.

3. Swedish Institute of Space Physics, Box 537, SE-751 21, Uppsala, Sweden.

4. Space Science Laboratory, University of California, Berkeley, CA 94720, USA.

5. Centre d'Etude des Environnements Terrestre et Planétaires, Velizy, France.

Abstract

Chorus Hissing Plasmaspheric hiss, a type of unstructured broadband, low-frequency radio emission, has long been known to exist in Earth's plasmasphere, but its origin has been uncertain. The source of hiss could be a different type of radio wave, called chorus, which originates outside the plasmasphere during geomagnetic storms. Both types of radio wave influence the behavior of energetic electrons in the near-Earth space environment, with implications for spacecraft and astronaut safety, but a correlation between the two has been difficult to establish experimentally. Recently, two of the five satellites of the THEMIS constellation were fortuitously able to record 4 minutes of electromagnetic wave data at high resolution during geomagnetically active conditions, detecting both chorus and hiss. An analysis of the data by Bortnik et al. (p. 775 ; see the Perspective by Santolik and Chum ) revealed that the two sets of waves were well correlated, with hiss lagging behind chorus as expected, implying that one indeed evolved into the other.

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

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