Long Lifetime Hiss Rays in the Disturbed Plasmasphere

Author:

Wu Zhiyong123ORCID,Su Zhenpeng123ORCID,Zheng Huinan123ORCID,Wang Yuming123ORCID,Miyoshi Yoshizumi4ORCID,Shinohara Iku5ORCID,Matsuoka Ayako6,Kasahara Yoshiya7ORCID,Tsuchiya Fuminori8,Kumamoto Atsushi8,Matsuda Shoya7,Kasaba Yasumasa8,Teramoto Mariko9ORCID,Hori Tomoaki4ORCID

Affiliation:

1. Deep Space Exploration Laboratory/School of Earth and Space Sciences University of Science and Technology of China Hefei China

2. CAS Center for Excellence in Comparative Planetology/CAS Key Laboratory of Geospace Environment/Mengcheng National Geophysical Observatory University of Science and Technology of China Hefei China

3. Collaborative Innovation Center of Astronautical Science and Technology Harbin China

4. Institute for Space‐Earth Environmental Research Nagoya University Nagoya Japan

5. Institute of Space and Astronautical Science Japan Aerospace Exploration Agency Sagamihara Japan

6. Graduate School of Science Kyoto University Kyoto Japan

7. Graduate School of Natural Science and Technology Kanazawa University Kanazawa Japan

8. Graduate School of Science Tohoku University Sendai Japan

9. Graduate School of Engineering Kyushu Institute of Technology Kitakyushu Japan

Abstract

AbstractPlasmaspheric hiss waves are important to shape the Earth’s electron radiation belt. These waves are commonly envisioned to have a long lifetime which allows them to permeate the global plasmasphere from a spatially restricted source. However, this hypothesis has not been experimentally confirmed yet, because of the challenging observational requirements in terms of location and timing. With wave and particle measurements from five magnetospheric satellites and detailed modeling, we present the first report of long lifetime (∼42 s) hiss rays in the substorm‐disturbed plasmasphere. The low‐frequency hiss waves are found to originate from the middle piece of the plasmaspheric plume, bounce between two hemispheres, and eventually drift into the plasmaspheric core. These hiss rays can travel through ∼3 hr magnetic local time and ∼4 magnetic shell. Such a long‐time and large‐scale permeation of hiss rays could benefit from the ducting process by plasmaspheric field‐aligned density irregularities.

Publisher

American Geophysical Union (AGU)

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