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Title: Spatial structure and temporal evolution of energetic particle injections in the inner magnetosphere during the 14 July 2013 substorm event

Journal Article · · Journal of Geophysical Research. Space Physics
DOI:https://doi.org/10.1002/2014JA020872· OSTI ID:1212463
 [1];  [1];  [1];  [1]; ORCiD logo [2];  [3];  [1];  [4];  [5]; ORCiD logo [6];  [7]
  1. Johns Hopkins University Applied Physics Laboratory, Laurel, MD (United States)
  2. Los Alamos National Lab. (LANL), Los Alamos, NM (United States)
  3. The Aerospace Corporation, El Segundo, CA (United States). Space Sciences Department.
  4. Kyoto Univ., Kyoto (Japan). Data Analysis Center for Geomagnetism and Space Magnetism, Graduate School of Science.
  5. Japan Aerospace Exploration Agency, Tsukuba (Japan)
  6. Univ. of Colorado, Boulder, CO (United States). Cooperative Institute for Research in Environmental Sciences; National Oceanic and Atmospheric Administration, Boulder, CO (United States). National Geophysical Data Center.
  7. New Jersey Institute of Technology, Newark, NJ (United States). Center for Solar-Terrestrial Research.

Recent results by the Van Allen Probes mission showed that the occurrence of energetic ion injections inside geosynchronous orbit could be very frequent throughout the main phase of a geomagnetic storm. Understanding, therefore, the formation and evolution of energetic particle injections is critical in order to quantify their effect in the inner magnetosphere. We present a case study of a substorm event that occurred during a weak storm (Dst ~ –40 nT) on 14 July 2013. Van Allen Probe B, inside geosynchronous orbit, observed two energetic proton injections within 10 min, with different dipolarization signatures and duration. The first one is a dispersionless, short-timescale injection pulse accompanied by a sharp dipolarization signature, while the second one is a dispersed, longer-timescale injection pulse accompanied by a gradual dipolarization signature. We combined ground magnetometer data from various stations and in situ particle and magnetic field data from multiple satellites in the inner magnetosphere and near-Earth plasma sheet to determine the spatial extent of these injections, their temporal evolution, and their effects in the inner magnetosphere. Our results indicate that there are different spatial and temporal scales at which injections can occur in the inner magnetosphere and depict the necessity of multipoint observations of both particle and magnetic field data in order to determine these scales.

Research Organization:
Los Alamos National Lab. (LANL), Los Alamos, NM (United States)
Sponsoring Organization:
USDOE
Grant/Contract Number:
AC52-06NA25396
OSTI ID:
1212463
Journal Information:
Journal of Geophysical Research. Space Physics, Vol. 120, Issue 3; ISSN 2169-9380
Publisher:
American Geophysical UnionCopyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 41 works
Citation information provided by
Web of Science

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Cited By (6)

Butterfly pitch angle distribution of relativistic electrons in the outer radiation belt: Evidence of nonadiabatic scattering journal June 2015
Study of field-aligned current (FAC), interplanetary electric field component ( E y ), interplanetary magnetic field component ( B z ), and northward ( x ) and eastward ( y ) components of geomagnetic field during supersubstorm: STUDY OF FIELD-ALIGNED CURRENT (FAC) journal May 2017
Drift‐Dispersed Flux Dropouts of Energetic Electrons Observed in Earth's Middle Magnetosphere by the Magnetospheric Multiscale (MMS) Mission journal March 2019
Continent‐Wide R1/R2 Current System and Ohmic Losses by Broad Dipolarization‐Injection Fronts journal June 2019
Contribution of Bursty Bulk Flows to the Global Dipolarization of the Magnetotail During an Isolated Substorm journal November 2019
ERG observations of drift echoes during a unique period of the satellite mission journal February 2019

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