Published December 30, 2019 | Version v1
Dataset Open

Simulation datasets for "Is Nightside Outflow Required to Induce Magntospheric Sawtooth Oscillations?"

Authors/Creators

  • 1. University of Hong Kong
  • 2. The Oliver J. Brambles, PhD
  • 3. National Center for Atmospheric Research
  • 4. Dartmouth College

Description

Processed simulation data for "Is Nightside Outflow Required to Induce Magntospheric Sawtooth Oscillations?"

"OpenFlux_sawtooth.mat" is the time series of the integrated open magnetic flux in the cusp O+ outflow simulation.

"tiltangle.mat" is the time evolution of magnetic inclination angle extracted at geostationary orbit for comparing the spatial extension of sawtooth substorms with observations from Cai et al. [2006].

 

Notes

The full simulation data (in the form of hdf4) are preserved at the NCAR Cheyenne supercomputer system (DOI:10.5065/D6RX99HX) and is available through the leading author of the paper.

Files

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md5:dfb4ad9cf89c02e5fc47c0ec6df6865c
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