SubAuroral Red Arc Generated by Inner Magnetosphere Heat Flux

This data repository contains necessary data files and plotting scripts that support Lin et al. SubAuroral Red Arc Generated by Inner Magnetosphere Heat Flux.

CIMI_HF_fig1.nc contains processed energetic H+ and O+ ion energy spectra measured by the HOPE instrument onboard RBSP-B satellite, and electron heat flux derived from the RBSP data and simulated by the Comprehensive Inner Magnetosphere Ionosphere model.
CIMI_HF_fig2.nc contains electron temperature, density, and red line 6300 A emission rate from TIEGCM simulation.
CIMI_HF_fig3.nc contains the 6300 A emission rate from two TIEGCM runs.

DOI

https://doi.org/10.5065/j1te-cq43

Temporal Range

2013-05-31 18:00:00 to 2013-06-02 00:00:00

Temporal Resolution

5.0 minute

Spatial Resolution

1.25 degreesLongitude
1.25 degreesLatitude

Related Links

N/A

GCMD Science Keywords

• Sun-Earth Interactions > Ionosphere/Magnetosphere Dynamics > Aurorae
• Sun-Earth Interactions > Ionosphere/Magnetosphere Dynamics > Geomagnetic Forecasts
• Sun-Earth Interactions > Ionosphere/Magnetosphere Dynamics > Ion Chemistry/Ionization
• Sun-Earth Interactions > Ionosphere/Magnetosphere Dynamics > Magnetic Storms

File Media Types

• application/x-netcdf
• image/png
• text/x-matlab

Support Contact

Dong Lin
UCAR/NCAR - High Altitude Observatory
ldong@ucar.edu

Data Curator

GDEX Curator
UCAR/NCAR - GDEX
gdex@ucar.edu

Credit

This work is supported by NASA DRIVE Science Center for Geospace Storms (CGS) under Grant 80NSSC22M0163, and Grants 80NSSC21K0008, 80NSSC21K1677, 80NSSC22K1635, and 80NSSC23K1055, and NASA Contract 80GSFC18C0061 to the University of Colorado, Boulder.

Legal Constraints

Creative Commons Attribution 4.0 International License.

Access Constraints

None

Full Metadata

DIF XML
ISO19139 XML
OAI DC
JSON-LD

Version History

1.0