Published March 9, 2022 | Version v1

2017 August Eclipse GITM simulation

  • 1. ROR icon NSF National Center for Atmospheric Research
  • 2. ROR icon The University of Texas at Arlington
  • 3. ROR icon Boston University

Contributors

Contact person:

  • 1. ROR icon NSF National Center for Atmospheric Research

Description

This data present GITM simulation results using different solar masks during the 2017 August Eclipse. Detailed descriptions of the masks used for the simulation can be found in Mrak et al. (2021) DOI: 10.1002/essoar.10509183.1.

Notes

Related Links

An EUV Model of Solar Eclipses using SDO-AIA Images and the Impacts on Ionosphere-Thermosphere System :

SpatioTemporal Characteristics

Longitude West Boundary: -180.0
Longitude East Boundary: 180.0
Latitude South Boundary: -90.0
Latitude North Boundary: 90.0

Temporal Range Start: 2017-08-20
Temporal Range End: 2017-08-21

Spatial Resolution: 2.5 degreesLongitude
Spatial Resolution: 1.25 degreesLatitude
Spatial Resolution: 0.33 scaleHeight

Temporal Resolution: 10.0 minute

Files

ReadMe.txt

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Additional details

Related works

Is cited by
Journal article: 10.1002/essoar.10509183.1 (DOI)

Dates

Valid
2017-08-20/2017-08-21