Work Description

Title: Space Weather Modeling Framework simulations of ground magnetometer data Open Access Deposited

h
Attribute Value
Methodology
  • Used the Geospace configuration of the Space Weather Modeling Framework to simulate the coupled Magnetosphere-Ionosphere system and find virtual ground magnetometer results to compare with observed measurements.
Description
  • Provided are the resultant and processed data.
Creator
Depositor
  • qusai@umich.edu
Contact information
Discipline
Funding agency
  • National Aeronautics and Space Administration (NASA)
  • National Science Foundation (NSF)
Keyword
Resource type
Last modified
  • 11/18/2022
Published
  • 05/19/2022
Language
DOI
  • https://doi.org/10.7302/dkjd-1j05
License
To Cite this Work:
Al Shidi, Q., Pulkkinen, T. (2022). Space Weather Modeling Framework simulations of ground magnetometer data [Data set], University of Michigan - Deep Blue Data. https://doi.org/10.7302/dkjd-1j05

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Files (Count: 5; Size: 635 MB)

# Space Weather Modeling Framework simulations of ground magnetometer data

## PARAM.in

This is a template input file used to generate the simulations. You can find
SWMF [here](https://github.com/MSTEM-QUDA/SWMF). The configuration and commit
hash used was:

SWMF original master 2022-04-05 1f775416b

GM/BATSRUS original master 2022-05-13 386c592

GM/BATSRUS/srcBATL original master 2022-05-13 a9b2640

GM/BATSRUS/srcUserExtra original master 2022-05-06 d4b585f

IE/Ridley_serial original master 2022-05-04 6dc60d1

IM/RCM2 original master 2022-01-16 0f7beff

share original master 2022-05-09 f543b9b

util original master 2022-03-14 29c284c

## Data

Data files are tarred and xzipped. To untar run with this command: `tar -xvf`

## indeces.tar.xz

Space seperated files of minute global indeces of each simulated geomagnetic
storm.

### geo*.log Headers

it year mo dy hr mn sc msc Kp K_12 K_13 K_14 K_15 K_16 K_17 K_18 K_19 K_20 K_21 K_22 K_23 K_00 K_01 K_02 K_03 K_04 K_05 K_06 K_07 K_08 K_09 K_10 K_11 AL AU AE AO

`it` is the time step, followed by the time in UTC. Next follows the storm K
indeces and the Auroral Electroject indeces are the last 4. These are the
simulated results.

### log*.log

it year mo dy hr mn sc msc dt rho mx my mz p bx by bz pmin pmax dst_sm dstflx_R=3.0 cpcpn cpcps

`it` is the time step, followed by the time in UTC. `dt` is the delta time
step, used in this study is `dst_sm` which is the SYM-H simulated and `cpcpn`
which is the north cross polar cap potential.

## stations.tar.xz

Comma seperated files of minute station magnetometer data for all storms. The
file names are the station abbreviations. Please visit
[SuperMAG](https://supermag.jhuapl.edu/) for a more
information.

### Headers

Year,Month,Day,Hour,Min,Sec,BnObs,BeObs,BdObs,BnSim,BeSim,BdSim

The first six are the times in UTC. The last six are the magnetic perturbation
components North, East and Down for Observed (Magnetometer) and Simulated
(SWMF).

## station_stats.txt

Statistical derivations for each station in a space seperated file.

### Headers

station geolon geolat maglon maglat mean std p0 p25 p50 p75 p100 bn_mean bn_std bn_p0 bn_p25 bn_p50 bn_p75 bn_p100 skew hss_50 hss_200

The station abbreviation and geographic and geomagnetic longitudes and latitudes
are given. Following is the mean, standard deviation and percentile of the
errors in B_Horizontal. The same is repeated for B_North.

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