Derivation of Hemispheric Ionospheric Current Functions From Ground-Level Magnetic Fields
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https://zenodo.org/record/2538169
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资源简介:
These files provide the input and output data for the Figures shown in the paper "Derivation of
Hemispheric Ionospheric Current Functions From Ground-Level Magnetic Fields" by Daniel Weimer, published in the Journal of Geophysical Research, Space Physics, paper number 2018JA026191, doi:10.1029/2018JA026191
Two IDL program files and the original, PDF versions of the figures are included.
The data are provided as IDL "SAVE" files, readable in IDL with the "RESTORE" command. NetCDF
versions are included, readable with any NetCDF software library. These NetCDF files have the same
names as the ".xdr" files, except they have the extension ".nc". Scalar variables (length 1) are put
into the Global Attributes in these files.
The files in this archive are:
Figures:
Figure_1.PDF
Figure_2.PDF
Figure_3.PDF
Figure_4.PDF
Figure_5.PDF
Figure_6.PDF
IDL Programs:
spherical_cap_90_fits.pro : Routines for fitting magnetic field data on a hemispheric cap (90
degrees), using spherical harmonics having both internal and external sources (or external alone),
and functions for evaluating the results as equivalent currents, or the magnetic field components.
AllLegendre.pro : Required by spherical_cap_90_fits.pro, provides computations of Associated
Legendre Polynominals as arrays, for all combinations of l and m, up to Lmax and Mmax, as well as first derivatives.
Data Files:
Figures_1_2_3_4_dB_ModelData.xdr : Magnetic field values (output from the 2013 empirical model),
shown in Figure 1, and used to calculate the coefficients used to make Figures 2, 3, and 4.
Contents:
ALLLATS FLOAT = Array[8640] , array of latitude values, degrees
ALLMLTS FLOAT = Array[8640] , array of Magnetic Local Time (MLT) values, hours
DBNS FLOAT = Array[8640] , array of northward magnetic field values
DBES FLOAT = Array[8640] , array of eastward magnetic field values
DBVS FLOAT = Array[8640] , array of vertical (downward) magnetic field values
NLATS FLOAT = 180.000
NMLTS INT = 48
empirical model inputs:
BT FLOAT = 10.0000 , magnitude of the IMF
ANGLE FLOAT = 180.000 , IMF clock angle
F107 FLOAT = 120.000 , F10.7 solar index
SWVEL FLOAT = 400.000 , solar wind velocity
TILTA FLOAT = 0.00000 , dipole tilt angle
Figures_2_3_4_SCHA90FitResults.xdr : The coefficients obtained from the fits, used to generate
Figures 2, 3, and 4.
Contents:
SPHCE DOUBLE = Array[115] , external spherical harmonic coefficients
SPHCI DOUBLE = Array[115] , interal spherical harmonic coefficients
NOINT_SPHCE DOUBLE = Array[115] , external spherical harmonic coefficients,
derived without using the internal terms in the fitting of the magnetic potential
The following variables are documented in the IDL program spherical_cap_90_fits.pro:
MAXL INT = 34
MAXM INT = 3
ODD INT = 1
EVEN INT = 0
CSIZE INT = 115
LS INT = Array[115]
MS INT = Array[115]
AB BYTE = Array[115]
Figures_3_4_dB_ModelData-Dst.xdr : Magnetic field values, after subtraction of the ring current
magnetic field, used to calculate the coefficients to make Figures 3 and 4.
Contents: Same variables as in file Figures_1_2_3_4_dB_ModelData.xdr
Figures_3_4_SCHA90FitResults-Dst.xdr : The coefficients obtained from fitting the magnetic field
that had the ring current subtracted, used to make Figures 3, and 4.
Contents: Same variables as in file Figures_2_3_4_SCHA90FitResults.xdr
Figure_5_dB_ModelDataTilt3x-Dst.xdr : eight sets of magnetic field values, after subtraction of the
ring current magnetic field, used to calculate the coefficients to generate Figure 5.
Contents: Similar variables as in file Figures_1_2_3_4_dB_ModelData.xdr, except that TILTA is
replaced by TILTS, an array with the eight dipole tilt angles. The magnetic field values are
replaced by these arrays:
DBN3X FLOAT = Array[180, 48, 3] , northward magnetic field, eight sets
DBE3X FLOAT = Array[180, 48, 3] , eastward magnetic field, eight sets
DBV3X FLOAT = Array[180, 48, 3] , vertical magnetic field, eight sets
Figure_5_SCHA90FitResultsTilt3x-Dst.xdr : eight sets of coefficients obtained from fitting the
magnetic field, used to make Figure 5.
Contents: Same variables as in file Figures_2_3_4_SCHA90FitResults.xdr, except for these arrays:
SPHCE3X DOUBLE = Array[115, 3] , external spherical harmonic coefficients, eight sets
SPHCI3X DOUBLE = Array[115, 3] , internal spherical harmonic coefficients, eight sets
Figure_6_dB_ModelDataClock8x-Dst.xdr : Eight sets of magnetic field values, after subtraction of
the ring current magnetic field, used to calculate the coefficients to generate Figure 6.
Contents: Similar variables as in file Figures_1_2_3_4_dB_ModelData.xdr, except that ANGLE is
replaced by ANGLES, an array with the eight IMF clock angles. The magnetic field values are
replaced by these arrays:
DBN8X FLOAT = Array[180, 48, 8] , northward magnetic field, eight sets
DBE8X FLOAT = Array[180, 48, 8] , eastward magnetic field, eight sets
DBV8X FLOAT = Array[180, 48, 8] , vertical magnetic field, eight sets
Figure_6_SCHAFitResultsClock8x-Dst.xdr : Eight sets of coefficients obtained from fitting the
magnetic field, used to make Figure 6.
Contents: Same variables as in file Figures_2_3_4_SCHA90FitResults.xdr, except for these arrays:
SPHCE8X DOUBLE = Array[115, 8] , external spherical harmonic coefficients, eight sets
SPHCI8X DOUBLE = Array[115, 8] , internal spherical harmonic coefficients, eight sets
创建时间:
2020-01-21



