Alternate Precipitation of Auroral Electrons and Ions by Bipolar Field-Aligned Electric Fields: Characteristic Events of Low-Altitude Reimei Observations
Authors/Creators
- 1. Nagoya University
- 2. Research Institute for Sustainable Humanosphere, Kyoto University
Description
This contains the original data used by the paper 'Alternate Precipitation of Auroral Electrons and Ions by Bipolar Field-Aligned Electric Fields: Characteristic Events of Low-Altitude Reimei Observations', which will appear in Geophysical Reseach Letters. The data were obtained by the Reimei satellite.
=====================================================================
EISA: electrostatic analyzer
[RE_ESA_*.sav (electrons), RE_ISA_*.sav (ions)]
=====================================================================
The file is in the IDL (Interactive Data Language) SAV format.IDL> restore,'RE_ESA_******.L2.sav' -- read sav fileIDL> help,eisa,/str
VERSION LONG 70317 -- version (not meaningful)
SENSOR INT 1 -- 1: ESA, -1: ISA
KSTEP DOUBLE Array[29] -- energy step [eV]
JS DOUBLE Array[12794] -- second from 2000/1/1 00:00:00UT
-- You can convert JS to year, month, day, and second of the day by the procedure JS2YMD in the JHU/APL/S1R library.
FLUX FLOAT Array[12794,22,29]
-- energy flux (time, pitch angle, energy)
-- [eV/cm2 s str eV]
PA FLOAT Array[12794,22] -- pitch angle [deg]
GAS_ERR LONG Array[12794]
-- 0: ok,
-- nonzero: magnetic field data unavailable
-- (calculation of pitch angle is unsuccessful)
KSTEPH DOUBLE Array[29]
-- higher energy boundary of energy bin in eV
KSTEPL DOUBLE Array[29]
-- lower energy boundary of energy bin in eV
As of 2025-02-16, the same data files are also available at https://reimei.isee.nagoya-u.ac.jp/sav/
=====================================================================
MAC: auroral camera
[RE_MAC*]
=====================================================================
printf,11,epoch
printf,11,format='(i4)',yy_obs
printf,11,format='(i2)',mo_obs
printf,11,format='(i2)',dd_obs
printf,11,format='(i2)',hhh
printf,11,format='(i2)',mmm
printf,11,format='(i2)',sss
printf,11,format='(i3)',msec
printf,11,format='(Z8)',ti
printf,11,format='(f7.2)',mac_t(n)
printf,11,format='(f7.2)',mac_1t(n)
printf,11,format='(f7.2)',mac_f1t(n)
printf,11,format='(i1)',imode
printf,11,format='(f7.2)',expos(n)
printf,11,format='(f7.2)',timres
printf,11,format='(i3)',quality
printf,11,glat(*,*,n,ch)
printf,11,glon(*,*,n,ch)
printf,11,format='(f10.4)',footlatn(n)
printf,11,format='(f10.4)',footlonn(n)
printf,11,format='(f10.4)',footaltn(n)
printf,11,format='(2i4)',footpixx1n(n),footpixy1n(n)
printf,11,format='(3f12.8)',footdirxn(n),footdiryn(n),footdirzn(n)
printf,11,image1(*,*)
where
epoch, yy_obs, mo_obs, dd_obs, hhh, mmm, sss, msec, ti represents the time of image data.
mac_t, mac_1t, mac_f1t are temperatures of imager elecgronics, CCD, and filter, respectively;
imode is an observation mode;
timres is a time interval of successive images;
quality is a data quality;
glat and glon are geographic latitudes and longitudes for each pixel of image;
footlatn, footlonn, footaltn are geographic latitude, longitude and altitude at footprint;
footpixx1n and footpixy1n are (x,y) pixel numbers in image correspond to the footprints;
footdirxy, footdiryn, foordirzn are the vector of foorprint direction in J2000 coordinate system;
image1(*,*) is an image data (usually 64x64 2-D array).
As of 2025-02-26, the same data files are also available at https://www.darts.isas.jaxa.jp/stp/data/index/Level-2/
=====================================================================
GAS: magentometer
[GAS_*]
=====================================================================
One line consists of 8 colums.
hh:mm:ss.sss dBn dBe dBd sigma(dBn) sigma(dBe) sigma(dBd) flag(1:MAC-on), where dBn, dBe, dBd are northward, eastward and downward, respectively.
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ET-20060729130611.png
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