Dataset for: Statistical properties of meso-scale plasma flows in the nightside high-latitude ionosphere
Authors/Creators
- 1. UCLA
- 2. Boston University, UCLA
- 3. University of Calgary
- 4. University of Texas at Arlington
Description
This dataset is a compilation of statistical results from Gabrielse et al. [2018] (https://doi.org/10.1029/2018JA025440). If you would like to use the dataset, please contact Christine Gabrielse (cgabrielse@ucla.edu, cgabrielse@gmail.com). Depending on how the results are used, the main authors request co-authorship on publications.
The following list describes the columns in each data file labeled, ***_FLOW-DATA-PCvsAO_YYYY.txt
Files named ***_FLOW-DATA-PCvsAO_YYYY_poleward.txt are for poleward-directed flows.
Each text file is for a different year (YYYY).
AO=auroral oval
PC=polar cap
time [YYYYMMDDhhmmss]
flagAO [-1=flow could not be observed. 0=flow could be observed, but was not. 1=flow was observed]
flagPC [-1=flow could not be observed. 0=flow could be observed, but was not. 1=flow was observed]
FWHMavg_AO [degrees]
FWHMkmavg_AO=[km]
longtestranges=[ignore]
Velmaxavg_AO=[m/s, actual average of max V in each range gate used]
VelmaxFITavg_AO=[m/s, determined from the Gaussian fits]
FWHMavg_PC=[degrees]
FWHMkmavg_PC=[km]
Velmaxavg_PC=[m/s, actual average of max V in each range gate used]
VelmaxFITavg_PC=[m/s, determined from the Gaussian fits]
;;For the bearings/orientation, see the orientation text files. The following four variables were calculated in a first step but are not
;;those used in the paper. They were not found with the strict selection criteria. Please do not use.
mbearingAO=[degrees in magnetic coordinates, a negative value is South of East (clockwise from East), a positive value is North of East (CC)]
mbearingPC=[degrees in magnetic coordinates, a negative value is South of East (clockwise from East), a positive value is North of East (CC)]
gbearingAO=[degrees in geographic coordinates, a negative value is South of East (clockwise from East), a positive value is North of East (CC)]
gbearingPC=[degrees in geographic coordinates, a negative value is South of East (clockwise from East), a positive value is North of East (CC)]
;;;;;;;;;;;;;;;
minlatAO=[degrees, min geographic latitude of the flow]
maxlatAO=[degrees, max geographic latitude of the flow]
minlatPC=[degrees, min geographic latitude of the flow]
maxlatPC=[degrees, max geographic latitude of the flow]
mltAO=[degrees (MLT)]
mltPC=[degrees (MLT)]
AE=[nT]
AL=[nT]
SYMH=[nT]
IMFBz=[nT]
IMFBy=[nT]
F107=[sfu]
The following list describes the columns in each data file labeled, ***_orientation_YYYY.txt
Files named ***_orientation_YYYY_poleward.txt are for poleward-directed flows.
Each text file is for a different year (YYYY).
The orientation was determined when enough bearings between RGs were available. See Gabrielse et al. [2018] for description.
https://doi.org/10.1029/2018JA025440
AO=auroral oval
PC=polar cap
time [YYYYMMDDhhmmss]
mbearingAO [degrees clockwise from magnetic North]
gbearingAO [degrees clockwise from geographic North]
mbearingPC [degrees clockwise from magnetic North]
gbearingPC [degrees clockwise from geographic North]
The following list describes the columns in each data file labeled, ***_SPEC_TEST_***_noRG1-2.txt
time [YYYYMMDDhhmmss]
RG [the range gate number at which the polar cap boundary was determined at RNK, or the auroral oval's equatorial boundary at SAS]
Files
README.txt
Files
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Additional details
Related works
- Is supplement to
- 10.1029/2018JA025440 (DOI)
References
- Gabrielse et al. [2018], https://doi.org/10.1029/2018JA025440