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Dataset . 2022
License: CC BY
Data sources: Datacite
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ZENODO
Dataset . 2022
License: CC BY
Data sources: ZENODO
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ZENODO
Dataset . 2022
License: CC BY
Data sources: Datacite
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FAST loss-cone electron precipitation database

Authors: Hatch, Spencer Mark;

FAST loss-cone electron precipitation database

Abstract

A FAST electron precipitation database derived from FAST EESA observations, covering beginning of mission (October 1996) through 2009. Number flux ('j') and energy flux ('je') moments are produced by integrating EESA measurements over all energies above 70 eV up to the EESA detector limit (30 keV), and over all pitch angles within the earthward portion of the loss cone (see references). ================================ EXPLANATION OF DATAFRAME COLUMNS ================================ 'j' : units of #/cm^2-s (ALL QUANTITIES ARE POSITIVE, WHERE I HAVE USED THE CONVENTION 'POSITIVE' == 'EARTHWARD') 'je' : units of mW/m^2 (ALL QUANTITIES ARE POSITIVE, WHERE I HAVE USED THE CONVENTION 'POSITIVE' == 'EARTHWARD') 'jerr' : units of #/cm^2-s (Number flux uncertainty, calculated using the Gershman et al (2015) method) 'jeerr' : units of mW/m^2 (Energy flux uncertainty, calculated using the Gershman et al (2015) method) 'orbit' : FAST orbit number 'alt' : FAST geodetic altitude, in km. (FAST altitude ranges from ~300-4180 km) 'apexmlt' : Magnetic local time in Apex-110 coordinates (see Laundal and Richmond (2016)) 'apexmlat' : Magnetic latitude in Apex-110 coordinates (see Laundal and Richmond (2016)) 'shadowRegion110' : Integer indicator of the region of the Earth's shadow that FAST's field-line footpoint at 110-km altitude lands ind. Takes on values [0,1,2], corresponding to ['Umbra','Penumbra','Sunlit']. Calculated by mapping FAST's location to 110-km altitude in Apex coordinates and then following the methodology of Jia et al. (2015). 'mono' = 0,1,2 : 'not monoenergetic','weak monoenergetic','strict monoenergetic' 'broad' = 0,1,2 : 'not broadband','weak broadband','strict broadband' 'diffuse' = 0,1 : 'not diffuse','diffuse' 'mono', ' broad', and 'diffuse' follow the Hatch et al. (2016) FAST adaptation of the Newell et al. (2009) classification scheme *NOTE: I do NOT force 'mono' and 'broad' to be exclusive categories! I consider it fine for precipitation to be identified as both 'broad' and 'mono' 'drop' : Boolean indicating whether a row should be dropped from the DataFrame ========== REFERENCES ========== Gershman, D. J., Dorelli, J. C., F.-Viñas, A., & Pollock, C. J. (2015). The calculation of moment uncertainties from velocity distribution functions with random errors. Journal of Geophysical Research A: Space Physics, 120(8), 6633–6645. https://doi.org/10.1002/2014JA020775 Hatch, S. M., Chaston, C. C., & LaBelle, J. (2016). Alfvén wave-driven ionospheric mass outflow and electron precipitation during storms. Journal of Geophysical Research: Space Physics, 121(8), 7828–7846. https://doi.org/10.1002/2016JA022805 Hatch, S. M., Labelle, J., Lotko, W., Chaston, C. C., & Zhang, B. (2017). IMF control of Alfvénic energy transport and deposition at high latitudes. Journal of Geophysical Research: Space Physics, 122(12). https://doi.org/10.1002/2017JA024175 Jia, X., Xu, M., Pan, X., & Mao, X. (2017). Eclipse Prediction Algorithms for Low-Earth-Orbiting Satellites. IEEE Transactions on Aerospace and Electronic Systems, 53(6), 2963–2975. https://doi.org/10.1109/TAES.2017.2722518 Laundal, K. M., & Richmond, A. D. (2016). Magnetic Coordinate Systems. Space Science Reviews, 1–33. https://doi.org/10.1007/s11214-016-0275-y Newell, P. T., Sotirelis, T., & Wing, S. (2009). Diffuse, monoenergetic, and broadband aurora: The global precipitation budget. Journal of Geophysical Research, 114, A09207. https://doi.org/http://dx.doi.org/10.1029/2009JA014326

{"references": ["Gershman, D. J., Dorelli, J. C., F.-Vi\u00f1as, A., & Pollock, C. J. (2015). The calculation of moment uncertainties from velocity distribution functions with random errors. Journal of Geophysical Research A: Space Physics, 120(8), 6633\u20136645.", "Hatch, S. M., Chaston, C. C., & LaBelle, J. (2016). Alfv\u00e9n wave-driven ionospheric mass outflow and electron precipitation during storms. Journal of Geophysical Research: Space Physics, 121(8), 7828\u20137846. https://doi.org/10.1002/2016JA022805", "Hatch, S. M., Labelle, J., Lotko, W., Chaston, C. C., & Zhang, B. (2017). IMF control of Alfv\u00e9nic energy transport and deposition at high latitudes. Journal of Geophysical Research: Space Physics, 122(12). https://doi.org/10.1002/2017JA024175", "Jia, X., Xu, M., Pan, X., & Mao, X. (2017). Eclipse Prediction Algorithms for Low-Earth-Orbiting Satellites. IEEE Transactions on Aerospace and Electronic Systems, 53(6), 2963\u20132975. https://doi.org/10.1109/TAES.2017.2722518", "Laundal, K. M., & Richmond, A. D. (2016). Magnetic Coordinate Systems. Space Science Reviews, 1\u201333. https://doi.org/10.1007/s11214-016-0275-y", "Newell, P. T., Sotirelis, T., & Wing, S. (2009). Diffuse, monoenergetic, and broadband aurora: The global precipitation budget. Journal of Geophysical Research, 114, A09207. https://doi.org/http://dx.doi.org/10.1029/2009JA014326"]}

Related Organizations
Keywords

FAST; Fast Auroral SnapShoT explorer; Electron precipitation; Auroral precipitation; Aurora; Magnetosphere-ionosphere transition region;

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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
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