{"@context":"http://schema.org","@type":"Dataset","@id":"https://doi.org/10.34691/FK2/ANOKLO","identifier":"https://doi.org/10.34691/FK2/ANOKLO","name":"Replicar los datos para: Ion and electron kappa-distribution functions along the plasma sheet - Time intervals data","creator":[{"@type":"Person","affiliation":{"@type":"Organization","name":"Universidad de Santiago de Chile"},"name":"Espinoza, C.M."},{"@type":"Person","affiliation":{"@type":"Organization","name":"Universidad de Santiago de Chile"},"name":"Stepanova, M."},{"@type":"Person","affiliation":{"@type":"Organization","name":"Universidad de Chile"},"name":"Moya, P.S"},{"@type":"Person","affiliation":{"@type":"Organization","name":"Lomonosov Moscow State University"},"name":"Antonova, E.E."},{"@type":"Person","affiliation":{"@type":"Organization","name":"Universidad de Chile"},"name":"Valdivia, J.A."}],"author":[{"@type":"Person","affiliation":{"@type":"Organization","name":"Universidad de Santiago de Chile"},"name":"Espinoza, C.M."},{"@type":"Person","affiliation":{"@type":"Organization","name":"Universidad de Santiago de Chile"},"name":"Stepanova, M."},{"@type":"Person","affiliation":{"@type":"Organization","name":"Universidad de Chile"},"name":"Moya, P.S"},{"@type":"Person","affiliation":{"@type":"Organization","name":"Lomonosov Moscow State University"},"name":"Antonova, E.E."},{"@type":"Person","affiliation":{"@type":"Organization","name":"Universidad de Chile"},"name":"Valdivia, J.A."}],"datePublished":"2019-06-20","dateModified":"2023-04-04","version":"1","description":"We use kappa distributions to model thousands of ion and electron flux spectra along the plasma sheet and analyze the variation of the spectral index κ and the temperature T in this region. We find that κ distributions are ubiquitous and fit well ion and electron flux spectra during quiet times, and during the expansion and recovery phases of substorms. Near Earth, and up to ∼12 RE, the κ indices are different than the rest of the plasma sheet, both for ions (κi) and electrons (κe). There is a significant dawn‐dusk asymmetry in κi toward the tail, which is enhanced during substorms. The ions also exhibit a permanent temperature asymmetry, determined by a colder dawnside. The whole tail becomes hotter during substorms, but it appears that most of the energy is deposited near Earth.","keywords":["Astronomía y astrofísica","Kappa distribution","Plasma sheet","electron spectrum","substorms","ion spectrum"],"citation":[{"@type":"CreativeWork","name":"Espinoza, C. M., Stepanova, M., Moya, P.S., Antonova, E.E., & Valdivia, J.A. (2018). Ion and electron kappa-distribution functions along the plasma sheet - Time intervals data. [Data set]","@id":"https://agupubs.onlinelibrary.wiley.com/doi/full/10.1029/2018GL078631","identifier":"https://agupubs.onlinelibrary.wiley.com/doi/full/10.1029/2018GL078631","url":"https://agupubs.onlinelibrary.wiley.com/doi/full/10.1029/2018GL078631"}],"license":"http://creativecommons.org/licenses/by/4.0","includedInDataCatalog":{"@type":"DataCatalog","name":"Repositorio de datos de investigación de la Universidad de Chile","url":"http://datos.uchile.cl"},"publisher":{"@type":"Organization","name":"Repositorio de datos de investigación de la Universidad de Chile"},"provider":{"@type":"Organization","name":"Repositorio de datos de investigación de la Universidad de Chile"},"distribution":[{"@type":"DataDownload","name":"MANIFEST.TXT","encodingFormat":"text/plain","contentSize":175,"@id":"https://doi.org/10.34691/UCHILE/ADTA9O/MKCTCF","identifier":"https://doi.org/10.34691/UCHILE/ADTA9O/MKCTCF","contentUrl":"http://datos.uchile.cl/api/access/datafile/51"},{"@type":"DataDownload","name":"README.TXT","encodingFormat":"text/plain","contentSize":753,"@id":"https://doi.org/10.34691/FK2/ANOKLO/SXFRGV","identifier":"https://doi.org/10.34691/FK2/ANOKLO/SXFRGV","contentUrl":"http://datos.uchile.cl/api/access/datafile/49"},{"@type":"DataDownload","name":"timesE.dat","encodingFormat":"text/x-fixed-field","contentSize":17694,"@id":"https://doi.org/10.34691/FK2/ANOKLO/B2SWDX","identifier":"https://doi.org/10.34691/FK2/ANOKLO/B2SWDX","contentUrl":"http://datos.uchile.cl/api/access/datafile/50"},{"@type":"DataDownload","name":"timesQ.dat","encodingFormat":"text/x-fixed-field","contentSize":165411,"@id":"https://doi.org/10.34691/FK2/ANOKLO/9CAOBV","identifier":"https://doi.org/10.34691/FK2/ANOKLO/9CAOBV","contentUrl":"http://datos.uchile.cl/api/access/datafile/53"},{"@type":"DataDownload","name":"timesR.dat","encodingFormat":"text/x-fixed-field","contentSize":12542,"@id":"https://doi.org/10.34691/FK2/ANOKLO/27YNZ6","identifier":"https://doi.org/10.34691/FK2/ANOKLO/27YNZ6","contentUrl":"http://datos.uchile.cl/api/access/datafile/52"}]}