@article{bdf2456353c34a71b5296a3f4d723263,
title = "Response of the Ionosphere-Plasmasphere Coupling to the September 2017 Storm: What Erodes the Plasmasphere so Severely?",
abstract = "We report an extreme erosion of the plasmasphere arising from the September 2017 storm. The cold electron density is identified from the upper limit frequency of upper hybrid resonance waves observed by the Plasma Wave Experiment instrument onboard the Exploration of energization and Radiation in Geospace/Arase satellite. The electron density profiles reveal that the plasmasphere was severely eroded during the recovery phase of the storm and the plasmapause was located at L = 1.6–1.7 at 23 UT 8 September 2017. This is the first report of deep erosion of the plasmasphere (LPP < 2) with the in situ observation of the electron density. The degree of the severity is much more than what is expected from the relatively moderate value of the SYM-H minimum (−146 nT). We attempt to find a possible explanation for the observed severe depletion by using both observational evidence and numerical simulations. Our results suggest that the middle latitude electric field had penetrated from the high-latitude storm time convection for several hours. Such an unusually long-lasting penetration event can cause this observed degree of severity.",
author = "Yuki Obana and Naomi Maruyama and Atsuki Shinbori and Hashimoto, {Kumiko K.} and Mariangel Fedrizzi and Masahito Nos{\'e} and Yuichi Otsuka and Nozomu Nishitani and Tomoaki Hori and Atsushi Kumamoto and Fuminori Tsuchiya and Shoya Matsuda and Ayako Matsuoka and Yoshiya Kasahara and Akimasa Yoshikawa and Yoshizumi Miyoshi and Iku Shinohara",
note = "Funding Information: This work was supported by JSPS KAKENHI Grants 15H05815, 15H05747, and 16H04057. Science data of the ERG (Arase) satellite were obtained from the ERG Science Center operated by ISAS/JAXA and ISEE/Nagoya University, Japan (https://ergsc.isee.nagoya‐u.ac.jp/ index.shtml.en). The present study analyzed the PWE‐HFA v03.00, MGF v01.00, and orbit v01 data. The solar wind parameters are obtained from the NASA OMNI website (https://omni- web.gsfc.nasa.gov/). We acknowledge use of NASA/GSFC's Space Physics Data Facility's OMNIWeb service and OMNI data. The GNSS data collection and processing were performed with the NICT Science Cloud. The Receiver Independent Exchange Format (RINEX) data for the GNSS‐TEC pro cessing are provided by the following organizations: UNAVCO (ftp://data‐ out.unavco.org), DGRSDUT (http:// gnss1.tudelft.nl), Arecibo Observatory (http://www.naic.edu), CDDIS (ftp:// cddis.gsfc.nasa.gov), CHAIN (ftp:// chain.physics.unb.ca), CORS (ftp:// www.ngs.noaa.gov), GDAF (ftp://geo- daf.mt.asi.it), BKG (ftp://igs.bkg.bund. de), IGS (ftp://rgpdata.ign.fr), EUOLG (ftp://olggps.oeaw.ac.at), Geoscience Australia (ftp://ftp.ga.gov.au), IGSIGN (ftp://igs.ensg.ign.fr), KASI (ftp://nfs. kasi.re.kr), PNGA (http://www.geodesy.cwu.edu), IBGE (ftp://geoftp.ibge. gov.br), RGCL (ftp://ftp.itacyl.es), TNG (ftp://196.15.132.3), SOPAC (ftp://garner.ucsd.edu), NRC (ftp://wcda.pgc. nrcan.gc.ca), GEONET (ftp:// 163.42.5.1), HRAO (ftp://geoid.hartrao. ac.za), GRN (ftp://rinex.smartnetna. com), GNNZ (ftp://ftp.geonet.org.nz), RENAG (ftp://renag.unice.fr), SONEL (ftp://ftp.sonel.org), FRDN (ftp://www. crs.inogs.it), LINZ (ftp://apps.linz.govt. nz), ROB (ftp://gnss.oma.be), GOP (ftp://ftp.pecny.cz), RGE (ftp:// 62.99.86.141), RGNA (ftp://geodesia. inegi.org.mx), CENAT (ftp://www. cenat.ac.cr), INGV (ftp://bancadati2. gm.ingv.it), REP (ftp://158.49.61.10), SWSBM (ftp://ftp‐out.sws.bom.gov.au), CORS (ftp://meristemum.carm.es), AFREF (ftp://ftp.afrefdata.org), WHU (ftp://igs.gnsswhu.cn), TLALOCNET (ftp://tlalocnet.udg.mx), NCEDC (ftp:// www.ncedc.org), ODT (ftp://ftp.odot. state.or.us), SWEPOS (ftp://ftp.swepos-data.lm.se), EUREF (ftp://www.epncb. oma.be), IGG (ftp://ftp.glonass‐iac.ru), SUGAUR (ftp://eos.ntu.edu.sg), NMA (ftp://ftp.statkart.no), NERC (ftp:// 128.243.138.204), and ERGNSS (ftp:// ftp.geodesia.ign.es). The results presented in this paper rely on the data collected at Huancayo, San Juan, and Kanoya from INTERMAGNET and Davao from MAGDAS. The Funding Information: The operation of SuperDARN Hokkaido East and West radar is supported by Special Funds for Education and Research (Energy Transport Processes in Geospace); the Inter-university Upper atmosphere Global Observation Network (IUGONET) project of the Ministry of Education, Culture, Sports, Science and Technology of Japan; and MEXT/JSPS KAKENHI Grants 16H06286 and 18KK0099. The work of T. H. and Y. M. was partly done at the ERG Science Center operated by JAXA/ISAS and ISEE, Nagoya University, Japan. This work was supported by NASA grants (NNX16AB83G, NNX15AI91G, 80NSSC17K0720, 80NSSC17K0718, 80NSSC19K0084, 80NSSC19K0277), NSF grants (AGS-1452298, AGS-1552248), and AFOSR FA9550-18-1-0483. Publisher Copyright: {\textcopyright}2019. American Geophysical Union. All Rights Reserved.",
year = "2019",
month = jun,
doi = "10.1029/2019SW002168",
language = "English",
volume = "17",
pages = "861--876",
journal = "Space Weather",
issn = "1542-7390",
publisher = "American Geophysical Union",
number = "6",
}