Observation of equatorial plasma bubbles by the airglow imager on ISS-IMAP
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- Material Type
- 記事
- Author/Editor
- Hiroyuki NakataAkira TakahashiToshiaki Takano
- Publication, Distribution, etc.
- Publication Date
- 2018-10-25
- Publication Date (W3CDTF)
- 2018-10-25
- Periodical title
- Progress in earth and planetary science
- No. or year of volume/issue
- 5(66)
- Volume
- 5(66)
- ISSN (Periodical Title)
- 2197-4284
- ISSN-L (Periodical Title)
- 2197-4284
- Text Language Code
- eng
- DOI
- 10.1186/s40645-018-0227-0
- Persistent ID (NDL)
- info:ndljp/pid/11190361
- Collection
- Collection (Materials For Handicapped People:1)
- Collection (particular)
- 国立国会図書館デジタルコレクション > 電子書籍・電子雑誌 > その他
- Acquisition Basis
- オンライン資料収集制度
- Date Accepted (W3CDTF)
- 2018-11-26T20:20:20+09:00
- Date Captured (W3CDTF)
- 2018-11-26
- Format (IMT)
- application/pdf
- Access Restrictions
- 国立国会図書館内限定公開
- Service for the Digitized Contents Transmission Service
- 図書館・個人送信対象外
- Availability of remote photoduplication service
- 可
- Periodical Title (URI)
- Periodical Title (Persistent ID (NDL))
- info:ndljp/pid/11018906
- Data Provider (Database)
- 国立国会図書館 : 国立国会図書館デジタルコレクション
- Summary, etc.
- Using 630 nm airglow data observed by an airglow imager on the International Space Station (ISS), the occurrence of equatorial plasma bubbles (EPBs) is studied. In order to examine the physical mechanisms in the boundary region between the Earth and the outer space, an ionosphere, mesosphere, upper atmosphere, and plasmasphere mapping (IMAP) mission had been conducted onboard the ISS since October 2012. The visible light and infrared spectrum imager (VISI) is utilized in the ISS-IMAP mission for nadir-looking observation of the earth’s atmospheric airglow. In this study, we automatically select EPBs according to the criterion for extracting the tilted dark lines from VISI data. Using the selected events, the dependence of the occurrence rate of EPBs is examined. There is no other report of the occurrence rate of EPBs using downward-looking visible airglow data (630 nm). In this result, the occurrence rate is high at all longitudes in the equinoctial seasons. In the solstice seasons, in contrast, the occurrence rate is very small especially in the Pacific and American sectors. This result is basically consistent with previous studies, e.g., those determined by plasma density data on DMSP satellites.During the June solstice in 2013, EPBs were observed in association with geomagnetic storms that occurred due to a southward turning of the IMF Bz. Using these events, we examined the storm-time features of the occurrence of EPBs in the Pacific-American sectors during the June solstice. In these sectors, where the occurrence rate of EPBs is very small during solstice seasons, some EPBs were observed in the peak and recovery phases of the storms. This result shows that the prompt penetration of electric fields causes the development of EPBs, in the data we analyzed, the geomagnetic storms did not inhibit the generation of EPB in the Pacific–American sectors.
- DOI
- 10.1186/s40645-018-0227-0
- Access Restrictions
- インターネット公開
- Rights (production)
- © The Author(s). 2018 This article is distributed under the terms of the Creative Commons Attribution 4.0 International License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted use, distribution, and reproduction in any medium, provided you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons license, and indicate if changes were made.
- Related Material (URI)
- Is Referenced By
- A study of equatorial plasma bubble structure using VHF radar and GNSS scintillations over the low-latitude regions
- References
- Ionospheric effects of major magnetic storms during the International Space Weather Period of September and October 1999: GPS observations, VHF/UHF scintillations, and in situ density structures at middle and equatorial latitudesIonospheric disturbances during the magnetic storm of 15 July 2000: Role of the fountain effect and plasma bubbles for the formation of large equatorial plasma density depletionsGeomagnetic conjugate observations of equatorial airglow depletionsEquatorial evening prereversal vertical drift and spread F suppression by disturbance penetration electric fieldsRadar observations of<i>F</i>region equatorial irregularitiesTime evolution and dynamics of equatorial backscatter plumes 1. Growth phaseAnalysis of the seasonal variations of equatorial plasma bubble occurrence observed from Haleakala, HawaiiThe ionospheric disturbance dynamoLong‐lasting disturbances in the equatorial ionospheric electric field simulated with a coupled magnetosphere‐ionosphere‐thermosphere modelPenetration of magnetospheric electric fields to the equator during a geomagnetic stormGlobal observations of the zonal drift speed of equatorial ionospheric plasma bubblesEffect of geomagnetic activity on equatorial radio VHF scintillations and spread <i>F</i>Effect of magnetic activity on plasma bubbles over equatorial and low-latitude regions in East AsiaSimulation study of penetration electric field effects on the low‐ to mid‐latitude ionosphereEquatorial F-region plasma depletion drifts: latitudinal and seasonal variationsDE 2 observations of morningside and eveningside plasma density depletions in the equatorial ionosphereResponse of the equatorial ionosphere at dusk to penetration electric fields during intense magnetic stormsStorm time equatorial plasma bubble zonal drift reversal due to disturbance Hall electric field over the Brazilian regionGlobal S4 index variations observed using FORMOSAT‐3/COSMIC GPS RO technique during a solar minimum yearDMSP observations of equatorial plasma bubbles in the topside ionosphere near solar maximumAbnormal evening vertical plasma drift and effects on ESF and EIA over Brazil‐South Atlantic sector during the 30 October 2003 superstormSeasonal-longitudinal variability of equatorial plasma bubblesInteraction between direct penetration and disturbance dynamo electric fields in the storm‐time equatorial ionosphereCoincident equatorial bubble detection by TIMED/GUVI and ROCSAT‐1Comparing plasma bubble occurrence rates at CHAMP and GRACE altitudes during high and low solar activityGeomagnetic control of equatorial plasma bubble activity modeled by the TIEGCM with <i>Kp</i>Occurrence of Equatorial Plasma Bubbles during Intense Magnetic StormsMagnetospheric disturbance induced equatorial plasma bubble development and dynamics: A case study in Brazilian sectorDetermination of low latitude plasma drift speeds from FUV imagesMidnight reversal of ionospheric plasma bubble eastward velocity to westward velocity during geomagnetically quiettime: Climatology and its model validationGlobal equatorial plasma bubble occurrence during the 2015 St. Patrick's Day stormAn analysis of the quiet time day‐to‐day variability in the formation of postsunset equatorial plasma bubbles in the Southeast Asian regionGravity wave initiation of equatorial spread F: A case studyA climatology of equatorial plasma bubbles from DMSP 1989–2004Longitudinal development of low‐latitude ionospheric irregularities during the geomagnetic storms of July 2004Longitudinal variability of annual changes in activity of equatorial spread <i>F</i> and plasma bubblesField‐aligned 777.4‐nm composite airglow images of equatorial plasma depletionsAn explanation for anomalous equatorial ionospheric electric fields associated with a northward turning of the interplanetary magnetic fieldEstimation of electron densities in the lower thermosphere from GUVI 135.6 nm tomographic inversions in support of SpreadFExIonospheric storm effects and equatorial plasma irregularities during the 17–18 March 2015 eventObservations of GPS ionospheric scintillations over Wuhan during geomagnetic stormsMonitoring of global ionospheric irregularities using the Worldwide GPS NetworkImaging Observation of the Earth's Mesosphere, Thermosphere and Ionosphere by VISI of ISS-IMAP on the International Space StationStorm-time magnetospheric currents inferred from mid-latitude geomagnetic field variations.Equatorial Ionospheric Scintillations and Zonal Irregularity Drifts Observed with Closely-Spaced GPS Receivers in Indonesia(<Special Issue>CPEA-Coupling Processes in the Equatorial Atmosphere)Occurrence characteristics of plasmabubble derived from global ground-based GPS receiver networks
- Data Provider (Database)
- 国立情報学研究所 : CiNii Research
- Original Data Provider (Database)
- 学術機関リポジトリデータベース雑誌記事索引データベースCrossrefCiNii Articles科学研究費助成事業データベース科学研究費助成事業データベース科学研究費助成事業データベース科学研究費助成事業データベース科学研究費助成事業データベースCrossref
- Bibliographic ID (NDL)
- 11190361
- NAID
- 120006546014
- DOI
- 10.15106/j00349.2011338818
- Related Material (URI)
- Data Provider (Database)
- 国立情報学研究所 : CiNii Research
- Original Data Provider (Database)
- Japan Link Center雑誌記事索引データベースCiNii Articles
- Bibliographic ID (NDL)
- 11190361
- NAID
- 40018928834