Deutsch
 
Datenschutzhinweis Impressum
  DetailsucheBrowse

Datensatz

DATENSATZ AKTIONENEXPORT
  Ionospheric Plasma Density Oscillation Related to EMIC Pc1 Waves

Kim, H., Shiokawa, K., Park, J., Miyoshi, Y., Miyashita, Y., Stolle, C., Kim, K., Matzka, J., Buchert, S., Fromm, T., Hwang, J. (2020): Ionospheric Plasma Density Oscillation Related to EMIC Pc1 Waves. - Geophysical Research Letters, 47, 15, e2020GL089000.
https://doi.org/10.1029/2020GL089000

Item is

Dateien

einblenden: Dateien
ausblenden: Dateien
:
5002770.pdf (Verlagsversion), 7MB
Name:
5002770.pdf
Beschreibung:
-
Sichtbarkeit:
Öffentlich
MIME-Typ / Prüfsumme:
application/pdf / [MD5]
Technische Metadaten:
Copyright Datum:
-
Copyright Info:
-
Lizenz:
-

Externe Referenzen

einblenden:

Urheber

einblenden:
ausblenden:
 Urheber:
Kim, Hyangpyo1, Autor
Shiokawa, Kazuo1, Autor
Park, Jaeheung1, Autor
Miyoshi, Yoshizumi1, Autor
Miyashita, Yukinaga1, Autor
Stolle, Claudia2, Autor              
Kim, Khan‐Hyuk1, Autor
Matzka, J.2, Autor              
Buchert, Stephan1, Autor
Fromm, Tanja1, Autor
Hwang, Junga1, Autor
Affiliations:
1External Organizations, ou_persistent22              
22.3 Geomagnetism, 2.0 Geophysics, Departments, GFZ Publication Database, Deutsches GeoForschungsZentrum, ou_146030              

Inhalt

einblenden:
ausblenden:
Schlagwörter: EMIC Pc1 wave; ULF wave; compressional mode; plasma density; oscillation; swarm satellite; proton precipitation
 Zusammenfassung: We report the first observation of plasma density oscillations coherent with magnetic Pc1 waves. Swarm satellites observed compressional Pc1 wave activity in the 0.5–3 Hz band, which was coherent with in situ plasma density oscillations. Around the Pc1 event location, the Antarctic Neumayer Station III (L ~ 4.2) recorded similar Pc1 events in the horizontal component while NOAA‐15 observed isolated proton precipitations at energies above 30 keV. All these observations support that the compressional Pc1 waves at Swarm are oscillations converted from electromagnetic ion cyclotron (EMIC) waves coming from the magnetosphere. The magnetic field and plasma density oscillate in‐phase. We compared the amplitudes of density and magnetic field oscillations normalized to background values and found that the density power is much larger than the magnetic field power. This difference cannot be explained by a simple magnetohydrodynamic (MHD) model, although steep horizontal/vertical gradients of background ionospheric density can partly reconcile the discrepancy.

Details

einblenden:
ausblenden:
Sprache(n): eng - Englisch
 Datum: 2020-07-052020-05-242020-07-082020-08-032020
 Publikationsstatus: Final veröffentlicht
 Seiten: 11
 Ort, Verlag, Ausgabe: -
 Inhaltsverzeichnis: -
 Art der Begutachtung: Expertenbegutachtung
 Identifikatoren: DOI: 10.1029/2020GL089000
GFZPOF: p3 PT1 Global Processes
 Art des Abschluß: -

Veranstaltung

einblenden:

Entscheidung

einblenden:

Projektinformation

einblenden:

Quelle 1

einblenden:
ausblenden:
Titel: Geophysical Research Letters
Genre der Quelle: Zeitschrift, SCI, Scopus, ab 2023 oa
 Urheber:
Affiliations:
Ort, Verlag, Ausgabe: -
Seiten: - Band / Heft: 47 (15) Artikelnummer: e2020GL089000 Start- / Endseite: - Identifikator: ISSN: 1944-8007
ISSN: 0094-8276
CoNE: https://gfzpublic.gfz-potsdam.de/cone/journals/resource/journals182
Publisher: American Geophysical Union (AGU)