Comparison of modified Woo’s solar phase scintillation model with ESA’s BepiColombo superior solar conjunction measurement data for X-band and Ka-band
- Standort
-
Deutsche Nationalbibliothek Frankfurt am Main
- ISSN
-
1868-2510
- Umfang
-
Online-Ressource
- Sprache
-
Englisch
- Anmerkungen
-
online resource.
- Erschienen in
-
Comparison of modified Woo’s solar phase scintillation model with ESA’s BepiColombo superior solar conjunction measurement data for X-band and Ka-band ; day:24 ; month:2 ; year:2022 ; pages:1-7
CEAS space journal / Confederation of European Aerospace Societies ; (24.2.2022), 1-7
- Urheber
- Beteiligte Personen und Organisationen
-
SpringerLink (Online service)
- DOI
-
10.1007/s12567-022-00426-3
- URN
-
urn:nbn:de:101:1-2022052620123218879865
- Rechteinformation
-
Open Access; Der Zugriff auf das Objekt ist unbeschränkt möglich.
- Letzte Aktualisierung
-
15.08.2025, 07:29 MESZ
Datenpartner
Dieses Objekt wird bereitgestellt von:
Deutsche Nationalbibliothek. Bei Fragen zum Objekt wenden Sie sich bitte an den Datenpartner.
Deutsche Nationalbibliothek. Bei Fragen zum Objekt wenden Sie sich bitte an den Datenpartner.
Beteiligte
- Chen, Shun-Ping
- Villalvilla, Jose
- SpringerLink (Online service)
Ähnliche Objekte (12)
Comparison of modified Woo’s solar phase scintillation model with ESA’s BepiColombo superior solar conjunction measurement data for X-band and Ka-band
Investigation of X-band and Ka-band amplitude scintillation based on measurement data collected during ESA’s BepiColombo superior solar conjunction campaign
Investigation of X‑band and Ka‑band amplitude scintillation based on measurement data collected during ESA’s BepiColombo superior solar conjunction campaign
How did the solar wind structure change around the solar maximum? From interplanetary scintillation observation
Scintillation measurements at Bahir Dar during the high solar activity phase of solar cycle 24
Interplanetary scintillation observations of interaction regions in the solar wind
Future opportunities in solar system plasma science through ESA’s exploration programme
Measurements of the direction of the solar wind using interplanetary scintillation
Solar flux dependence of coherence scales in scintillation patterns produced by ESF irregularities
GPS TEC, scintillation and cycle slips observed at high latitudes during solar minimum
EISCAT measurements of solar wind velocity and the associated level of interplanetary scintillation
Simultaneous interplanetary scintillation and optical measurements of the acceleration of the slow solar wind
Comparison of modified Woo’s solar phase scintillation model with ESA’s BepiColombo superior solar conjunction measurement data for X-band and Ka-band
Investigation of X-band and Ka-band amplitude scintillation based on measurement data collected during ESA’s BepiColombo superior solar conjunction campaign
Investigation of X‑band and Ka‑band amplitude scintillation based on measurement data collected during ESA’s BepiColombo superior solar conjunction campaign
How did the solar wind structure change around the solar maximum? From interplanetary scintillation observation
Scintillation measurements at Bahir Dar during the high solar activity phase of solar cycle 24
Interplanetary scintillation observations of interaction regions in the solar wind
Future opportunities in solar system plasma science through ESA’s exploration programme
Measurements of the direction of the solar wind using interplanetary scintillation
Solar flux dependence of coherence scales in scintillation patterns produced by ESF irregularities
GPS TEC, scintillation and cycle slips observed at high latitudes during solar minimum
EISCAT measurements of solar wind velocity and the associated level of interplanetary scintillation
Simultaneous interplanetary scintillation and optical measurements of the acceleration of the slow solar wind
Comparison of modified Woo’s solar phase scintillation model with ESA’s BepiColombo superior solar conjunction measurement data for X-band and Ka-band
Investigation of X-band and Ka-band amplitude scintillation based on measurement data collected during ESA’s BepiColombo superior solar conjunction campaign
Investigation of X‑band and Ka‑band amplitude scintillation based on measurement data collected during ESA’s BepiColombo superior solar conjunction campaign
How did the solar wind structure change around the solar maximum? From interplanetary scintillation observation
Scintillation measurements at Bahir Dar during the high solar activity phase of solar cycle 24
Interplanetary scintillation observations of interaction regions in the solar wind
Future opportunities in solar system plasma science through ESA’s exploration programme
Measurements of the direction of the solar wind using interplanetary scintillation
Solar flux dependence of coherence scales in scintillation patterns produced by ESF irregularities
GPS TEC, scintillation and cycle slips observed at high latitudes during solar minimum
EISCAT measurements of solar wind velocity and the associated level of interplanetary scintillation