Comparison of modified Woo’s solar phase scintillation model with ESA’s BepiColombo superior solar conjunction measurement data for X-band and Ka-band

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Location: Deutsche Nationalbibliothek Frankfurt am Main

ISSN: 1868-2510

Extent: Online-Ressource

Language: Englisch

Notes: online resource.

Bibliographic citation: 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

Creator: Chen, Shun-Ping
Villalvilla, Jose

Contributor: SpringerLink (Online service)

DOI: 10.1007/s12567-022-00426-3

URN: urn:nbn:de:101:1-2022052620123218879865

Rights: Open Access; Der Zugriff auf das Objekt ist unbeschränkt möglich.

Last update: 15.08.2025, 7:29 AM CEST

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Chen, Shun-Ping
Villalvilla, Jose
SpringerLink (Online service)

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Comparison of modified Woo’s solar phase scintillation model with ESA’s BepiColombo superior solar conjunction measurement data for X-band and Ka-band

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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

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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

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Comparison of modified Woo’s solar phase scintillation model with ESA’s BepiColombo superior solar conjunction measurement data for X-band and Ka-band

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Other Objects (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

Simultaneous interplanetary scintillation and optical measurements of the acceleration of the slow solar wind

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