In-Situ observations of a co-rotating interaction region at Venus identified by IPS and STEREO

Standard

In-Situ observations of a co-rotating interaction region at Venus identified by IPS and STEREO. / Whittaker, I. C.; Dorrian, Gareth David; Breen, A.; Grande, M.; Barabash, S.

In: Solar Physics, Vol. 265, No. 1-2, 01.08.2010, p. 197-206.

Research output: Contribution to journalArticlepeer-review

Harvard

Whittaker, IC, Dorrian, GD, Breen, A, Grande, M & Barabash, S 2010, 'In-Situ observations of a co-rotating interaction region at Venus identified by IPS and STEREO', Solar Physics, vol. 265, no. 1-2, pp. 197-206. https://doi.org/10.1007/s11207-010-9608-2

APA

Whittaker, I. C., Dorrian, G. D., Breen, A., Grande, M., & Barabash, S. (2010). In-Situ observations of a co-rotating interaction region at Venus identified by IPS and STEREO. Solar Physics, 265(1-2), 197-206. https://doi.org/10.1007/s11207-010-9608-2

Vancouver

Author

Whittaker, I. C. ; Dorrian, Gareth David ; Breen, A. ; Grande, M. ; Barabash, S. / In-Situ observations of a co-rotating interaction region at Venus identified by IPS and STEREO. In: Solar Physics. 2010 ; Vol. 265, No. 1-2. pp. 197-206.

Bibtex - Download

@article{bd2f94ffe3824b8d84a39bbb05119491,
title = "In-Situ observations of a co-rotating interaction region at Venus identified by IPS and STEREO",
abstract = "This paper reports on the first combination of results from in-situ plasma measurements at Venus, using data from Venus Express, and remote sensing data from observations of interplanetary scintillation (IPS). In so doing, we demonstrate the value of combining remote sensing and in-situ techniques for the purpose of investigating interaction between solar wind, under several different conditions, and the Venusian magnetosphere. The ion mass analyser instrument (IMA) is used to investigate solar wind interaction with the Venusian magnetosphere in the presence of two different solar wind phenomena; a co-rotating interaction region (CIR) and a coronal mass ejection (CME). The CIR, detected with IPS and sampled in-situ at Venus is found to dramatically affect upstream solar wind conditions.These case studies demonstrate how combining results from these different data sources can be of considerable value when investigating such phenomena.",
keywords = "Co-rotating interaction region, IPS, Venus, Venus express, Combination of remote sensing and in situ, Ion counts, CME, Mass loading",
author = "Whittaker, {I. C.} and Dorrian, {Gareth David} and A. Breen and M. Grande and S. Barabash",
note = "Whittaker, I. C., Dorrian, G. D., Breen, A., Grande, M., Barabash, S. (2010). In-Situ observations of a co-rotating interaction region at Venus identified by IPS and STEREO. Solar Physics, 265 (1-2), 197-206. I Whittaker was M Grande's PhD student at this time. The paper refers to his thesis work.",
year = "2010",
month = aug,
day = "1",
doi = "10.1007/s11207-010-9608-2",
language = "English",
volume = "265",
pages = "197--206",
journal = "Solar Physics",
issn = "0038-0938",
publisher = "Springer Nature",
number = "1-2",

}

RIS (suitable for import to EndNote) - Download

TY - JOUR

T1 - In-Situ observations of a co-rotating interaction region at Venus identified by IPS and STEREO

AU - Whittaker, I. C.

AU - Dorrian, Gareth David

AU - Breen, A.

AU - Grande, M.

AU - Barabash, S.

N1 - Whittaker, I. C., Dorrian, G. D., Breen, A., Grande, M., Barabash, S. (2010). In-Situ observations of a co-rotating interaction region at Venus identified by IPS and STEREO. Solar Physics, 265 (1-2), 197-206. I Whittaker was M Grande's PhD student at this time. The paper refers to his thesis work.

PY - 2010/8/1

Y1 - 2010/8/1

N2 - This paper reports on the first combination of results from in-situ plasma measurements at Venus, using data from Venus Express, and remote sensing data from observations of interplanetary scintillation (IPS). In so doing, we demonstrate the value of combining remote sensing and in-situ techniques for the purpose of investigating interaction between solar wind, under several different conditions, and the Venusian magnetosphere. The ion mass analyser instrument (IMA) is used to investigate solar wind interaction with the Venusian magnetosphere in the presence of two different solar wind phenomena; a co-rotating interaction region (CIR) and a coronal mass ejection (CME). The CIR, detected with IPS and sampled in-situ at Venus is found to dramatically affect upstream solar wind conditions.These case studies demonstrate how combining results from these different data sources can be of considerable value when investigating such phenomena.

AB - This paper reports on the first combination of results from in-situ plasma measurements at Venus, using data from Venus Express, and remote sensing data from observations of interplanetary scintillation (IPS). In so doing, we demonstrate the value of combining remote sensing and in-situ techniques for the purpose of investigating interaction between solar wind, under several different conditions, and the Venusian magnetosphere. The ion mass analyser instrument (IMA) is used to investigate solar wind interaction with the Venusian magnetosphere in the presence of two different solar wind phenomena; a co-rotating interaction region (CIR) and a coronal mass ejection (CME). The CIR, detected with IPS and sampled in-situ at Venus is found to dramatically affect upstream solar wind conditions.These case studies demonstrate how combining results from these different data sources can be of considerable value when investigating such phenomena.

KW - Co-rotating interaction region

KW - IPS

KW - Venus

KW - Venus express

KW - Combination of remote sensing and in situ

KW - Ion counts

KW - CME

KW - Mass loading

UR - http://hdl.handle.net/2160/8321

U2 - 10.1007/s11207-010-9608-2

DO - 10.1007/s11207-010-9608-2

M3 - Article

VL - 265

SP - 197

EP - 206

JO - Solar Physics

JF - Solar Physics

SN - 0038-0938

IS - 1-2

ER -

View graph of relations
Citation formats