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Global view of refilling of the plasmasphere

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Global view of refilling of the plasmasphere. / Sandel, B. R.; Denton, M. H.
In: Geophysical Research Letters, Vol. 34, No. L17102, 09.2007, p. 1-5.

Research output: Contribution to Journal/MagazineJournal articlepeer-review

Harvard

Sandel, BR & Denton, MH 2007, 'Global view of refilling of the plasmasphere', Geophysical Research Letters, vol. 34, no. L17102, pp. 1-5. https://doi.org/10.1029/2007GL030669

APA

Sandel, B. R., & Denton, M. H. (2007). Global view of refilling of the plasmasphere. Geophysical Research Letters, 34(L17102), 1-5. https://doi.org/10.1029/2007GL030669

Vancouver

Sandel BR, Denton MH. Global view of refilling of the plasmasphere. Geophysical Research Letters. 2007 Sept;34(L17102):1-5. doi: 10.1029/2007GL030669

Author

Sandel, B. R. ; Denton, M. H. / Global view of refilling of the plasmasphere. In: Geophysical Research Letters. 2007 ; Vol. 34, No. L17102. pp. 1-5.

Bibtex

@article{bd327a0bc0f3495f9b41234752d42052,
title = "Global view of refilling of the plasmasphere",
abstract = "We use observations by the IMAGE Extreme Ultraviolet Imager (EUV) to characterize the outflow of He+ from the ionosphere to the plasmasphere under quiet conditions. The view afforded by the IMAGE orbit encompasses the entire plasmasphere in a single exposure, enabling us to examine for the first time the globally-averaged properties of plasmasphere refilling. We focus on a study period that begins with a moderate erosion event, and follow refilling during multiple orbits for a period of 69 hours. The inferred volume refilling rate, averaged over azimuth and time, ranges from ∼1 He+ cm−3 h−1 at L = 3.3 to ∼7 × 10−2 He+ cm−3 h−1 at L = 6.3 and is generally consistent with earlier, more local measurements. We show that the measured radial abundance profiles match those predicted by the Sheffield University Plasmasphere Ionosphere Model (SUPIM) for 2 ≤ L ≤ 4.",
keywords = "plasmasphere modelling DCS-publications-id, art-864, DCS-publications-credits, iono, DCS-publications-personnel-id, 123",
author = "Sandel, {B. R.} and Denton, {M. H.}",
year = "2007",
month = sep,
doi = "10.1029/2007GL030669",
language = "English",
volume = "34",
pages = "1--5",
journal = "Geophysical Research Letters",
issn = "0094-8276",
publisher = "John Wiley & Sons, Ltd",
number = "L17102",

}

RIS

TY - JOUR

T1 - Global view of refilling of the plasmasphere

AU - Sandel, B. R.

AU - Denton, M. H.

PY - 2007/9

Y1 - 2007/9

N2 - We use observations by the IMAGE Extreme Ultraviolet Imager (EUV) to characterize the outflow of He+ from the ionosphere to the plasmasphere under quiet conditions. The view afforded by the IMAGE orbit encompasses the entire plasmasphere in a single exposure, enabling us to examine for the first time the globally-averaged properties of plasmasphere refilling. We focus on a study period that begins with a moderate erosion event, and follow refilling during multiple orbits for a period of 69 hours. The inferred volume refilling rate, averaged over azimuth and time, ranges from ∼1 He+ cm−3 h−1 at L = 3.3 to ∼7 × 10−2 He+ cm−3 h−1 at L = 6.3 and is generally consistent with earlier, more local measurements. We show that the measured radial abundance profiles match those predicted by the Sheffield University Plasmasphere Ionosphere Model (SUPIM) for 2 ≤ L ≤ 4.

AB - We use observations by the IMAGE Extreme Ultraviolet Imager (EUV) to characterize the outflow of He+ from the ionosphere to the plasmasphere under quiet conditions. The view afforded by the IMAGE orbit encompasses the entire plasmasphere in a single exposure, enabling us to examine for the first time the globally-averaged properties of plasmasphere refilling. We focus on a study period that begins with a moderate erosion event, and follow refilling during multiple orbits for a period of 69 hours. The inferred volume refilling rate, averaged over azimuth and time, ranges from ∼1 He+ cm−3 h−1 at L = 3.3 to ∼7 × 10−2 He+ cm−3 h−1 at L = 6.3 and is generally consistent with earlier, more local measurements. We show that the measured radial abundance profiles match those predicted by the Sheffield University Plasmasphere Ionosphere Model (SUPIM) for 2 ≤ L ≤ 4.

KW - plasmasphere modelling DCS-publications-id

KW - art-864

KW - DCS-publications-credits

KW - iono

KW - DCS-publications-personnel-id

KW - 123

U2 - 10.1029/2007GL030669

DO - 10.1029/2007GL030669

M3 - Journal article

VL - 34

SP - 1

EP - 5

JO - Geophysical Research Letters

JF - Geophysical Research Letters

SN - 0094-8276

IS - L17102

ER -