EUV-dependence of Venusian dayside ionopause altitude: VEX and PVO observations

The Venusian dayside ionosphere, similar to other planetary ionospheres, is produced primarily by ionization of its neutral upper atmosphere due to solar extreme ultraviolet (EUV) radiation. It has become clear that the expansion of the ionosphere may be strongly controlled by the EUV level, as exhi...

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Main Authors: QianQian Han, Markus Fraenz, Yong Wei, Eduard Dubinin, Jun Cui, LiHui Chai, ZhaoJin Rong, WeiXing Wan, Yoshifumi Futaana
Format: Article
Language:English
Published: Science Press 2020-01-01
Series:Earth and Planetary Physics
Subjects:
Online Access:http://www.eppcgs.org/article/doi/10.26464/epp2020011?pageType=en
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author QianQian Han
Markus Fraenz
Yong Wei
Eduard Dubinin
Jun Cui
LiHui Chai
ZhaoJin Rong
WeiXing Wan
Yoshifumi Futaana
author_facet QianQian Han
Markus Fraenz
Yong Wei
Eduard Dubinin
Jun Cui
LiHui Chai
ZhaoJin Rong
WeiXing Wan
Yoshifumi Futaana
author_sort QianQian Han
collection DOAJ
description The Venusian dayside ionosphere, similar to other planetary ionospheres, is produced primarily by ionization of its neutral upper atmosphere due to solar extreme ultraviolet (EUV) radiation. It has become clear that the expansion of the ionosphere may be strongly controlled by the EUV level, as exhibited in data collected by the Pioneer Venus Orbiter (PVO) during one solar cycle (1978–1992). However, the EUV-dependence of the Venusian dayside ionopause altitude, which defines the outer boundary of the ionosphere, remains obscure because the PVO crossed the dayside ionopause only during the solar maximum; its periapsis lifted too high during the solar minimum. Recently, during the period 2006–2014, which included the longest and quietest solar minimum of the past several decades, Venus Express (VEX) provided measurements of the photoelectron boundary (PEB) over the northern high-latitude region. Since the photoelectron boundary is closely related to the ionopause, we have an opportunity to analyze the EUV effect on the dayside ionopause by combining PVO and VEX observations. We have evaluated and then reduced the orbit bias effect in data from both PVO and VEX, and then used the results to derive a relationship between solar EUV level and the dayside ionopause altitude. We find that the dayside ionopause altitude increases as the solar EUV level increases, which is consistent with theoretical expectations.
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spelling doaj.art-897fac6111504167bc3f150e54f1338f2022-12-22T03:42:33ZengScience PressEarth and Planetary Physics2096-39552020-01-0141738110.26464/epp2020011hanqianqian-01EUV-dependence of Venusian dayside ionopause altitude: VEX and PVO observationsQianQian Han0Markus Fraenz1Yong Wei2Eduard Dubinin3Jun Cui4LiHui Chai5ZhaoJin Rong6WeiXing Wan7Yoshifumi Futaana8Key Laboratory of Earth and Planetary Physics, Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing 100029, ChinaMax-Planck-Institute for Solar System Research, Goettingen, DE 37077, GermanyKey Laboratory of Earth and Planetary Physics, Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing 100029, ChinaMax-Planck-Institute for Solar System Research, Goettingen, DE 37077, GermanySchool of Atmospheric Sciences, Sun Yat-Sen University, Zhuhai Guangdong 519082, ChinaKey Laboratory of Earth and Planetary Physics, Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing 100029, ChinaKey Laboratory of Earth and Planetary Physics, Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing 100029, ChinaKey Laboratory of Earth and Planetary Physics, Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing 100029, ChinaSwedish Institute of Space Physics, Kiruna, SE 98128, SwedenThe Venusian dayside ionosphere, similar to other planetary ionospheres, is produced primarily by ionization of its neutral upper atmosphere due to solar extreme ultraviolet (EUV) radiation. It has become clear that the expansion of the ionosphere may be strongly controlled by the EUV level, as exhibited in data collected by the Pioneer Venus Orbiter (PVO) during one solar cycle (1978–1992). However, the EUV-dependence of the Venusian dayside ionopause altitude, which defines the outer boundary of the ionosphere, remains obscure because the PVO crossed the dayside ionopause only during the solar maximum; its periapsis lifted too high during the solar minimum. Recently, during the period 2006–2014, which included the longest and quietest solar minimum of the past several decades, Venus Express (VEX) provided measurements of the photoelectron boundary (PEB) over the northern high-latitude region. Since the photoelectron boundary is closely related to the ionopause, we have an opportunity to analyze the EUV effect on the dayside ionopause by combining PVO and VEX observations. We have evaluated and then reduced the orbit bias effect in data from both PVO and VEX, and then used the results to derive a relationship between solar EUV level and the dayside ionopause altitude. We find that the dayside ionopause altitude increases as the solar EUV level increases, which is consistent with theoretical expectations.http://www.eppcgs.org/article/doi/10.26464/epp2020011?pageType=envenusionopauseionospheresolar activity
spellingShingle QianQian Han
Markus Fraenz
Yong Wei
Eduard Dubinin
Jun Cui
LiHui Chai
ZhaoJin Rong
WeiXing Wan
Yoshifumi Futaana
EUV-dependence of Venusian dayside ionopause altitude: VEX and PVO observations
Earth and Planetary Physics
venus
ionopause
ionosphere
solar activity
title EUV-dependence of Venusian dayside ionopause altitude: VEX and PVO observations
title_full EUV-dependence of Venusian dayside ionopause altitude: VEX and PVO observations
title_fullStr EUV-dependence of Venusian dayside ionopause altitude: VEX and PVO observations
title_full_unstemmed EUV-dependence of Venusian dayside ionopause altitude: VEX and PVO observations
title_short EUV-dependence of Venusian dayside ionopause altitude: VEX and PVO observations
title_sort euv dependence of venusian dayside ionopause altitude vex and pvo observations
topic venus
ionopause
ionosphere
solar activity
url http://www.eppcgs.org/article/doi/10.26464/epp2020011?pageType=en
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