Articles | Volume 38, issue 3
https://doi.org/10.5194/angeo-38-703-2020
© Author(s) 2020. This work is distributed under
the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
Special issue:
https://doi.org/10.5194/angeo-38-703-2020
© Author(s) 2020. This work is distributed under
the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
Regular paper
| 
10 Jun 2020
Regular paper |
| 10 Jun 2020
| 10 Jun 2020
From the Sun to Earth: effects of the 25 August 2018 geomagnetic storm
Mirko Piersanti
CORRESPONDING AUTHOR
Physics Department, Istituto Nazionale di Fisica Nucleare (INFI), University of Rome Tor Vergata, Rome, Italy
Paola De Michelis
Istituto Nazionale di Geofisica e Vulcanologia, Rome, Italy
Dario Del Moro
University of Rome Tor Vergata, Rome, Italy
Roberta Tozzi
Istituto Nazionale di Geofisica e Vulcanologia, Rome, Italy
Michael Pezzopane
Istituto Nazionale di Geofisica e Vulcanologia, Rome, Italy
Giuseppe Consolini
Istituto di Astrofisica e Planetologia Spaziali, Istituto Nazionale di Astrofisica (INAF-IAPS), Rome, Italy
Maria Federica Marcucci
Istituto di Astrofisica e Planetologia Spaziali, Istituto Nazionale di Astrofisica (INAF-IAPS), Rome, Italy
Monica Laurenza
Istituto di Astrofisica e Planetologia Spaziali, Istituto Nazionale di Astrofisica (INAF-IAPS), Rome, Italy
Simone Di Matteo
Catholic University of America, NASA Goddard Space Flight Center, Greenbelt, Maryland, USA
Alessio Pignalberi
Istituto Nazionale di Geofisica e Vulcanologia, Rome, Italy
Virgilio Quattrociocchi
Istituto di Astrofisica e Planetologia Spaziali, Istituto Nazionale di Astrofisica (INAF-IAPS), Rome, Italy
Department of Physical and Chemical Sciences, University of L'Aquila, L'Aquila, Italy
Piero Diego
Istituto di Astrofisica e Planetologia Spaziali, Istituto Nazionale di Astrofisica (INAF-IAPS), Rome, Italy
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This paper presents a completely new method based on a new data analysis technique (ALIF) to determine both the environmental and instrumental backgrounds applied to all the DEMETER satellite electric and magnetic field data over L'Aquila's seismic region. Interestingly, on 4 April 2009, when DEMETER flew exactly over L'Aquila at 20:29 UT, an anomalous signal was observed at 333 Hz on both the electric and magnetic field data, whose characteristics seem to be related to pre-seismic activity.
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We investigate the time variation of the magnetospheric and Earth's magnetic field during both quiet and disturbed periods. We identify the timescale variations associated with different magnetospheric current systems, solar-wind–magnetosphere high-frequency interactions, ionospheric processes, and internal dynamics of the magnetosphere. In addition, we propose a new local index for the identification of the intensity of a geomagnetic storm on the ground.
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Manuscript not accepted for further review
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In-situ measurements validation is always a delicate matter of study until data are collected by a single mission. In case of different missions operating almost in the same environment (i.e. latitude, altitude, local time) it is of fundamental importance the detection of instrumental setting and algorithms to provide the best accordance among measurements. The present work aims to validate both Swarm and CSES plasma density measures for the improvements of the ionospheric models development.
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We investigate the time variation of the magnetospheric and Earth's magnetic field during both quiet and disturbed periods. We identify the timescale variations associated with different magnetospheric current systems, solar-wind–magnetosphere high-frequency interactions, ionospheric processes, and internal dynamics of the magnetosphere. In addition, we propose a new local index for the identification of the intensity of a geomagnetic storm on the ground.
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Subject: Magnetosphere & space plasma physics | Keywords: Solar wind–magnetosphere interactions
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Velocity of magnetic holes in the solar wind from Cluster multipoint measurements
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Solar wind magnetic holes can cross the bow shock and enter the magnetosheath
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Local time extent of magnetopause reconnection using space–ground coordination
The asymmetric geospace as displayed during the geomagnetic storm on 17 August 2001
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In our study, we looked at the boundary between the Earth's magnetic field and the interplanetary magnetic field emitted by the Sun, called the magnetopause. While other studies focus on the magnetopause motion near Earth's equator, we have studied it in polar regions. The motion of the magnetopause is faster towards the Earth than towards the Sun. We also found that the occurrence of unusual magnetopause locations is due to similar solar influences in the equatorial and in the polar regions.
Henriette Trollvik, Tomas Karlsson, and Savvas Raptis
Ann. Geophys., 41, 327–337, https://doi.org/10.5194/angeo-41-327-2023, https://doi.org/10.5194/angeo-41-327-2023, 2023
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The solar wind is in a plasma state and can exhibit a range of phenomena like waves and instabilities. One observed phenomenon in the solar wind is magnetic holes (MHs). They are localized depressions in the magnetic field. We studied the motion of MHs using the multispacecraft ESA Cluster mission. We derived their velocities in the solar wind frame and found that both linear and rotational MHs are convected with the solar wind.
Beket Tulegenov, Joachim Raeder, William D. Cramer, Banafsheh Ferdousi, Timothy J. Fuller-Rowell, Naomi Maruyama, and Robert J. Strangeway
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Ann. Geophys., 40, 687–699, https://doi.org/10.5194/angeo-40-687-2022, https://doi.org/10.5194/angeo-40-687-2022, 2022
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Magnetic holes are curious localized dropouts of magnetic field strength in the solar wind (the flow of ionized gas continuously streaming out from the sun). In this paper we show that these magnetic holes can cross the bow shock (where the solar wind brake down to subsonic velocity) and enter the region close to Earth’s magnetosphere. These structures may therefore represent a new type of non-uniform solar wind–magnetosphere interaction.
Invariability of relationship between the polar cap magnetic activity and geoeffective interplanetary electric fieldby Troshichev et al. (2011)
Peter Stauning
Ann. Geophys. Discuss., https://doi.org/10.5194/angeo-2020-52, https://doi.org/10.5194/angeo-2020-52, 2020
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In Troshichev et al. (2006) an error was made in the calculations of Polar Cap (PC) index scaling parameters. For the publication commented here, Troshichev et al. (2011), the authors state having used scaling parameters of the invalid PC index version but have actually substituted parameters from another version instead. The mingling of PC index versions has resulted in erroneous illustrations in Figs. 1, 2, 3, 6, 7, and 8 and the issuing of non-substantiated statements.
Antti Lakka, Tuija I. Pulkkinen, Andrew P. Dimmock, Emilia Kilpua, Matti Ala-Lahti, Ilja Honkonen, Minna Palmroth, and Osku Raukunen
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We study how the Earth's space environment responds to two different amplitude interplanetary coronal mass ejection (ICME) events that occurred in 2012 and 2014 by using the GUMICS-4 global MHD model. We examine local and large-scale dynamics of the Earth's space environment and compare simulation results to in situ data. It is shown that during moderate driving simulation agrees well with the measurements; however, GMHD results should be interpreted cautiously during strong driving.
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Magnetopause reconnection is a process whereby the Sun explosively transfers energy to the Earth. Whether the process is spatially patchy or spatially continuous and extended has been under long debate. We use space–ground coordination to overcome the limitations of previous studies and reliably interpret spatial extent. Our result strongly indicates that both patchy and extended reconnection is possible and, interestingly, that extended reconnection grows from a localized patch via spreading.
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In this paper we take advantage of having two auroral imaging missions giving simultaneous data of both the southern and northern aurora. Combined with all available in situ measurements from space and global ground-based networks, we explore the asymmetric behavior of geospace. We find large auroral asymmetries and different reconnection geometry in the two hemispheres. During substorm expansion phase asymmetries are reduced.
Jay R. Johnson, Simon Wing, and Enrico Camporeale
Ann. Geophys., 36, 945–952, https://doi.org/10.5194/angeo-36-945-2018, https://doi.org/10.5194/angeo-36-945-2018, 2018
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The magnetospheric response to the solar wind is nonlinear. Information theoretical tools are able to characterize the nonlinearities in the system. We show that nonlinear significance of Dst peaks at lags of 3–12 hours which can be attributed to VBs, which also exhibits similar behavior. However, the nonlinear significance that peaks at lags of 25, 50, and 90 hours can be attributed to internal dynamics, which may be related to the relaxation of the ring current.
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Short summary
This paper presents a comprehensive analysis of the solar event that occurred on 25 August 2018. This kind of comprehensive analysis plays a key role in better understanding the complexity of the processes occurring in the Sun–Earth system determining the geoeffectiveness of manifestations of solar activity. The analysis presented here shows for the first time a direct link between characteristics of solar perturbation, the magnetosphere–ionosphere system response and space weather effects.
This paper presents a comprehensive analysis of the solar event that occurred on 25 August 2018....
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