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Ion-Ion Cross-Field Instability of Lower Hybrid Waves in the Inner Coma of Comet 67P
DOI: 10.1029/2022JA030535 Bibcode: 2022JGRA..12730535O

Karlsson, Tomas; Stenberg Wieser, Gabriella; Odelstad, Elias +2 more

We show that an ion-ion cross-field streaming instability between cold newborn cometary ions and heated heavy ions that were picked up upstream is likely a contributing source of observed lower hybrid (LH) waves in the inner coma of comet 67P/Churyumov-Gerasimenko. Electric field oscillations in the LH frequency range are common here, and have pre…

2022 Journal of Geophysical Research (Space Physics)
Rosetta 1
Observations of a Solar Energetic Particle Event From Inside and Outside the Coma of Comet 67P
DOI: 10.1029/2022JA030398 Bibcode: 2022JGRA..12730398W

Coates, A. J.; Palmerio, E.; Jones, G. H. +12 more

We analyze observations of a solar energetic particle (SEP) event at Rosetta's target comet 67P/Churyumov-Gerasimenko during 6-10 March 2015. The comet was 2.15 AU from the Sun, with the Rosetta spacecraft approximately 70 km from the nucleus placing it deep inside the comet's coma and allowing us to study its response. The Eastern flank of an int…

2022 Journal of Geophysical Research (Space Physics)
Rosetta 1
The Response of Saturn's Dawn Field-Aligned Currents to Magnetospheric and Ring Current Conditions During Cassini's Proximal Orbits: Evidence for a Region 2 Response at Saturn
DOI: 10.1029/2021JA029852 Bibcode: 2022JGRA..12729852H

Dougherty, M. K.; Roussos, E.; Cowley, S. W. H. +3 more

Cassini's 2017 proximal orbits provided the opportunity to examine the auroral field-aligned currents in the northern hemisphere dawn sector in relation to wider magnetospheric conditions. We combine three recent studies to examine the response of the dawn region auroral field-aligned currents and the azimuthal ring currents to compressions and ex…

2022 Journal of Geophysical Research (Space Physics)
Cassini 1
Mirror Mode Storms Observed by Solar Orbiter
DOI: 10.1029/2022JA030754 Bibcode: 2022JGRA..12730754D

Fedorov, A.; Karlsson, T.; Owen, C. J. +8 more

Mirror modes (MMs) are ubiquitous in space plasma and grow from pressure anisotropy. Together with other instabilities, they play a fundamental role in constraining the free energy contained in the plasma. This study focuses on MMs observed in the solar wind by Solar Orbiter (SolO) for heliocentric distances between 0.5 and 1 AU. Typically, MMs ha…

2022 Journal of Geophysical Research (Space Physics)
SolarOrbiter 1
Poleward Moving Auroral Arcs and Pc5 Oscillations
DOI: 10.1029/2022JA030362 Bibcode: 2022JGRA..12730362S

Sato, N.; Tanaka, Y.; Ebihara, Y. +6 more

We present an example of one-to-one correspondence between poleward moving auroral arcs (PMAAs) and Pc5 oscillations observed at the Time History of Events and Macroscale Interactions during Substorms (THEMIS) Ground Based Observatory station Gillam. The PMAAs consisted of four successive intensifications (named PMAA1, PMAA2, PMAA3 and PMAA4) with…

2022 Journal of Geophysical Research (Space Physics)
Cluster 0
Reply to Comment by Stauning on "The PC Index Variations During 23/24 Solar Cycles: Relation to Solar Wind Parameters and Magnetic Disturbances"
DOI: 10.1029/2022JA030519 Bibcode: 2022JGRA..12730519T

Sormakov, D. A.; Troshichev, O. A.; Dolgacheva, S. A. +1 more

The polar cap magnetic activity index (PC) was approved by IAGA as an index characterizing the solar wind energy input into the magnetosphere. Relation of the PC index to solar wind parameters and solar activity during 23/24 solar cycles has been studied in paper (Troshichev et al., 2021, https://doi.…

2022 Journal of Geophysical Research (Space Physics)
SOHO 0
Joint Cluster/Ground-Based Studies in the First 20 Years of the Cluster Mission
DOI: 10.1029/2021JA029928 Bibcode: 2022JGRA..12729928F

Fear, R. C.

Ground-based facilities make an important contribution to our understanding of the magnetospheric system. Coordination with ground-based facilities has been embedded within the Cluster mission since before launch, and this has given rise to a large number of studies which have exploited data from both Cluster and one or more of the diverse range o…

2022 Journal of Geophysical Research (Space Physics)
Cluster 0
Magnetosheath Filamentary Structures Driven by Foreshock Energetic Ions
DOI: 10.1029/2022JA030266 Bibcode: 2022JGRA..12730266W

Wei, Xinhua; Ma, Yuduan; Yang, Junying +1 more

Previous simulation studies have revealed the formation of magnetosheath filamentary structures by foreshock energetic ions. We report Cluster and Double Star observations of three such events triggered by a foreshock bubble, a hot flow anomaly and a traveling foreshock, respectively. In each case, in association with the onset of foreshock energe…

2022 Journal of Geophysical Research (Space Physics)
Cluster DoubleStar 0
Detection of Equatorial Plasma Velocity Modulations Associated With Planetary Period Oscillations in Saturn's Magnetosphere
DOI: 10.1029/2021JA030198 Bibcode: 2022JGRA..12730198B

Wilson, R. J.; Cowley, S. W. H.; Provan, G. +1 more

We analyze a database of 8920 measurements of thermal ion vector velocities obtained by the Cassini CAPS/IMS instrument in the near-equatorial (±10° latitude) region of Saturn's magnetosphere in the radial range of 5.5-21.5 Saturn radii (RS) for the presence of modulations due to planetary period oscillations (PPOs). The data span 2004-…

2022 Journal of Geophysical Research (Space Physics)
Cassini 0
Deriving CME Density From Remote Sensing Data and Comparison to In Situ Measurements
DOI: 10.1029/2020JA028380 Bibcode: 2021JGRA..12628380T

Temmer, M.; Veronig, A. M.; Vršnak, B. +8 more

We determine the three dimensional geometry and deprojected mass of 29 well observed coronal mass ejections (CMEs) and their interplanetary counterparts (ICMEs) using combined Solar Terrestrial Relations Observatory Solar and Heliospheric Observatory white light data. From the geometry parameters, we calculate the volume of the CME for the magneti…

2021 Journal of Geophysical Research (Space Physics)
SOHO 42