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PIC Simulations of Microinstabilities and Waves at Near-Sun Solar Wind Perpendicular Shocks: Predictions for Parker Solar Probe and Solar Orbiter
DOI: 10.3847/2041-8213/abaf59 Bibcode: 2020ApJ...900L..24Y

Yang, Zhongwei; Liu, Ying D.; Guo, Fan +6 more

Microinstabilities and waves excited at moderate-Mach-number perpendicular shocks in the near-Sun solar wind are investigated by full particle-in-cell simulations. By analyzing the dispersion relation of fluctuating field components directly issued from the shock simulation, we obtain key findings concerning wave excitations at the shock front: (1…

2020 The Astrophysical Journal
SolarOrbiter 11
Momentum and Pressure Balance of a Comet Ionosphere
DOI: 10.1029/2020GL088666 Bibcode: 2020GeoRL..4788666W

Nilsson, H.; Goetz, C.; Richter, I. +3 more

We calculate the momentum flux and pressure of ions measured by the Ion Composition Analyzer (ICA) on the Rosetta mission at comet 67P/Churyumov-Gerasimenko. The total momentum flux stays roughly constant over the mission, but the contributions of different ion populations change depending on heliocentric distance. The magnetic pressure, calculate…

2020 Geophysical Research Letters
Rosetta 11
Kernel-phase analysis: Aperture modeling prescriptions that minimize calibration errors
DOI: 10.1051/0004-6361/201936981 Bibcode: 2020A&A...636A..72M

Martinache, Frantz; Kammerer, Jens; N'Diaye, Mamadou +5 more

Context. Kernel phase is a data analysis method based on a generalization of the notion of closure phase, which was invented in the context of interferometry, but it applies to well corrected diffraction dominated images produced by an arbitrary aperture. The linear model upon which it relies theoretically leads to the formation of observable quan…

2020 Astronomy and Astrophysics
eHST 11
The Broad-lined Ic Supernova ZTF18aaqjovh (SN 2018bvw): An Optically Discovered Engine-driven Supernova Candidate with Luminous Radio Emission
DOI: 10.3847/1538-4357/ab7f3b Bibcode: 2020ApJ...893..132H

Kulkarni, S. R.; Cenko, S. Bradley; Riddle, Reed +25 more

We present ZTF18aaqjovh (SN 2018bvw), a high-velocity ("broad-lined") stripped-envelope (Type Ic) supernova (Ic-BL SN) discovered in the Zwicky Transient Facility one-day cadence survey. ZTF18aaqjovh shares a number of features in common with engine-driven explosions: the photospheric velocity and the shape of the optical light curve are very simi…

2020 The Astrophysical Journal
INTEGRAL 11
Sequential Observations of Flux Transfer Events, Poleward-Moving Auroral Forms, and Polar Cap Patches
DOI: 10.1029/2019JA027674 Bibcode: 2020JGRA..12527674H

Russell, C. T.; Khotyaintsev, Y.; Fear, R. C. +17 more

We report the observation of solar wind-magnetosphere-ionosphere interactions using a series of flux transfer events (FTEs) observed by Magnetospheric MultiScale (MMS) mission located near the dayside magnetopause on 18 December 2017. The FTEs were observed to propagate duskward and either southward or slightly northward, as predicted under duskwa…

2020 Journal of Geophysical Research (Space Physics)
Cluster 11
Outbursts of comets at large heliocentric distances: Concise review and numerical simulations of brightness jumps
DOI: 10.1016/j.pss.2020.104867 Bibcode: 2020P&SS..18404867W

Wesołowski, M.; Gronkowski, P.; Tralle, I.

The outburst of comet brightness is spectacular and well-known manifestation of the physical activity of these relatively small cosmic bodies. The outbursts of brightness are observed for periodic comets, as well as for the comets moving along parabolic trajectories. The most known comet representing such kind of activity is the comet 29P/Schwassm…

2020 Planetary and Space Science
Rosetta 11
End-of-mission calibration of the Cassini Imaging Science Subsystem
DOI: 10.1016/j.pss.2020.104898 Bibcode: 2020P&SS..18504898K

Porco, Carolyn; West, Robert; Verbiscer, Anne +3 more

We provide an end-of-mission update to the in-flight calibration of the Imaging Science Subsystem cameras on the Cassini spacecraft, resolving discrepancies in our previous analyses from 2004 to 2010, incorporating data through the end of the mission, adding a correction for the weak but measurable camera sensitivity decline over time, and providi…

2020 Planetary and Space Science
Cassini eHST 11
Investigating the Chromospheric Footpoints of the Solar Wind
DOI: 10.3847/2041-8213/abce69 Bibcode: 2020ApJ...905L..33B

De Pontieu, Bart; McIntosh, Scott W.; Brooks, David H. +1 more

Coronal holes present the source of the fast solar wind. However, the fast solar wind is not unimodal—there are discrete, but subtle, compositional, velocity, and density structures that differentiate different coronal holes as well as wind streams that originate within one coronal hole. In this Letter we exploit full-disk observational "mosaics" …

2020 The Astrophysical Journal
IRIS 11
ALMA Observations of the Extraordinary Carina Pillars: HH 901/902
DOI: 10.3847/1538-3881/ab6295 Bibcode: 2020AJ....159...62C

Ho, Paul T. P.; Mesa-Delgado, Adal; Toalá, Jesús A. +4 more

We present Atacama Large Millimeter/Submillimeter Array 1.3 mm continuum and C18O(2-1), N2D+(3-2), 13CS(5-4), and 12CO(2-1) line sensitive and high angular resolution (∼0"3) observations of the famous Carina pillars and protostellar objects HH 901/902. Our observations reveal for the first tim…

2020 The Astronomical Journal
eHST 11
The Hα Emission Line Variations of HR 6819
DOI: 10.3847/2041-8213/aba51c Bibcode: 2020ApJ...898L..44G

Gies, Douglas R.; Wang, Luqian

The star system HR 6819 was recently proposed by Rivinius et al. as the site of the nearest example of a stellar-mass black hole. Their spectra show evidence of two components: a B3 III star in a 40 day orbit and a stationary B-emission line star. Based upon the orbital mass function and the lack of evidence of a spectral component with reflex orb…

2020 The Astrophysical Journal
IUE 11