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CME-HSS Interaction and Characteristics Tracked from Sun to Earth
DOI: 10.1007/s11207-019-1515-6 Bibcode: 2019SoPh..294..121H

Veronig, Astrid M.; Dumbović, Mateja; Temmer, Manuela +9 more

In a thorough study, we investigate the origin of a remarkable plasma and magnetic field configuration observed in situ on June 22, 2011, near L1, which appears to be a magnetic ejecta (ME) and a shock signature engulfed by a solar wind high-speed stream (HSS). We identify the signatures as an Earth-directed coronal mass ejection (CME), associated…

2019 Solar Physics
SOHO 53
What the Sudden Death of Solar Cycles Can Tell Us About the Nature of the Solar Interior
DOI: 10.1007/s11207-019-1474-y Bibcode: 2019SoPh..294...88M

Rempel, Matthias; McIntosh, Scott W.; Leamon, Robert J. +3 more

We observe the abrupt end of solar-activity cycles at the Sun's Equator by combining almost 140 years of observations from ground and space. These "terminator" events appear to be very closely related to the onset of magnetic activity belonging to the next solar cycle at mid-latitudes and the polar-reversal process at high latitudes. Using multi-s…

2019 Solar Physics
SOHO 39
Unexpected Behavior of the Solar Wind Mass Flux During Solar Maxima: Two Peaks at Middle Heliolatitudes
DOI: 10.1007/s11207-018-1391-5 Bibcode: 2019SoPh..294...17K

Quémerais, Eric; Koutroumpa, Dimitra; Katushkina, Olga +2 more

In this work we study the temporal and latitudinal variations of the solar wind mass flux at 1 AU derived from SOHO/SWAN data on backscattered solar Lyman-α radiation in 1996 - 2018. Previously Katushkina et al. (J. Geophys. Res.118, 2800, 2013) have shown that the latitudinal profiles of the solar wind mass flux during the solar maximum 2001 - 20…

2019 Solar Physics
SOHO 29
Which Photospheric Characteristics Are Most Relevant to Active-Region Coronal Mass Ejections?
DOI: 10.1007/s11207-019-1523-6 Bibcode: 2019SoPh..294..130K

Guerra, Jordan A.; Park, Sung-Hong; Bloomfield, D. Shaun +2 more

We investigate the relation between characteristics of coronal mass ejections and parameterizations of the eruptive capability of solar active regions widely used in solar flare-prediction schemes. These parameters, some of which are explored for the first time, are properties related to topological features, namely, magnetic polarity-inversion li…

2019 Solar Physics
SOHO 26
CMEs in the Heliosphere: II. A Statistical Analysis of the Kinematic Properties Derived from Single-Spacecraft Geometrical Modelling Techniques Applied to CMEs Detected in the Heliosphere from 2007 to 2017 by STEREO/HI-1
DOI: 10.1007/s11207-019-1444-4 Bibcode: 2019SoPh..294...57B

Rodriguez, L.; Möstl, C.; Kilpua, E. K. J. +10 more

Recent observations with the Heliospheric Imagers (HIs) onboard the twin NASA Solar Terrestrial Relations Observatory (STEREO) spacecraft have provided unprecedented observations of a large number of coronal mass ejections (CMEs) in the inner heliosphere. In this article we discuss the generation of the HIGeoCAT CME catalogue and perform a statist…

2019 Solar Physics
SOHO 25
Are Solar Energetic Particle Events and Type II Bursts Associated with Fast and Narrow Coronal Mass Ejections?
DOI: 10.1007/s11207-019-1518-3 Bibcode: 2019SoPh..294..134K

Gopalswamy, N.; Kahler, S. W.; Ling, A. G.

Gradual solar energetic (E >10 MeV) particle (SEP) events and metric through kilometric wavelength type II radio bursts are usually associated with shocks driven by fast (V ≥900 kms−1) and wide (W ≥60) coronal mass ejections (FW CMEs). This criterion was established empirically by several studies from solar cycle 23. The …

2019 Solar Physics
SOHO 19
Interplanetary Coronal Mass Ejections During Solar Cycles 23 and 24: Sun-Earth Propagation Characteristics and Consequences at the Near-Earth Region
DOI: 10.1007/s11207-019-1443-5 Bibcode: 2019SoPh..294...54S

Joshi, Bhuwan; Cho, K. -S.; Moon, Y. -J. +2 more

In this article, we present a statistical study probing the relation between interplanetary coronal mass ejections (ICMEs) observed at 1 AU and their corresponding coronal mass ejections at the near-Sun region. The work encompasses the ICME activity that occurred during Solar Cycles 23 and 24 (1996 - 2017) while presenting an overall picture of IC…

2019 Solar Physics
SOHO 19
A Catalogue of Forbush Decreases Recorded on the Surface of Mars from 2012 Until 2016: Comparison with Terrestrial FDs
DOI: 10.1007/s11207-019-1454-2 Bibcode: 2019SoPh..294...66P

Wimmer-Schweingruber, R. F.; Heber, B.; Herbst, K. +9 more

Forbush decreases (FDs) in galactic cosmic rays (GCRs) have been recorded by neutron monitors (NMs) at Earth for more than 60 years. For the past five years, with the establishment of the Radiation Assessment Detector (RAD) onboard the Mars Science Laboratory (MSL) rover Curiosity at Mars, it is possible to continuously detect, for the first time,…

2019 Solar Physics
SOHO 18
Solar Flare Forecasting from Magnetic Feature Properties Generated by the Solar Monitor Active Region Tracker
DOI: 10.1007/s11207-018-1392-4 Bibcode: 2019SoPh..294....6D

Bloomfield, D. Shaun; Domijan, Katarina; Pitié, François

We study the predictive capabilities of magnetic-feature properties (MF) generated by the Solar Monitor Active Region Tracker (SMART: Higgins et al. in Adv. Space Res.47, 2105, 2011) for solar-flare forecasting from two datasets: the full dataset of SMART detections from 1996 to 2010 which has been previously studied by Ahmed et al. (Solar Phys.28…

2019 Solar Physics
SOHO 17
Development of a Fast CME and Properties of a Related Interplanetary Transient
DOI: 10.1007/s11207-019-1529-0 Bibcode: 2019SoPh..294..139G

Grechnev, V. V.; Kochanov, A. A.; Kiselev, V. I. +5 more

We study the development of a coronal mass ejection (CME) caused by a prominence eruption on 24 February 2011 and properties of a related interplanetary CME (ICME). The prominence destabilized, accelerated, and produced an M3.5 flare, a fast CME, and a shock wave. The eruption at the east limb was observed in quadrature by the Atmospheric Imaging …

2019 Solar Physics
SOHO 16