Search Results - "Panasenco, O."
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A Solar Source of Alfvénic Magnetic Field Switchbacks: In Situ Remnants of Magnetic Funnels on Supergranulation Scales
Published in The Astrophysical journal (01-12-2021)“…Abstract One of the striking observations from the Parker Solar Probe (PSP) spacecraft is the prevalence in the inner heliosphere of large amplitude, Alfvénic…”
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Observations of Solar Wind from Earth-directed Coronal Pseudostreamers
Published in The Astrophysical journal (20-02-2019)“…Low-speed ( 450 km s−1) solar wind is widely considered to originate from streamer loops that intermittently release their contents into the heliosphere, in…”
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3
Interchange reconnection as the source of the fast solar wind within coronal holes
Published in Nature (London) (08-06-2023)“…The fast solar wind that fills the heliosphere originates from deep within regions of open magnetic field on the Sun called ‘coronal holes’. The energy source…”
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2010 AUGUST 1-2 SYMPATHETIC ERUPTIONS. I. MAGNETIC TOPOLOGY OF THE SOURCE-SURFACE BACKGROUND FIELD
Published in The Astrophysical journal (01-11-2012)“…A sequence of apparently coupled eruptions was observed on 2010 August 1-2 by Solar Dynamics Observatory and STEREO. The eruptions were closely synchronized…”
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USING CORONAL CELLS TO INFER THE MAGNETIC FIELD STRUCTURE AND CHIRALITY OF FILAMENT CHANNELS
Published in The Astrophysical journal (01-08-2013)“…Coronal cells are visible at temperatures of ~1.2 MK in Fe XII coronal images obtained from the Solar Dynamics Observatory and Solar Terrestrial Relations…”
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Deprojected Trajectory of Blobs in the Inner Corona
Published in Solar physics (01-07-2018)“…We have carried out a statistical analysis of the kinematical behavior of small white-light transients (blobs) as tracers of the slow solar wind. The…”
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Stereoscopic Analysis of the 31 August 2007 Prominence Eruption and Coronal Mass Ejection
Published in Solar physics (2013)“…The spectacular prominence eruption and CME of 31 August 2007 are analyzed stereoscopically using data from NASA’s twin Solar Terrestrial Relations Observatory…”
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THE DISAPPEARING SOLAR FILAMENT OF 2003 JUNE 11: A THREE-BODY PROBLEM
Published in The Astrophysical journal (20-12-2011)“…The eruption of a large quiescent filament on 2003 June 11 was preceded by the birth of a nearby active region--a common scenario. In this case, however, the…”
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The link between CMEs, filaments and filament channels
Published in Annales geophysicae (1988) (15-10-2008)“…We present a broad concept for the build-up to eruptive solar events which needs to be tested in future observational and theoretical research. In this concept…”
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Conference Proceeding Journal Article -
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Coronal mass ejection and solar flare initiation processes without appreciable changes of the large-scale magnetic field topology
Published in Advances in space research (2006)“…We demonstrate that spurious three-dimensional re-constructions from two-dimensional images and movies of solar flares and coronal mass ejections can arise as…”
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Parker Solar Probe: Four Years of Discoveries at Solar Cycle Minimum
Published in Space science reviews (01-02-2023)“…Launched on 12 Aug. 2018, NASA’s Parker Solar Probe had completed 13 of its scheduled 24 orbits around the Sun by Nov. 2022. The mission’s primary science goal…”
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12
Rolling motion in erupting prominences observed by STEREO
Published in Journal of atmospheric and solar-terrestrial physics (20-06-2011)“…We analyze the large-scale dynamical forms of three erupting prominences (filaments) observed by at least one of the two STEREO spacecraft and which reveal…”
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Solar origins of intense geomagnetic storms in 2002 as seen by the CORONAS-F satellite
Published in Advances in space research (2005)“…We analyze solar origins of intense geomagnetic perturbations recorded during 2002. All of them were related to coronal mass ejections (CMEs). The initiation…”
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14
Reversal of Heliospheric Magnetic Field Polarity: Theoretical Model
Published in Solar system research (01-01-2002)“…A simple analytical model of the reversal of the heliospheric magnetic field is suggested. The shape of the heliospheric current sheet is found for each…”
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15
A MODEL FOR MAGNETICALLY COUPLED SYMPATHETIC ERUPTIONS
Published in The Astrophysical journal (2011)Get full text
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16
Interchange reconnection as the source of the fast solar wind within coronal holes
Published 07-06-2023“…The fast solar wind that fills the heliosphere originates from deep within regions of open magnetic field on the Sun called coronal holes. The energy source…”
Get full text
Journal Article -
17
A solar source of Alfv\'enic magnetic field switchbacks: {\em in situ} remnants of magnetic funnels on supergranulation scales
Published 02-09-2021“…One of the striking observations from the Parker Solar Probe (PSP) spacecraft is the prevalence in the inner heliosphere of large amplitude, Alfv\'enic…”
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Journal Article -
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IOPscience - The Disappearing Solar Filament of 2003 June 11: A Three-body Problem
Published in The Astrophysical journal (20-12-2011)Get full text
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19
Parker Solar Probe: Four Years of Discoveries at Solar Cycle Minimum
Published 06-01-2023“…Space Science Reviews 2023 Launched on 12 Aug. 2018, NASA's Parker Solar Probe had completed 13 of its scheduled 24 orbits around the Sun by Nov. 2022. The…”
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Journal Article -
20
2010 August 1-2 sympathetic eruptions: I. Magnetic topology of the source-surface background field
Published 26-09-2012“…A sequence of apparently coupled eruptions was observed on 2010 August 1-2 by SDO and STEREO. The eruptions were closely synchronized with one another, even…”
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Journal Article