Results 101 to 110 of about 2,118 (212)

The Whole Heliosphere Interval in the Context of a Long and Structured Solar Minimum: An Overview from Sun to Earth [PDF]

, 2011
Throughout months of extremely low solar activity during the recent extended solar-cycle minimum, structural evolution continued to be observed from the Sun through the solar wind and to the Earth.
McIntosh, S, Riley, P., Lei, J, Leiner, J., Webb, D, Mewaldt, R. A., Leamon, R. J., R. A. Mewaldt, B. J. Thompson, de Toma, G, G. de Toma, de Toma, G., Gibson, S. E., McIntosh, S., Webb, D., Y. Elsworth, Elsworth, Yvonne, Leamon, RJ, Gibson, SE, Emery, B, S. E. Gibson, Emery, B., J. Lei, P. Riley, Zhao, L, S. McIntosh, Riley, P, B. Emery, D. Webb, Elsworth, Y., Thompson, BJ, Zhao, L., Thompson, B. J., R. J. Leamon, Mewaldt, RA, L. Zhao   +35 more
core   +1 more source

Multispacecraft Energetic Particle Enhancements Associated with a Single Corotating Interaction Region

The Astrophysical Journal
The radial evolution of particles accelerated at corotating interaction regions (CIRs) is not fully understood, particularly the distance range over which this particle acceleration occurs and how the energy spectra are modulated by transport through the
M. J. Starkey, M. A. Dayeh, M. I. Desai, R. Bučík, S. T. Hart, H. A. Elliott   +5 more
doaj   +1 more source

The Magnetic Connectivity of the Sun to the Heliosphere

, 2010
A prime research focus of the upcoming Solar Probe Plus and Solar Orbiter missions will be to determine how the heliospheric magnetic field and plasma connect to the Sun's corona and photosphere.
Antiochos, S. K.
core   +1 more source

Solar Dynamics and Its Effects on the Heliosphere and Earth

, 2006
The SOHO and Cluster missions form a single ESA cornerstone. Yet they observe very different regions in our solar system: the solar atmosphere on one hand and the Earth’s magnetosphere on the other.
Schwenn,R., Klecker,B., Baker, D. N., Schwenn, R., Klecker, B., Schwartz, S. J., Klecker, B, Steiger, R, Steiger,R.Von, Schwartz, S. J, Schwartz,S.J., Schwenn, R, von Steiger, R., Baker,D.N., Baker, D. N   +14 more
core   +1 more source

An Empirical Model of Energetic Neutral Atom Imaging of the Heliosphere and Its Implications for Future Heliospheric Missions at Great Heliocentric Distances [PDF]

, 2019
Several concepts for heliospheric missions operating at heliocentric distances far beyond Earth orbit are currently investigated by the scientific community.
Barabash, S., Wurz, Peter, Fichtner, H., Futaana, Y., Galli, André   +4 more
core   +1 more source

A predicted small and round heliosphere [PDF]

, 2018
The shape of the solar wind bubble within the interstellar medium, the so-called heliosphere, has been explored over six decades(1-7). As the Sun moves through the surrounding partially-ionized medium, neutral hydrogen atoms penetrate the heliosphere ...
Loeb, Abraham, Opher, Merav, Drake, J.F., Toth, Gabor   +3 more
core  

Mapping Our Path through the Local Interstellar Medium: High-resolution Ultraviolet Absorption Spectroscopy of Sight Lines along the Sun’s Historical Trajectory

The Astrophysical Journal
Using high-resolution UV data obtained from the Space Telescope Imaging Spectrograph on board the Hubble Space Telescope, we focus on eight sight lines along the Sun’s historical trajectory to reconstruct the morphology of our most recent interstellar ...
Hunter Vannier, Seth Redfield, Brian E. Wood, Hans-Reinhard Müller, Jeffrey L. Linsky, Priscilla C. Frisch   +5 more
doaj   +1 more source

Characterizing the Impact of Alfvén Wave Forcing in Interplanetary Space on the Distribution of Near-Earth Solar Wind Speeds

The Astrophysical Journal Letters
Broadly, solar wind source regions can be classified by their magnetic topology as intermittently and continuously open to the heliosphere. Early models of solar wind acceleration do not account for the fastest, nontransient solar wind speeds observed ...
B. L. Alterman
doaj   +1 more source

A slow coronal mass ejection with rising X-ray source

, 2005
An eruptive event, which occurred on 16th April 2002, is discussed. Using images from the Transition Region and Coronal Explorer ( TRACE) at 195 angstrom, we observe a lifting flux rope which gives rise to a slow coronal mass ejection ( CME).
Harra, LK, Mandrini, CH, van Driel-Gesztelyi, L, Matthews, SA, Goff, CP   +4 more
core  

Magnetic Connectivity in the Time-dependent Corona and Heliosphere

The Astrophysical Journal Letters
Magnetic flux fills the heliosphere, expands outward from the solar corona, and is fundamentally related to the structure and dynamics of the solar corona and solar wind.
Roberto Lionello, Cooper Downs, Emily I. Mason, Jon A. Linker, Pete Riley, Mathew J. Owens   +5 more
doaj   +1 more source