Results 191 to 200 of about 10,278 (236)

Connecting energetic electrons at the Sun and in the heliosphere through X-ray and radio diagnostics [PDF]

David Paipa-Leon, Nicole Vilmer, M. Maksimović, Vratislav Krupař, A. Vecchio   +4 more
openalex   +1 more source

NASA Sun-Earth Connections Theory Program: The Structure and Dynamics of the Solar Corona and Inner Heliosphere

, 2013
Z. Mikić, J. M. Grebowsky
openalex   +1 more source

Properties of Magnetic Switchbacks in the Near-Sun Solar Wind. [PDF]

Space Sci Rev
Badman ST, Fargette N, Matteini L, Agapitov OV, Akhavan-Tafti M, Bale SD, Bharati Das S, Bizien N, Bowen TA, Dudok de Wit T, Froment C, Horbury T, Huang J, Jagarlamudi VK, Larosa A, Madjarska MS, Panasenco O, Pariat E, Raouafi NE, Rouillard AP, Ruffolo D, Sioulas N, Soni SL, Sorriso-Valvo L, Suen GHH, Velli M, Verniero J.   +26 more
europepmc   +1 more source

Multispacecraft Observations of the 2024 September 9 Backside Solar Eruption That Resulted in a Sustained Gamma Ray Emission Event. [PDF]

Sol Phys
Gopalswamy N, Mäkelä P, Akiyama S, Xie H, Yashiro S, Bale SD, Wimmer-Schweingruber RF, Kühl P, Krucker S.   +8 more
europepmc   +1 more source

Polarity-resolved far-side magnetograms based on helioseismic measurements. [PDF]

Sci Rep
Hamada A, Jain K, Strecker H, Lindsey C, Suárez DO.   +4 more
europepmc   +1 more source

Evidence for small-scale torsional Alfvén waves in the solar corona. [PDF]

Nat Astron
Morton RJ, Gao Y, Tajfirouze E, Tian H, Van Doorsselaere T, Schad TA.   +5 more
europepmc   +1 more source

Alfvén waves in the solar corona: resonance velocity, damping length, and charged particles acceleration by kinetic Alfvén waves. [PDF]

Sci Rep
Ayaz S, Zank GP, Khan IA, Li G, Rivera YJ.   +4 more
europepmc   +1 more source

Synergetic observations of the Sun and heliosphere with Solar Orbiter/Metis and Parker Solar Probe

Daniele Telloni
openalex   +1 more source

The importance of boundary evolution for solar-wind modelling. [PDF]

Sci Rep
Owens MJ, Barnard L, Arge CN.
europepmc   +1 more source

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The Sun and Heliosphere at Solar Maximum

Science, 2003
Recent Ulysses observations from the Sun's equator to the poles reveal fundamental properties of the three-dimensional heliosphere at the maximum in solar activity. The heliospheric magnetic field originates from a magnetic dipole oriented nearly perpendicular to, instead of nearly parallel to, the Sun's rotation axis.
R G Marsden, J Geiss, D J McComas
exaly   +5 more sources