Results 131 to 140 of about 438 (164)

Psyche Mission Description and Design Rationale. [PDF]

Space Sci Rev
Polanskey CA, Elkins-Tanton LT, Bell JF, Alonge EK, Bairstow SH, Binzel RP, Biswas A, Bury L, Cisneros E, Han D, Jun I, Klipstein WM, Lawrence DJ, McCoy TJ, Mastrodemos N, Merayo JMG, Noble SK, Oh DY, Oran R, Ortega CA, Park RS, Peplowski PN, Prettyman TH, Rayman MD, Ream JB, Roatsch T, Weise TM, Wenkert DD, Weiss BP, Zuber MT.   +29 more
europepmc   +1 more source

Different Behavior of Density Perturbations Between Dayside and Nightside in the Martian Thermosphere and the Ionosphere Associated With Atmospheric Gravity Waves. [PDF]

J Geophys Res Space Phys
Nakagawa H, England SL, Kumar A, Benna M, Harada Y, Sakai S, Terada N, Seki K, Yoshida N.   +8 more
europepmc   +1 more source

Atacama Large Aperture Submillimeter Telescope (AtLAST) science: Probing the transient and time-variable sky. [PDF]

Open Res Eur
Orlowski-Scherer J, Maccarone T, Bright J, Kamiński T, Koss M, Mohan A, Miguel Montenegro-Montes F, Næss S, Ricci C, Severgnini P, Stanke T, Vignali C, Wedemeyer S, Booth M, Cicone C, Di Mascolo L, Johnstone D, Mroczkowski T, Cordiner M, Greiner J, Hatziminaoglou E, van Kampen E, Klaassen P, Lee M, Liu D, Saintonge A, Smith M, Thelen A.   +27 more
europepmc   +1 more source

GOES-R Series X-Ray Sensor (XRS): 1. Design and Pre-Flight Calibration. [PDF]

J Geophys Res Space Phys
Woods TN, Eden T, Eparvier FG, Jones AR, Woodraska DL, Chamberlin PC, Machol JL.   +6 more
europepmc   +1 more source

Interstellar Mapping And Acceleration Probe: The NASA IMAP Mission. [PDF]

Space Sci Rev
McComas DJ, Christian ER, Schwadron NA, Gkioulidou M, Allegrini F, Baker DN, Bzowski M, Clark G, Cohen CMS, Cohen I, Collura C, Cully MJ, Dalla S, Desai MI, Driesman A, Eng D, Fox NJ, Funsten HO, Fuselier SA, Galli A, Giacalone J, Hahn J, Hegarty KP, Horbury T, Horanyi M, Kistler LM, Kubiak MA, Kubota S, Livi S, Lugaz N, Lee CO, Luhmann J, Matthaeus W, Mitchell DG, Mitchell JG, Moebius E, Pope S, Provornikova E, Rankin JS, Reisenfeld DB, Reno C, Richardson JD, Russell CT, Shaw-Lecerf MM, Scherrer J, Skoug RM, Shen MM, Spence HE, Sternovsky Z, Strumik M, Szalay JR, Tapley M, Tokumaru M, Turner DL, Weidner S, Westlake J, Wurz P, Zank GP.   +57 more
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Oscillations of coronal loops and second pulsations of solar radio emission

Astronomy Letters, 2007
The dispersion properties of the sausage eigenmodes of oscillations in a thin magnetic flux tube are numerically analyzed in terms of ideal magnetohydrodynamics (MHD). The period of the modes accompanied by the emission of MHD waves into the surrounding medium, which leads to acoustic damping of oscillations, is determined by the radius of the tube ...
Yulia Kopylova, Yu T Tsap, Melnikov A V
exaly   +2 more sources

Unusually low coronal radio emission at the solar minimum

Solar Physics, 1992
We present two-dimensional observations of the quiet Sun at 73.8, 50.0, and 38.5 MHz obtained with the Clark Lake Radioheliograph during the sunspot minimum period of September 1986. The observed peak brightness temperatures during the entire period of sunspot minimum are found to be extremely low, lying in the range (0.6 × 105 K − 2.5 × 105 K).
G. Thejappa, M. R. Kundu
openaire   +1 more source

Statistical Links between Solar Cosmic Rays, Type-II Radio Emission, and Coronal Mass Ejections

Geomagnetism and Aeronomy, 2021
Type-II radio emission often accompanies events in solar cosmic rays and is an indicator of the propagation of a shock wave in the solar corona. Conversely, the shock wave associated with coronal mass ejections plays an important role in the acceleration of solar protons.
G. A. Bazilevskaya, Yu. I. Logachev, E. I. Daibog, N. A. Vlasova, E. A. Ginzburg, V. N. Ishkov, L. L. Lazutin, M. D. Nguyen, G. M. Surova, O. S. Yakovchuk   +9 more
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Density Depletion in a Coronal Flux Tube Associated With Solar Radio Emission

Solar Physics, 2006
A discussion, which is motivated by recent study of solar radio emission, is presented to address the issue under what conditions the depletion of plasma density in a flux tube in the corona may take place. Two particular situations are of interest: One is that density is depleted due to the presence of beams of energetic particles, and the other is ...
C. S. Wu, C. B. Wang, Q. M. Lu
openaire   +1 more source