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Characteristic magnetic field and speed properties of interplanetary coronal mass ejections and their sheath regions
Owens, M. J.; Crooker, N. U.; Siscoe, G. L. +2 more
Prediction of the solar wind conditions in near-Earth space, arising from both quasi-steady and transient structures, is essential for space weather forecasting. To achieve forecast lead times of a day or more, such predictions must be made on the basis of remote solar observations. A number of empirical prediction schemes have been proposed to fo…
An HST Search for Supernovae Accompanying X-Ray Flashes
Cenko, S. B.; Peterson, B. A.; Price, P. A. +24 more
We present the results from a Hubble Space Telescope ACS search for supernovae associated with X-ray flashes 020903, 040701, 040812, and 040916. We find strong evidence that XRF 020903 (z=0.25) was associated with a SN 1998bw-like supernova and confirm this using optical spectroscopy at t~25 days. We find no evidence, however, for SN 1998bw-like s…
Contribution of nonadiabatic ions to the cross-tail current in an O+ dominated thin current sheet
Lundin, R.; Balogh, A.; Klecker, B. +8 more
During storm times, O+ can dominate both the pressure and the density in the plasma sheet. Because of the contribution from ion outflow, the plasma sheet is already oxygen-rich prior to substorm onset. At substorm onset the fraction of O+ contributing to the pressure and density increases. In the O+ dominated thin …
Global structure of Jupiter's magnetospheric current sheet
Khurana, Krishan K.; Schwarzl, Hannes K.
Jupiter's magnetosphere contains a gigantic sheet-like structure located near its dipole magnetic equator that contains most of the plasma and energetic particles swirling in Jupiter's magnetosphere. Called the "current sheet," it behaves like a rigid structure inside a radial distance of ∼50 RJ where the periodic reversals of the B
Kelu-1 Is a Binary L Dwarf: First Brown Dwarf Science from Laser Guide Star Adaptive Optics
Leggett, S. K.; Liu, Michael C.
We present near-infrared (1-2.4 µm) imaging of the L dwarf Kelu-1 obtained with the Keck sodium laser guide star adaptive optics (LGS AO) system as part of a high angular resolution survey for substellar binaries. Kelu-1 was one of the first free-floating L dwarfs identified, and the origin of its overluminosity compared to objects of simila…
Magnetic Reconnection Rate and Flux-Rope Acceleration of Two-Ribbon Flares
Lin, Jun; Xu, Yan; Qiu, Jiong +3 more
Forbes & Lin derived simple equations to link the properties of magnetic reconnection in the corona to observed signatures of solar flares. We measured the photospheric magnetic fields and the flare ribbon separation speeds then applied these equations to derive two physical terms for the magnetic reconnection rates: the rate of magnetic flux …
A spectroscopic study of the surfaces of Saturn's large satellites: H 2O ice, tholins, and minor constituents
Emery, Joshua P.; Cruikshank, Dale P.; Owen, Tobias C. +7 more
We present spectra of Saturn's icy satellites Mimas, Enceladus, Tethys, Dione, Rhea, and Hyperion, 1.0-2.5 µm, with data extending to shorter (Mimas and Enceladus) and longer (Rhea and Dione) wavelengths for certain objects. The spectral resolution ( R=λ/Δλ) of the data shown here is in the range 800-1000, depending on the specific instrumen…
The Magnetosheath
Sahraoui, F.; Lucek, E. A.; Walker, S. N. +5 more
Detection of Ne VIII in the Low-Redshift Warm-Hot Intergalactic Medium
Tripp, Todd M.; Sembach, Kenneth R.; Savage, Blair D. +2 more
High-resolution FUSE and STIS observations of the bright QSO HE 0226-4110 (zem=0.495) reveal the presence of a multiphase absorption-line system at zabs(OVI)=0.20701 containing absorption from H I (Lyα to Lyθ), C III, O III, O IV, O VI, N III, Ne VIII, Si III, S VI, and possibly S V. Single-component fits to the Ne VIII and O…
Weak-Lensing Analysis of the z~=0.8 Cluster CL 0152-1357 with the Advanced Camera for Surveys
Ford, H. C.; Demarco, R.; Rosati, P. +5 more
We present a weak-lensing analysis of the X-ray-luminous cluster CL 0152-1357 at z~=0.84 using Hubble Space Telescope/Advanced Camera for Surveys (ACS) observations. The unparalleled resolution and sensitivity of ACS enable us to measure weakly distorted, faint background galaxies to the extent that the number density reaches ~175 arcmin-2