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Related papers: Using Early Data to Illuminate the Pioneer Anomaly

200 papers

It is introduced a hypothesis that the gravitational potential in the universe changes linearly with the time. This enables to explain the Hubble red shift and the anomalous acceleration of Pioneer 10 and 11.

General Relativity and Quantum Cosmology · Physics 2007-05-23 Kostadin Trencevski

We use broadband sensitive LOFAR observations in the 25-80 MHz frequency range to study the single-pulse emission properties of the mode-switching pulsar B0943+10. We review the derivation of magnetospheric geometry, originally based on…

Solar and Stellar Astrophysics · Physics 2018-09-05 Anna Bilous

We illustrate the energy transfer during planetary flybys as a function of time using a number of flight mission examples. The energy transfer process is rather more complicated than a monotonic increase (or decrease) of energy with time.…

Astrophysics · Physics 2008-11-26 John D. Anderson , James K. Campbell , Michael Martin Nieto

We present XMM-Newton and Chandra observations of 1E1048.1-5937, being the first to show evidence for a significant variation in the X-ray luminosity of this Anomalous X-ray Pulsar (AXP). While during the first XMM-Newton (2000 December)…

Astrophysics · Physics 2009-11-10 S. Mereghetti , A. Tiengo , L. Stella , G. L. Israel , N. Rea , S. Zane , T. Oosterbroek

We present CO(2-1), $^{13}$CO(2-1), CO(6-5), CO(7-6), and SO(6$_5-5_4$) line observations made with the {\it IRAM 30 m} and {\it APEX} radiotelescopes and the {\it Submillimeter Array} toward the highly collimated and extended southwest…

Astrophysics of Galaxies · Physics 2015-05-13 Luis A. Zapata , Johannes Schmid-Burgk , Dirk Muders , Peter Schilke , Karl Menten , Rolf Guesten

Drift-pair bursts are an unusual type of solar low-frequency radio emission, which appear in the dynamic spectra as two parallel drifting bright stripes separated in time. Recent imaging spectroscopy observations allowed for the…

Solar and Stellar Astrophysics · Physics 2020-07-30 Alexey A. Kuznetsov , Nicolina Chrysaphi , Eduard P. Kontar , Galina Motorina

Electron beams accelerated in solar flares and escaping from the Sun along open magnetic field lines can trigger intense radio emissions known as type III solar radio bursts. Utilizing observations by Parker Solar Probe (PSP), STEREO-A…

Solar and Stellar Astrophysics · Physics 2025-10-02 Francesco Azzollini , Eduard P. Kontar

In this letter, we address the question of whether the almost four standard deviations difference between theory and experiment for the muon anomalous magnetic moment $a_\mu$ can be explained as a higher-order Standard Model perturbation…

High Energy Physics - Phenomenology · Physics 2019-10-16 Francisco Campanario , Henryk Czyż , Janusz Gluza , Tomasz Jeliński , Germán Rodrigo , Szymon Tracz , Dmitry Zhuridov

We present new results from high sensitivity GMRT observations of PSR B0826-34. We provide a model to explain the observed subpulse drift properties of this pulsar, including the apparent reversals of the drift direction. In this model, PSR…

Astrophysics · Physics 2009-11-10 Y. Gupta , J. Gil , J. Kijak , M. Sendyk

In 1933 Dayton Miller published in this journal the results of his voluminous observations using his ether drift interferometer, and proclaimed that he had determined the "absolute motion of the earth". This result is in direct conflict…

Classical Physics · Physics 2007-05-23 Thomas J. Roberts

The anomalous X-ray pulsars (AXPs) represent a growing class of neutron stars discovered at X-ray energies. While the nature of their multi-wavelength emission mechanism is still under debate, evidence has been recently accumulating in…

Astrophysics · Physics 2009-11-10 Samar Safi-Harb , Jennifer West

Observations from the Atmospheric Imaging Assembly (AIA) onboard the Solar Dynamics Observatory (SDO) reveal ubiquitous episodic outflows (jets) with an average speed around 120 km s-1 at temperatures often exceeding a million degree in…

Solar and Stellar Astrophysics · Physics 2011-07-27 Hui Tian , Scott W. McIntosh , Shadia Rifal Habbal , Jiansen He

We measure the mean frequencies of acoustic waves propagating toward and away from a sunspot employing a spot-centered Fourier-Hankel decomposition of p-mode amplitudes as measured from a set of observations made at the South Pole in 1991.…

Astrophysics · Physics 2007-05-23 D. C. Braun , Y. Fan , C. Lindsey , S. M. Jefferies

I review recent observational progress on Anomalous X-ray Pulsars, with an emphasis on timing, variability, and spectra. Highlighted results include the recent timing and flux stabilization of the notoriously unstable AXP 1E 1048.1-5937,…

Astrophysics · Physics 2008-11-26 V. M. Kaspi

Polar corona is often explored to find the energy source for the acceleration of the fast solar wind. Earlier observations show omni-presence of quasi-periodic disturbances, travelling outward, which is believed to be caused by the…

Solar and Stellar Astrophysics · Physics 2011-02-16 S. Krishna Prasad , D. Banerjee , G. R. Gupta

We show that the time-dependent Doppler effect should induce measureable deviations of the time history of the projected orbit of a star around the supermassive black hole in the Galactic center (SgrA*) from the expected Keplerian history.…

Astrophysics · Physics 2007-05-23 Abraham Loeb

Tidal distension of spacecraft electronics due to spin and solar and galactic gravitation elegantly explains all variations in the anomaly reported by Anderson et al. Contrary to their conclusion, a constant residue seems to be present in…

Astrophysics · Physics 2007-05-23 V Guruprasad

Recently several long-period radio transients have been discovered, with strongly polarised coherent radio pulses appearing on timescales between tens to thousands of seconds [1,2]. In some cases the radio pulses have been interpreted as…

Several spacecrafts show an anomalous flyby. In a previous paper a non-prefered reference frame is studied moving uniformly relative to the prefered one. In this article the Doppler frequency residual is derived. The prefered reference…

General Physics · Physics 2011-09-28 Walter Petry

Three-dimensional (3-D) dynamical models of hot Jupiter atmospheres predict very strong wind speeds. For tidally locked hot Jupiters, winds at high altitude in the planet's atmosphere advect heat from the day side to the cooler night side…

Earth and Planetary Astrophysics · Physics 2015-05-30 Eliza Miller-Ricci Kempton , Emily Rauscher