India-u.s. continue cooperative space research news release no. 64-19
Equatorial electrojet investigation by sounding rockets with magnetometer
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Equatorial electrojet investigation by sounding rockets with magnetometer
Toroidal ring current system indicated by data from magnetometer aboard Explorer VI SATELLITE
Measurement of magnetic fields on moon surface using proton magnetometer from unmanned vehicle
Radiation, passive, magnetometer, meteorite flux, and solar-cell damage experiments by lunar- anchored satellite
Hydromagnetic radiation modulation and sampling telemetry - electromagnetic signal detection by magnetometer from spacecraft
Room sized magnetic shield system for evaluation of magnetometers
Magnetic shields of Mumetal for magnetometer sensors of Mariner Mars spacecraft
Earth geomagnetic core field model construction from land and ocean magnetometer data
Double gas cell rubidium vapor magnetometers in Nike-Apache rockets and ionospheric current detection
Geomagnetic field measurements from rockets using proton magnetometer
Method for demodulating spin-modulated data from magnetometer sensors mounted on spinning satellites
Nike-Apache rocket ionospheric current measurements using rubidium-vapor magnetometer
Nonmagnetic, explosive-actuated indexing device for magnetometer experiment on Pioneer IV SPACE probe flight
Interplanetary magnetic field measurements using flux gate magnetometer sensor mounted on Pioneer VI space probe, noting various graphs
Nonmagnetic, explosive-actuated indexing device for magnetometer experiment aboard Pioneer VI AND VII spacecrafts
Statistical properties of interplanetary magnetic field variations, charged particles propagation in solar system and photospheric processes analyzed, using Mariner II magnetometer
Fluxgate magnetometer for OGO-E spacecraft in observing MHD waves and magnetic field structures in space
Spatial and temporal variability of the magnetic field component induced by ocean circulation is investigated on the basis of a standard thin-shell approximation of electro- and magneto-static equations. Well-known difficulties of numerical solution of the governing equations are resolved by reducing the problem to an equation for the electric field potential,(ef) as opposed to a more conventional approach focused on the vertical jump, (psi), of the magnetic field potential across a combined ocean/ marine-sediment-layer spherical shell. The present formulation permits using more realistic input data on ocean currents and ultimately yields much greater (by at least an order of magnitude) values of the magnetic field at sea surface than predicted in earlier studies. Such large values are comparable to, and in some cases exceed, magnetic field variations caused by lithospheric and ionospheric sources on monthly to interannual timescales. At the 400-km altitude (of CHAMP satellite), the field attains 6 nT. The model predictions show favorable comparisons with some in situ measurements as well as with Challenging Minisatellite Payload (CHAMP) satellite magnetometer data.