Search Publications

Solar magnetic feature detection and tracking for space weather monitoring
DOI: 10.1016/j.asr.2010.06.024 Bibcode: 2011AdSpR..47.2105H

Bloomfield, D. S.; Gallagher, P. T.; McAteer, R. T. J. +1 more

We present an automated system for detecting, tracking, and cataloging emerging active regions throughout their evolution and decay using SOHO Michelson Doppler Interferometer (MDI) magnetograms. The SolarMonitor Active Region Tracking (SMART) algorithm relies on consecutive image differencing to remove both quiet-Sun and transient magnetic featur…

2011 Advances in Space Research
SOHO 66
Ion- and electron-acoustic solitons and double layers in multi-component space plasmas
DOI: 10.1016/j.asr.2010.12.013 Bibcode: 2011AdSpR..47.1558L

Lakhina, G. S.; Singh, S. V.; Kakad, A. P.

A general model for the ion- and electron-acoustic solitons and double layers in a multi-component unmagnetized plasma consisting of background electrons, counter-streaming electron beams and ions is discussed. The model is based on the multi-fluid equations and the Poisson equation, and uses the Sagdeev pseudo-potential techniques. For identical …

2011 Advances in Space Research
Cluster 57
Time-dependent cosmic ray modulation
DOI: 10.1016/j.asr.2010.12.007 Bibcode: 2011AdSpR..47.1529M

Ferreira, S. E. S.; Potgieter, M. S.; Engelbrecht, N. E. +2 more

Time-dependent cosmic ray modulation is calculated over multiple solar cycles using our well established two-dimensional time-dependent modulation model. Results are compared to Voyager 1, Ulysses and IMP cosmic ray observations to establish compatibility. A time-dependence in the diffusion and drift coefficients, implicitly contained in recent ex…

2011 Advances in Space Research
Ulysses 33
An overview of RADOM results for earth and moon radiation environment on Chandrayaan-1 satellite
DOI: 10.1016/j.asr.2011.05.009 Bibcode: 2011AdSpR..48..779D

Girish, V.; Vadawale, S. V.; Goswami, J. N. +5 more

The RADiatiOn Monitor (RADOM) is a miniature dosimeter-spectrometer that flew onboard the Chandrayaan-1 lunar mission in order to monitor the local radiation environment. Primary objective of the RADOM experiment was to measure the total absorbed dose, flux of surrounding energetic particles and spectrum of the deposited energy from high energy pa…

2011 Advances in Space Research
Chandrayaan-1 22
Coronal mass ejection detection using wavelets, curvelets and ridgelets: Applications for space weather monitoring
DOI: 10.1016/j.asr.2010.03.028 Bibcode: 2011AdSpR..47.2118G

Gallagher, P. T.; Young, C. A.; McAteer, R. T. J. +1 more

Coronal mass ejections (CMEs) are large-scale eruptions of plasma and magnetic field that can produce adverse space weather at Earth and other locations in the Heliosphere. Due to the intrinsic multiscale nature of features in coronagraph images, wavelet and multiscale image processing techniques are well suited to enhancing the visibility of CMEs…

2011 Advances in Space Research
SOHO 15
Actors of the main activity in large complex centres during the 23 solar cycle maximum
DOI: 10.1016/j.asr.2011.02.001 Bibcode: 2011AdSpR..47.2081S

Mandrini, C. H.; Schmieder, B.; Molodij, G. +10 more

During the maximum of Solar Cycle 23, large active regions had a long life, spanning several solar rotations, and produced large numbers of X-class flares and CMEs, some of them associated to magnetic clouds (MCs). This is the case for the Halloween active regions in 2003. The most geoeffective MC of the cycle (Dst = -457) had its source during th…

2011 Advances in Space Research
SOHO 13
Simulation of cometary jets in interaction with the solar wind
DOI: 10.1016/j.asr.2011.05.024 Bibcode: 2011AdSpR..48.1108W

Glassmeier, K. -H.; Koenders, C.; Motschmann, U. +3 more

The influence of cometary jets on the solar wind interaction is studied with a 3D hybrid simulation. Anisotropic outgassing patterns were until recently not considered in cometary simulations, despite strong anisotropies found at observations. Comet 67P Churyumov-Gerasimenko, the target of the ROSETTA mission, was chosen as a case study for a simu…

2011 Advances in Space Research
Rosetta 13
Unusually strong magnetic fields in Titan's ionosphere: T42 case study
DOI: 10.1016/j.asr.2011.02.009 Bibcode: 2011AdSpR..48..314W

Coates, A. J.; Russell, C. T.; Wei, H. Y. +7 more

Observations of unusually large magnetic fields in the ionosphere indicate periods of maximum stress on Titan's ionosphere and potentially of the strongest loss rates of ionospheric plasma. During Titan flyby T42, the observed magnetic field attained a maximum value of 37 nT between an altitude of 1200 and 1600 km, about 20 nT stronger than on any…

2011 Advances in Space Research
Cassini 11
Kink-like mode of a double gradient instability in a compressible plasma current sheet
DOI: 10.1016/j.asr.2011.07.008 Bibcode: 2011AdSpR..48.1531K

Korovinskiy, D. B.; Semenov, V. S.; Erkaev, N. V. +4 more

A linear MHD instability of the electric current sheet, characterized by a small normal magnetic field component, varying along the sheet, is investigated. The tangential magnetic field component is modeled by a hyperbolic function, describing Harris-like variations of the field across the sheet. For this problem, which is formulated in a 3D domai…

2011 Advances in Space Research
Cluster 9
Background and pickup ion velocity distribution dynamics in Titan's plasma environment: 3D hybrid simulation and comparison with CAPS T9 observations
DOI: 10.1016/j.asr.2011.05.026 Bibcode: 2011AdSpR..48.1114L

Hartle, R. E.; Sittler, E. C.; Cooper, J. F. +2 more

In this report we discuss the ion velocity distribution dynamics from the 3D hybrid simulation. In our model the background, pickup, and ionospheric ions are considered as a particles, whereas the electrons are described as a fluid. Inhomogeneous photoionization, electron-impact ionization and charge exchange are included in our model. We also tak…

2011 Advances in Space Research
Cassini 9