Protected mode

Known as: Protected virtual address mode, Pmode, 386 Enhanced Mode 
In computing, protected mode, also called protected virtual address mode, is an operational mode of x86-compatible central processing units (CPUs… (More)
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50 relations
3 GB barrier32-bitAddress spaceBIOS
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2011
2011
Modelling solar irradiance variability on time scales from minutes to months
We analyze and model total solar irradiance variability on time scales from minutes to months, excluding variations due to p-mode… (More)
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2010
2010
UNUSUAL TRENDS IN SOLAR P-MODE FREQUENCIES DURING THE CURRENT EXTENDED MINIMUM
Received ; accepted – 2 – ABSTRACT We investigate the behavior of the intermediate-degree mode frequencies of the sun during the… (More)
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2009
2009
Physical fractionation of soil organic matter : Destabilization of deep soil carbon following harvesting of a temperate coniferous forest
[1] Developing a better understanding of the processes involved in controlling soil carbon (C) storage and turnover in native… (More)
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2005
2005
Ant-aphid interactions in multispecies ant communities: Some ecological and ethological aspects
Investigations of the interactions between aphids and ants in multispecies ant communities and an experimental investigation of… (More)
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2004
2004
Implications of habitat choice for protected polymorphisms
In this paper, we re-examine how heterogeneous environments can enable protected polymorphisms. Building on the classical models… (More)
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2001
2001
VEGETATION MAPPING AND CLASSIFICATION IN MADAGASCAR ( USING GIS ) : IMPLICATIONS AND RECOMMENDATIONS FOR THE CONSERVATION OF BIODIVERSITY
A map of the ‘Remaining Primary Vegetation’ in Madagascar has been derived (Map 1) and divided into broad vegetation zones. It is… (More)
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2001
2001
Density discontinuity of a neutron star and gravitational waves
Gravitational wave interferometers such as LIGO, VIRGO, GEO600, and TAMA300 on earth, and LISA in space [1] are almost ready to… (More)
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1999
1999
How much do helioseismological inferences depend upon the assumed reference model ?
We investigate systematic uncertainties in determining the proÐles of the solar sound speed, density, and adiabatic index using… (More)
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1998
1998
Towards gravitational-wave asteroseismology
We present new results for pulsating neutron stars. We have calculated the eigenfrequencies of the modes that one would expect to… (More)
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1997
1997
Properties of Sun-like Stars with Planets: ρ1 Cancri, τ Bootis, and υ Andromedae
  • Sallie L. Baliunas, Gregory W. Henry, Robert Andrew Donahue, Francis C. Fekel, Willie Soon
  • 1997
Radial velocity variations have revealed planets orbiting 51 Peg, 47 UMa, and 70 Vir, and a low-mass companion orbiting HD 114762… (More)
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